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PHOTOELECTRON ANGULAR DISTRIBUTION PARAMETERS FOR ELEMENTS Z=1 TO Z=54 IN THE PHOTOELECTRON ENERGY RANGE 100–5000 eV
Atomic Data and Nuclear Data Tables 77, 97–159 (2001) doi:10.1006/adnd.2000.0849, available online at http://www.idealibrary.com on
PHOTOELECTRON ANGULAR DISTRIBUTION PARAMETERS FOR ELEMENTS Z = 1 TO Z = 54 IN THE PHOTOELECTRON ENERGY RANGE 100–5000 eV M. B. TRZHASKOVSKAYA Petersburg Nuclear Physics Institute, 188300 Gatchina, Russia and V. I. NEFEDOV and V. G. YARZHEMSKY Kurnakov Institute of General and Inorganic Chemistry of the Russian Academy of Sciences, 31 Leninsky, 117907 Moscow, Russia
Parameters of the angular distribution of photoelectrons along with the subshell photoionization cross sections calculated for all subshells of atoms with 1 ≤ Z ≤ 54 are presented in the Table for nine photoelectron energies in the range 100–5000 eV. Relativistic treatment of the photoeffect is used. The calculations have been performed within the quadrupole approximation with the central Dirac–Fock–Slater potential. The hole left by the emitted electron has been taken into account in the framework of the frozen orbital approximation. Applications of nondipolar parameters to photoelectron angular distribution in solids, to quantitative x-ray photoelectron spectroscopy analysis, and to the x-ray standing wave method are discussed. ° 2001 Academic Press C
0092-640X/01 $35.00 C 2001 by Academic Press Copyright ° All rights of reproduction in any form reserved.
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Photoelectron Angular Distribution
CONTENTS INTRODUCTION .................................................................. Method of Calculation........................................................ Applications of Nondipolar Parameters.................................... Photoelectron Angular Distribution in Solids ....................... X-ray Photoelectron Spectroscopy ................................... X-ray Standing Wave Method .........................................
98 100 102 102 103 103
EXPLANATION OF TABLE ..................................................... Example ........................................................................
106 106
TABLE Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 ...................................
107
INTRODUCTION In photoeffect studies it is common to consider the angular distribution of photoelectrons within the electric dipole approximation (see, for example, [1–3] and references given therein). In this case the differential photoionization cross section for circularly polarized and unpolarized photons can be written as ¸ · σi β dσi (1) = 1 − P2 (cos θ ) , dÄ 4π 2
dipole approximation has also been demonstrated in recent experiments [18–20] where the photoionization of Ne, Ar, and Kr has been studied at photoelectron energies E ≤ 3000 eV.
characterized by the energy- and subshell-dependent asymmetry parameter β of the photoelectron angular distribution. Here σi is the photoionization cross section for the ith atomic subshell, P2 (cos θ ) is the second order Legendre polynomial, and θ is the angle between the vectors of photon (k) and photoelectron (p) propagation (Fig. 1). In keeping with Eq. (1), the currently available tables which may be used for estimation of the photoelectron angular distribution contain values of the photoionization cross sections σi and of the dipole parameter β [3–5]. However, there exist many investigations [6–17] where the angular distribution has been shown to differ significantly from that calculated within the dipole approximation, even for low photoelectron kinetic energies just above the photoionization threshold. In [6–11] the influence of quadrupole terms on the angular distribution has been studied using a nonrelativistic treatment of the photoeffect. Relativistic calculations have been carried out for a number of atoms using the quadrupole approximation [14, 15] as well as taking into account all multipoles of the radiation field [12, 13]. The breakdown of the
FIG. 1. Angles and directions. k and p represent the photon and photoelectron directions, respectively, ε gives the photon polarization direction, and S the direction normal to the solid taget.
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Photoelectron Angular Distribution
The angular distribution parameters have been calculated in the quadrupole approximation. The subshell photoionization cross sections σi have been computed including all multipoles L of the radiation field. Advantage has been taken of experimental values of the electron binding energies [27–29]. The electron wavefunctions have been computed by the use of the central Dirac–Fock–Slater (DFS) potential [30, 31] with allowance made for the hole in the atomic subshell from which an electron has been emitted. It is well known that relativistic effects may change the calculated photoelectron angular distribution parameters even at low energies. As shown in Refs. [14, 15, 32], the β parameter for s shells, which is equal to 2 within the nonrelativistic approximation, may differ considerably from this value. For outer s shells of heavy atoms, the parameter β obtained in relativistic calculations changes drastically with energy, even reversing sign near the photoionization threshold. As to the nondipolar parameters γ and δ, the comparison of our DFS results with nonrelativistic calculations [9] obtained by the use of the Hartree–Fock–Slater potential shows that the difference may also be substantial. The present relativistic parameters γ and δ for the 4s, 4 p, and 3d shells of Xe are listed in Table A along with the nonrelativistic values from [9]. In both works, the atomic model based on the statistical consideration of the exchange has been used. We present in this Table relativistic calculations for two cases: without regard for the hole (nh) and with allowance made for the hole (h). As is obvious from Table A, there is a large difference between relativistic values γ (R) and nonrelativistic values γ (NR) for the 3d shell in the energy range E < ∼ 500 eV. For the 4s shell the parameter γ (R) differs from γ (NR) appreciably, occasionally by several multiples, at energies E > ∼ 1000 eV. For the 4 p shell the parameters δ(R) and δ(NR), even though small in magnitude, differ from one another by several multiples over the entire energy range considered. It should also be pointed out that at energies E < ∼ 100 eV there is a significant discrepancy between the relativistic values of γ (R) obtained for the 4 p and 3d shells with and without regard for the hole (see Table A and Refs. [14, 15]). The peculiarities of the angular distribution parameters for different shells of atoms with different Z have been studied in [12, 14, 15]. The energy dependence of the parameters may be seen from Fig. 2, where the values of β and γ , as well as the values of δ multiplied by 10, are plotted for the 1s, 2 p3/2 , 3d5/2 , 4d5/2 , 5s, and 5 p3/2 shells of Xe over a wide energy range 5 eV ≤ E ≤ 50,000 eV. As indicated in Fig. 2, the nondipolar parameter γ is comparable in magnitude with the dipole parameter β in some energy regions; occasionally, |γ | > |β|. The small parameter δ increases considerably at energies E > ∼ 10,000 eV for p and d shells. Of special interest
In Ref. [9], simple expressions have been presented which describe adequately the angular distribution in various cases of photon polarization by the use of two additional nondipolar parameters γ and δ along with the dipole parameter β. According to Ref. [9], the photoelectron angular distribution for circular polarized and unpolarized photons may be written as µ ¶ · ¸ γ σi β dσi = 1− P2 (cos θ ) + sin2 θ + δ cos θ . (2) dÄ 4π 2 2 For linearly polarized photons the angular distribution may be represented as σi dσi = [1 + β P2 (cos θ) + (δ + γ cos2 θ) sin θ cos ϕ], dÄ 4π (3) where θ is the angle between the vector p and the photon polarization direction ε, the vector ε being coincident with the z axis; ϕ is the angle between the vector k and the plane passing through the z axis and the vector p. The angular distribution for the case of partially polarized photons is [21] ½ σi β 3 3 dσi = 1+ + Pβ cos 2θ + (P −1)β sin2 θ cos2 ϕ dÄ 4π 4 4 4 ¸ ¾ ½ · (P − 1) (1 − sin2 θ cos2 ϕ) + δ + γ P cos2 θ − 2 ¾ × sin θ cos ϕ , (4) where P is the fraction of photons polarized in the z direction. Calculations of the nondipolar parameters γ and δ have been performed only for several atoms. The atomic potential based either on the approximate consideration of the electron exchange interaction [7–13] or on the exact treatment of the exchange [6, 14, 15] has been used. The electron correlation effects have been considered in the framework of the random phase approximation for Ar [22] and Ne [23]. Currently, the most extensive calculations of the nondipolar parameters are given in Refs. [9] and [24] for the noble gases Ne, Ar, Kr, and Xe and in [25] for atoms with atomic numbers 3 ≤ Z ≤ 18. The present work provides the parameters of the photoelectron angular distribution for all elements 1 ≤ Z ≤ 54. The Table contains values of the three angular distribution parameters β, γ , and δ together with the subshell photoionization cross sections σi for nine photoelectron energies in the range 100 eV ≤ E ≤ 5000 eV. Relativistic treatment of the photoeffect [26] has been used. The calculations have been carried out in the one-electron approximation for a free atom. 99
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Photoelectron Angular Distribution
TABLE A
Relativistic (R) and Nonrelativistic (NR) [9] Calculations of the Parameters γ and δ vs Photoelectron Energy, E, for Xe, Z = 54 4s shell
4 p shell
3d shell
E b (NR) = 193 eV E b (4s1/2 ) = 213 eV
E b (NR) = 149 eV E b (4 p1/2 ) = 157 eV, E b (4 p3/2 ) = 147 eV
E b (NR) = 693 eV E b (3d3/2 ) = 689 eV , E b (3d5/2 ) = 676 eV
γ NR E (eV)
γ R
NR
nh
h
100
0.35
0.37
0.37
0.05
200
0.36
0.41
0.38
0.27
500
0.28
0.35
0.32
0.23
1000
0.12
0.19
0.17
0.02
2000
−0.05
−0.01
−0.02
0.03
4000
−0.08
−0.11
−0.10
0.37
5000
−0.01
−0.07
−0.07
0.54
δ R
γ
NR
nh
h
−0.09 −0.08 0.17 0.15 0.22 0.19 0.02 0.00 0.02 0.02 0.38 0.41 0.56 0.61
−0.01 0.00 0.20 0.18 0.19 0.16 0.02 0.00 0.02 0.02 0.38 0.41 0.56 0.61
0.02 0.01 −0.01 −0.01 0.00 0.03 0.04
R
NR
nh
h
0.05 0.05 0.04 0.04 0.01 0.01 0.00 0.00 0.00 0.00 0.01 0.01 0.01 0.02
0.05 0.05 0.03 0.03 0.01 0.01 0.00 0.00 0.00 0.00 0.01 0.01 0.01 0.02
−0.02 −0.04 −0.01 0.16 0.46 0.82 0.93
δ R
NR
nh
h
−0.05 −0.05 −0.09 −0.09 −0.06 −0.05 0.12 0.14 0.49 0.49 0.95 0.94 1.10 1.09
−0.07 −0.07 −0.10 −0.10 −0.06 −0.05 0.14 0.15 0.49 0.50 0.95 0.94 1.10 1.09
−0.01 −0.01 0.02 0.05 0.09 0.17 0.21
R nh
h
0.00 0.00 0.00 0.00 0.03 0.03 0.05 0.05 0.08 0.08 0.13 0.14 0.16 0.17
−0.01 −0.01 0.00 0.00 0.02 0.02 0.05 0.05 0.08 0.08 0.13 0.14 0.16 0.17
Note. E b (NR) is the binding energy given in [9], E b (n`j) is the experimental binding energy used in the present paper. In the relativistic case two values for shells with j = ` − 1/2 (upper) and with j = ` + 1/2 (lower) are listed. Relativistic values are presented for the cases where (i) no allowance is made for the hole (nh), and (ii) the hole is taken into account in the frozen orbital approximation (h).
is the oscillating character of all three curves β(E), γ (E), and δ(E) for outer 5 p3/2 and 4d5/2 shells as well as of γ (E) for the 5s shell. The comparison of our calculations with relativistic computations [24] performed in the independent particle approximation reveals that values of the β, γ , and δ parameters agree to within several percent or better, exclusive of regions where the parameters change rapidly with energy. All oscillatory features like the ones seen in Fig. 2 are usually well reproduced, although the curves may be shifted in energy. These deviations appear to arise from possible differences in the details of the physical assumptions. As discussed in detail in the literature [1, 2, 14, 15, 24], theoretical model assumptions underlying calculations of the photoionization parameters, like a different consideration of the exchange interaction, taking into account the hole, and including the correlation effects, may affect the values of the parameters. The influence of these physical assumptions may be important in two cases: (i) at low photoelectron energies E< ∼ 100 eV and (ii) at those E where a parameter becomes small in magnitude. In these energy regions a more rigorous treatment of photoionization may be required.
Method of Calculation The differential cross section in the ith atomic subshell for circularly polarized and unpolarized photons in the quadrupole approximation can be written as " # 4 X σi dσi = 1+ Bn Pn (cos θ) . dÄ 4π n=1
(5)
We use a relativistic formalism [3, 26] in studies of photoionization. All formulae below are given in relativistic units, in which the Compton wavelength h--/m 0 c is defined as the unit of length, and the electron rest mass m 0 c2 is the unit of energy, that is, h-- = m 0 = c = 1. The subshell photoionization cross section σi in Eq. (5) is defined by the following expression: σi =
4π 2 α X X {(2L + 1)[Q 3=L ,L (κ)]2 k κ L + L[Q 3=L+1,L (κ)]2 + (L + 1)[Q 3=L−1,L (κ)]2 p − 2 L(L + 1)Q 3=L−1,L (κ)Q 3=L+1,L (κ)}. (6)
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Photoelectron Angular Distribution
¤ − 3Q 11 (κ1 )Q 11 (κ2 ) − Q 21 (κ1 )Q 21 (κ2 ) √ £√ + 30W (12 j1 j2 ; 2 ji ) 10Q 01 (κ1 )Q 22 (κ2 ) − Q 11 (κ1 ) √ √ ¤ × [3Q 12 (κ2 ) − 6Q 32 (κ2 )] − 5Q 21 (κ1 )Q 22 (κ2 ) 5 − √ W (22 j1 j2 ; 2 ji )[Q 12 (κ1 )[3Q 12 (κ2 ) 14 √ − 2 6Q 32 (κ2 )] + 5Q 22 (κ1 )Q 22 (κ2 ) ) + 2Q 32 (κ1 )Q 32 (κ2 )] ,
B3 =
B4 = FIG. 2. Photoelectron angular distribution parameters β (solid line), γ (dashed line), and δ × 10 (dot-dashed line) versus photoelectron energy E for Xe.
The coefficients B1 , B2 , B3 , and B4 may be represented as follows: B1 =
B2 =
p 4π 2 α X (−1) j1 + j2 +|κi | |κ1 ||κ2 | C 10 j1 1/2 j2 −1/2 kσi κ1 ,κ2 ¡ ¢© √ × sin δκ1 − δκ2 3 6W (11 j1 j2 ; 1 ji ) √ × [ 2Q 01 (κ1 )Q 11 (κ2 ) + Q 11 (κ1 )Q 21 (κ2 )] √ √ £ + 3 2W (12 j1 j2 ; 1 ji ) Q 01 (κ1 )[ 6Q 12 (κ2 ) √ − 2Q 32 (κ2 )] + 15Q 11 (κ1 )Q 22 (κ2 ) − Q 21 (κ1 ) √ √ ¤ × [ 3Q 12 (κ2 ) − 2Q 32 (κ2 )] √ − 5W (22 j1 j2 ; 1 ji )[ 6 Q 12 (κ1 )Q 22 (κ2 ) ª + 2Q 22 (κ1 )Q 32 (κ2 )] ,
(8)
p 4π 2 α X (−1) j1 + j2 +|κi | |κ1 ||κ2 | C 30 j1 1/2 j2 −1/2 kσi κ1 ,κ2 ¡ £ ¢© √ × sin δκ1 − δκ2 2 3W (12 j1 j2 ; 3 ji ) Q 01 (κ1 ) √ √ × [ 6Q 12 (κ2 ) − 2Q 32 (κ2 )] + 15Q 11 (κ1 )Q 22 (κ2 ) √ √ ¤ − Q 21 (κ1 )[ 3Q 12 (κ2 ) − 2Q 32 (κ2 )] √ √ + 10 2W (22 j1 j2 ; 3 ji )[ 3Q 12 (κ1 )Q 22 (κ2 ) √ ª (9) + 2Q 22 (κ1 )Q 32 (κ2 )] , p 4π 2 α X (−1) j1 + j2 +|κi | |κ1 ||κ2 | C 40 j1 1/2 j2 −1/2 kσi κ1 ,κ2 ( r ¡ ¢ 10 W (22 j1 j2 ; 4 ji ) × cos δκ1 − δκ2 2 7 √ £ × Q 12 (κ1 )[−3Q 12 (κ2 ) + 2 6Q 32 (κ2 )] ) ¤ − 5Q 22 (κ1 )Q 22 (κ2 ) − 2Q 32 (κ1 )Q 32 (κ2 ) .
(10)
The coefficients B1 , B2 , and B3 are related to the parameters β, γ , and δ describing the photoelectron angular distribution in accordance with Eqs. (2)–(4), in the following way: β = –2B2 , γ = –5B3 , δ = B1 + B3 .
(11)
The coefficient B4 , which is small in magnitude in the energy range considered, does not enter into expressions for the parameters β, γ , and δ. Equation (10) for B4 is presented here for completeness in line with the exact formula (5) for the differential cross section in the quadrupole approximation. In Eqs. (6–10) κ = (` – j)(2 j + 1) is the relativistic quantum number, ` and j are quantum numbers of the orbital and total angular momenta of the electron, k is the photon energy, α = e2 / h-- c is the fine-structure constant, C jJ1M m 1 j2 m 2 is the Clebsch–Gordan coefficient, W (L 1 L 2 j1 j2 ; n ji ) is the Racah coefficient, and (δκ1 − δκ2 ) is the corresponding phase shift for the two possible final continuum states characterized by
(7)
p 4π 2 α X (−1) j1 + j2 +|κi | |κ1 ||κ2 | C 20 j1 1/2 j2 −1/2 kσi κ1 ,κ2 (r ¡ ¢ 3 W (11 j1 j2 ; 2 ji ) × cos δκ1 − δκ2 2 √ £ × 2Q 01 (κ1 )[−Q 01 (κ2 ) + 2Q 21 (κ2 )] 101
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κ1 and κ2 . The reduced matrix element Q ΛL (κ) has the form
The continuum wavefunctions are normalized per unit energy range so that at large distances
Q ΛL (κ) = [(2`¯ + 1)(2`i + 1)/(2Λ + 1)]1/2 `¯ 1/2 j Λ0 × C`0` 1/2 ji R1Λ ¯ i 0 A`i Λ
1
1
s G κ (r ) → and
Λ
1
j1
(12)
where E here √ is the total electron energy including the rest mass, p = E 2 − 1. The computational accuracy of our calculations is better than 0.1%. This accuracy does not include possible uncertainties due to the physical approximations mentioned above. It should be pointed out that in the Table the values of the subshell cross section σi are always given for completely filled shells. To obtain σi for a partially filled atomic subshell i, the value from the Table should be divided by 2 ji + 1 and multiplied by the actual occupation number of the ith subshell.
j2 L
G i (r )Fκ (r ) jΛ (kr ) dr 0
Applications of Nondipolar Parameters (13)
∞
R2Λ =
Photoelectron Angular Distribution in Solids
Fi (r )G κ (r ) jΛ (kr ) dr. 0
Accounting for the photoelectron elastic scattering in the solid results in the following expressions for nonpolarized and linearly polarized excitation sources:
Here jΛ (kr ) is the spherical Bessel function of order Λ, G(r ) = rg(r ) and F(r ) = r f (r ) are the large and small components of the Dirac radial electron wavefunction. Indices i and κ refer to bound and continuum states, respectively. Electron wavefunctions are calculated in the DFS atomic field, the exchange term of the potential being written as Vex = −Cα
· ¸1/3 3 3 ρ(r ) , 2 π
for nonpolarized photons µ ¶ · ¸ β γ aσi dσi = D1 − P2 (cos θ) + sin2 θ + δ cos θ , dÄ 4π 4 2 (17)
(14) for linearly polarized photons · aσi β dσi = D1 + P2 (cos θ ) dÄ 4π 2 ¶ ¸ µ γ cos2 θ + δ sin θ cos ϕ . + 2
where ρ(r ) is the total radial electron density. The coefficient C = 1 is chosen according to Ref. [30]. The wavefunctions of the initial bound states are computed in the self-consistent DFS field of a neutral atom. Continuum wavefunctions are calculated in the frozen orbital approximation where the DFS field of the ion with the hole produced after photoionization is considered, the ion potential being computed by the use of the bound wavefunctions of the neutral atom. The bound electron wavefunctions are normalized so that Z
∞ 0
£
E −1 cos( pr + δκ ), πp
∞
R1Λ = Z
κ |κ|
s
L
is the normalized coefficient of recoupling of four angular momenta. The radial integrals R1Λ and R2Λ can be written as Z
(16) Fκ (r ) →
where `¯ = 2 j − ` and `1 1/2 A`2 1/2
E +1 sin( pr + δκ ) πp
L
+ [(2` + 1)(2`¯i + 1)/(2Λ + 1)]1/2 ` 1/2 j ¯ Λ0 × C`0 1/2 ji R2Λ , `¯i 0 A`i Λ
Photoelectron Angular Distribution
¤ G i2 (r ) + Fi2 (r ) dr = 1.
(18)
Here a = 1 − ω, where ω is the single scattering albedo, D1 = H (ω, α)a −0.5 , H (ω, α) is the Chandrasekhar function, and α is the emission angle of the photoelectron relative to the direction normal to the surface (Fig. 1). Formulae (17) and (18) are obtained using the transport theory approach and the results are in good agreement with the Monte Carlo calculations [16, 17].
(15)
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In contrast to the dipole angular distribution parameter β, the nondipolar parameters γ and δ make the angular distribution dependent on the direction of the photon propagation vector k. Specifically, if the projection of the photoelectron propagation vector p on the photon direction k is positive, i.e., for the back side of the solid sample, the intensity increases in comparison with the dipole approximation. Conversely, for the front side of the solid sample the intensity decreases [25] (see Fig.3). Experimental determination of the γ and δ values has been carried out in [19, 20] based on the photoelectron angular dependence. Our calculations [15, 25] are in good agreement with experimental values for Ar 1s and for Kr 2s and 2 p lines.
Photoelectron Angular Distribution
FIG. 4. Dependence of the q-values of 1s lines on the atomic number for a photon energy 1486.6 eV. The side of the sample facing the photon beam is considered, where cos θ< 0, q < 0 (see Eq. (19) for θ = 125.6◦ ).
X-ray Photoelectron Spectroscopy 54.4◦ since there is no β dependence of the intensity at this angle and, in the dipole approximation, the XPS intensities are proportional to the subshell photoionization cross sections. However, this is not the case when the nondipolar parameters are taken into account. In [33] the q-value is calculated as
The nondipolar parameters γ and δ are important for quantitative x-ray photoelectron spectroscopy (XPS) analysis. Some commercial spectrometers are set at an angle θ =
q=
γ (1 − cos2 θ) cos θ 2
(19)
for all the intense XPS lines used for quantitative analysis in the case of θ = 54.4◦ . The q-value is known to be approximately equal to the percent contribution of nondipolar transitions to the intensity calculated in the dipole approximation. The q-value is shown to be as large as 15% in some cases. As an example, results for 1s lines are given for a photon energy of 1486.6 eV in Fig. 4 [25]. X-ray Standing Wave Method The importance of nondipolar parameters for the interpretation of x-ray standing wave measurements is discussed in [34]. In that paper the parameter Q is introduced which takes into account nondipolar contributions to the intensities of photoelectron lines. In Table B the experimental TABLE B
Experimental and Theoretical Q-Parameters (see text) Line: k (eV): Q exp : Q theor :
FIG. 3. Intensity dependence of Be 1s line (arbitrary units) on the emission angle for a photon energy 1253.6 eV. (A) Linearly polarized excitation. (B) Unpolarized excitation. (1) Dipole approximation. (2) Dipolar and nondipolar contributions for the front sample side. (3) Dipolar and nondipolar contributions for the back sample side.
a b
103
I 3p 2355 0.03a 0.04
I 3d 2355 0.21a 0.23
O 1s 2975 0.27b 0.26
F 1s 2975 0.25b 0.26
Ref. [34]. Ref. [35].
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
15. M. B. Trzhaskovskaya, Yu. I. Kharitonov, V. I. Nefedov, and V. G. Yarzhemsky, Optica i Spectroscopia 88, 547 (2000) [in Russian]
Q-parameters for lines in iodine, oxygen, and fluorine are compared with the calculated ones. The calculations are performed in the approximation used in this paper at the photon energies given in Table B.
16. V. I. Nefedov and I. S. Nefedova, J. Electr. Spectrosc. 107, 131 (2000)
Acknowledgments
17. V. I. Nefedov and I. S. Nefedova, J. Electr. Spectrosc. (to be published)
This work is supported by Grant of Russian Foundation for Basic Research No 99-03-32640. The authors are grateful to the referee for useful comments.
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31. I. M. Band, M. A. Listengarten, M. B. Trzhaskovskaya, and V. I. Fomichev, Complex of Programs RAINE, Part I, Leningrad Nuclear Physics Institute Publication No. 289 (1976)
Photoelectron Angular Distribution
Band and M. B. Trzhaskovskaya, Poverkhnost 6, 16 (2000) [in Russian]
32. T. E. H. Walker and J. T. Waber, J. Phys. B 7, 674 (1974)
34. C. J. Fisher, R. Ithin, R. G. Jones, G. J. Jackson, D. P. Woodruff, and B. C. C. Cowie, J. Phys.: Condens. Matter. 10, L623 (1998)
33. V. I. Nefedov, V. G. Yarzhemsky, I. S. Nefedova, I. M.
35. D. P. Woodruff, private communication (1998)
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EXPLANATION OF TABLE TABLE .
Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 The Table contains the values of the subshell photoionization cross sections σi , Eq. (6), and of the photoelectron angular distribution parameters β, γ , and δ, Eqs. (7–11), at nine photoelectron energies in the range 100 eV ≤ E ≤ 5000 eV. The photoionization cross sections σi are given in kb (=10−21 cm2 ) for completely filled subshells. To obtain σi for a partially filled atomic subshell i, the value from the Table should be divided by 2 ji + 1 and multiplied by the actual occupation number of the ith subshell. Z Atomic number Shell Atomic subshell in which the photoionization occurs Experiment subshell binding energy in eV from [27–29] Eb E Photoelectron energy in eV σ Subshell photoionization cross section in kb (=10−21 cm2 ) β Dipole parameter of the angular distribution γ Nondipolar parameter γ of the angular distribution δ Nondipolar parameter δ of the angular distribution Example In the Table, the first data block gives the parameters for the 1s shell of hydrogen, Z = 1. The binding energy of this shell, rounded off to two digits, is equal to 14 eV. At the photoelectron energy E = 100 eV the subshell photoionization cross section σ = 0.2607 × 102 kb = 0.2607 × 10−19 cm2 , the dipole angular distribution parameter β = 1.999, and the nondipolar parameters γ = 0.237 and δ = −0.164 × 10−8 .
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TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables H, Z = 1 Shell 1s1/2 Eb = 14 eV
100 .2607+2 1.999 .237+0 –.164–8
200 .3564+1 1.998 .335+0 –.210–8
500 .2076+0 1.995 .530+0 –.169–8
1000 .2183–1 1.989 .748+0 .309–8
E (eV) 1500 .5691–2 1.984 .915+0 .144–7
2000 .2173–2 1.979 .105+1 .263–7
3000 .5535–3 1.968 .129+1 .913–7
4000 .2085–3 1.958 .148+1 .129–6
5000 .9749–4 1.947 .165+1 .483–6
100 .1411+3 1.999 .187+0 .525–7
200 .3134+2 1.998 .279+0 .597–7
500 .2831+1 1.995 .499+0 .122–7
1000 .3453+0 1.990 .733+0 .172–6
E (eV) 1500 .9821–1 1.985 .881+0 .181–6
2000 .3996–1 1.980 .103+1 –.717–8
3000 .1060–1 1.967 .130+1 .115–6
4000 .4069–2 1.958 .147+1 .680–6
5000 .1963–2 1.949 .162+1 .758–6
100 .3658+3 1.999 .177+0 –.121–6 .2905+2 2.000 .141+0 –.534–7
200 .1044+3 1.998 .276+0 .180–8 .6171+1 1.999 .238+0 .228–7
500 .1276+2 1.996 .471+0 .195–6 .5399+0 1.996 .468+0 –.469–8
1000 .1996+1 1.990 .699+0 .262–6 .7194–1 1.991 .683+0 .166–7
E (eV) 1500 .6168+0 1.985 .872+0 .302–6 .2094–1 1.985 .879+0 .524–7
2000 .2601+0 1.980 .102+1 .328–6 .8490–2 1.980 .101+1 .127–6
3000 .7406–1 1.969 .126+1 .494–6 .2347–2 1.969 .127+1 .201–6
4000 .2976–1 1.959 .146+1 .700–6 .9237–3 1.959 .145+1 .603–6
5000 .1451–1 1.948 .163+1 .106–5 .4462–3 1.947 .164+1 .583–6
σ β γ δ σ β γ δ
100 .4680+3 1.999 .160+0 –.405–6 .8391+2 2.000 .112+0 –.782–7
200 .1773+3 1.998 .262+0 –.264–6 .1884+2 1.999 .213+0 –.760–7
500 .2972+2 1.995 .463+0 .702–7 .2054+1 1.996 .427+0 –.693–8
1000 .5539+1 1.991 .684+0 .351–6 .3027+0 1.991 .672+0 .225–7
E (eV) 1500 .1870+1 1.985 .855+0 .485–6 .9275–1 1.986 .846+0 .687–7
2000 .8315+0 1.980 .100+1 .594–6 .3915–1 1.981 .985+0 .159–6
3000 .2525+0 1.970 .124+1 .848–6 .1127–1 1.970 .123+1 .346–6
4000 .1053+0 1.959 .144+1 .117–5 .4559–2 1.960 .144+1 .620–6
5000 .5267–1 1.949 .162+1 .160–5 .2239–2 1.949 .162+1 .961–6
σ β γ δ
100 .4687+3 1.999 .145+0 –.769–6
200 .2237+3 1.998 .244+0 –.647–6
500 .5013+2 1.995 .448+0 –.271–6
1000 .1110+2 1.991 .675+0 .207–6
E (eV) 1500 .4051+1 1.986 .846+0 .523–6
2000 .1892+1 1.980 .989+0 .755–6
3000 .6116+0 1.970 .123+1 .116–5
4000 .2647+0 1.960 .143+1 .164–5
5000 .1358+0 1.949 .160+1 .222–5
σ β γ δ
He, Z = 2 Shell 1s1/2 Eb = 25 eV
σ β γ δ
Li, Z = 3 Shell 1s1/2 Eb = 58 eV 2s1/2 Eb = 5 eV
σ β γ δ σ β γ δ
Be, Z = 4 Shell 1s1/2 Eb = 115 eV 2s1/2 Eb = 9 eV
B, Z = 5 Shell 1s1/2 Eb = 192 eV
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TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables B, Z = 5 (continued) Shell 2s1/2 Eb = 12 eV 2 p1/2 Eb = 8 eV
σ β γ δ σ β γ δ
100 .1694+3 2.000 .742–1 –.136–6 .3876+2 1.241 .153+0 .125–1
200 .4261+2 1.999 .177+0 –.134–6 .5378+1 0.920 .182+0 .259–1
500 .5253+1 1.997 .389+0 –.563–7 .2925+0 0.548 .262+0 .586–1
1000 .8689+0 1.992 .633+0 .248–7 .2420–1 0.305 .348+0 .989–1
E (eV) 1500 .2789+0 1.987 .814+0 .889–7 .5145–2 0.181 .397+0 .129+0
2000 .1205+0 1.981 .966+0 .159–6 .1667–2 0.127 .384+0 .154+0
3000 .3594–1 1.971 .121+1 .407–6 .3384–3 0.088 .446+0 .195+0
4000 .1492–1 1.961 .142+1 .735–6 .1067–3 0.061 .511+0 .229+0
5000 .7462–2 1.950 .160+1 .118–5 .4297–4 0.033 .582+0 .259+0
σ β γ δ σ β γ δ σ β γ δ
100 .4240+3 1.999 .128+0 –.120–5 .2500+3 2.000 .391–1 –.226–6 .9818+2 1.380 .149+0 .107–1
200 .2399+3 1.998 .227+0 –.112–5 .7188+2 1.999 .136+0 –.228–6 .1495+2 1.099 .204+0 .214–1
500 .6913+2 1.996 .431+0 –.747–6 .9932+1 1.997 .349+0 –.870–7 .9207+0 0.685 .286+0 .507–1
1000 .1809+2 1.991 .661+0 –.176–6 .1778+1 1.993 .589+0 .140–7 .8638–1 0.438 .371+0 .890–1
E (eV) 1500 .7150+1 1.986 .835+0 .294–6 .5983+0 1.988 .777+0 .796–7 .1939–1 0.313 .417+0 .120+0
2000 .3502+1 1.980 .979+0 .687–6 .2674+0 1.982 .937+0 .179–6 .6439–2 0.216 .460+0 .147+0
3000 .1198+1 1.970 .122+1 .137–5 .8230–1 1.972 .119+1 .458–6 .1321–2 0.119 .504+0 .190+0
4000 .5375+0 1.960 .142+1 .204–5 .3483–1 1.962 .139+1 .869–6 .4244–3 0.078 .549+0 .224+0
5000 .2828+0 1.950 .159+1 .276–5 .1767–1 1.951 .157+1 .141–5 .1741–3 0.057 .582+0 .253+0
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3688+3 1.999 .106+0 –.169–5 .3172+3 2.000 .104–1 –.379–6 .1901+3 1.454 .133+0 .988–2 .3788+3 1.455 .133+0 .101–1
200 .2356+3 1.998 .209+0 –.166–5 .1030+3 2.000 .951–1 –.363–6 .3229+2 1.239 .210+0 .182–1 .6429+2 1.241 .210+0 .186–1
500 .8359+2 1.996 .413+0 –.133–5 .1602+2 1.998 .304+0 –.116–6 .2199+1 0.825 .308+0 .437–1 .4371+1 0.827 .308+0 .440–1
1000 .2554+2 1.991 .643+0 –.713–6 .3061+1 1.993 .551+0 –.428–7 .2219+0 0.544 .379+0 .812–1 .4402+0 0.546 .379+0 .814–1
E (eV) 1500 .1092+2 1.986 .819+0 –.155–6 .1074+1 1.988 .742+0 .454–7 .5255–1 0.405 .436+0 .113+0 .1041+0 0.408 .435+0 .113+0
2000 .5614+1 1.981 .967+0 .352–6 .4936+0 1.983 .895+0 .188–6 .1829–1 0.318 .492+0 .137+0 .3620–1 0.323 .491+0 .137+0
3000 .2034+1 1.970 .121+1 .131–5 .1573+0 1.973 .115+1 .498–6 .3879–2 0.202 .548+0 .180+0 .7663–2 0.209 .545+0 .180+0
4000 .9444+0 1.960 .141+1 .226–5 .6793–1 1.962 .137+1 .945–6 .1254–2 0.127 .578+0 .217+0 .2473–2 0.137 .574+0 .217+0
5000 .5088+0 1.950 .158+1 .322–5 .3493–1 1.952 .155+1 .158–5 .5194–3 0.083 .625+0 .247+0 .1022–2 0.096 .620+0 .247+0
C, Z = 6 Shell 1s1/2 Eb = 288 eV 2s1/2 Eb = 16 eV 2 p1/2 Eb = 11 eV
N, Z = 7 Shell 1s1/2 Eb = 403 eV 2s1/2 Eb = 20 eV 2 p1/2 Eb = 14 eV 2 p3/2 Eb = 14 eV
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TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables O, Z = 8 Shell 1s1/2 Eb = 538 eV 2s1/2 Eb = 28 eV 2 p1/2 Eb = 14 eV 2 p3/2 Eb = 14 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3160+3 1.999 .795–1 –.226–5 .3572+3 2.000 –.975–2 –.621–6 .3183+3 1.486 .111+0 .941–2 .6340+3 1.487 .111+0 .963–2
200 .2206+3 1.998 .187+0 –.229–5 .1306+3 2.000 .577–1 –.560–6 .5985+2 1.337 .199+0 .159–1 .1191+3 1.339 .199+0 .163–1
500 .9256+2 1.996 .395+0 –.202–5 .2302+2 1.998 .260+0 –.199–6 .4449+1 0.957 .320+0 .380–1 .8832+1 0.959 .320+0 .382–1
1000 .3253+2 1.991 .626+0 –.138–5 .4727+1 1.994 .513+0 –.140–6 .4744+0 0.645 .399+0 .740–1 .9398+0 0.648 .399+0 .743–1
E (eV) 1500 .1500+2 1.986 .802+0 –.768–6 .1719+1 1.989 .702+0 .104–7 .1177+0 0.491 .463+0 .104+0 .2329+0 0.494 .462+0 .104+0
2000 .8087+1 1.981 .951+0 –.185–6 .8077+0 1.984 .861+0 .131–6 .4199–1 0.397 .500+0 .129+0 .8297–1 0.401 .499+0 .130+0
3000 .3107+1 1.970 .120+1 .974–6 .2664+0 1.974 .112+1 .495–6 .9294–2 0.273 .575+0 .173+0 .1833–1 0.280 .573+0 .173+0
4000 .1493+1 1.960 .140+1 .217–5 .1175+0 1.964 .134+1 .104–5 .3085–2 0.191 .635+0 .208+0 .6070–2 0.201 .631+0 .208+0
5000 .8238+0 1.950 .157+1 .340–5 .6126–1 1.953 .152+1 .169–5 .1289–2 0.136 .661+0 .239+0 .2531–2 0.148 .656+0 .239+0
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2699+3 1.999 .497–1 –.290–5 .3764+3 2.000 –.206–1 –.960–6 .4608+3 1.491 .931–1 .947–2 .9173+3 1.492 .933–1 .963–2
200 .2012+3 1.998 .162+0 –.301–5 .1531+3 2.000 .250–1 –.839–6 .9682+2 1.400 .183+0 .147–1 .1924+3 1.402 .183+0 .151–1
500 .9660+2 1.995 .375+0 –.281–5 .3050+2 1.999 .216+0 –.367–6 .7933+1 1.071 .324+0 .339–1 .1573+2 1.074 .325+0 .340–1
1000 .3843+2 1.991 .609+0 –.220–5 .6754+1 1.995 .472+0 –.245–6 .8987+0 0.750 .426+0 .672–1 .1778+1 0.752 .426+0 .675–1
E (eV) 1500 .1900+2 1.986 .785+0 –.154–5 .2537+1 1.990 .662+0 –.503–7 .2307+0 0.581 .486+0 .957–1 .4556+0 0.584 .486+0 .958–1
2000 .1073+2 1.981 .935+0 –.898–6 .1219+1 1.985 .826+0 .602–7 .8403–1 0.469 .526+0 .122+0 .1657+0 0.473 .525+0 .122+0
3000 .4370+1 1.971 .118+1 .410–6 .4140+0 1.975 .109+1 .502–6 .1934–1 0.339 .606+0 .164+0 .3805–1 0.345 .604+0 .164+0
4000 .2177+1 1.960 .138+1 .180–5 .1861+0 1.965 .130+1 .104–5 .6568–2 0.255 .656+0 .200+0 .1289–1 0.264 .652+0 .200+0
5000 .1230+1 1.950 .156+1 .328–5 .9848–1 1.955 .149+1 .178–5 .2786–2 0.190 .702+0 .232+0 .5459–2 0.201 .697+0 .231+0
100 .2313+3 1.999 .184–1 –.361–5
200 .1813+3 1.998 .134+0 –.381–5
500 .9695+2 1.995 .353+0 –.371–5
1000 .4296+2 1.991 .591+0 –.314–5
E (eV) 1500 .2267+2 1.986 .769+0 –.246–5
2000 .1338+2 1.981 .918+0 –.177–5
3000 .5764+1 1.971 .117+1 –.347–6
4000 .2974+1 1.961 .137+1 .120–5
5000 .1722+1 1.950 .155+1 .286–5
F, Z = 9 Shell 1s1/2 Eb = 694 eV 2s1/2 Eb = 38 eV 2 p1/2 Eb = 17 eV 2 p3/2 Eb = 17 eV
Ne, Z = 10 Shell 1s1/2 Eb = 870 eV
σ β γ δ
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TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Ne, Z = 10 (continued) Shell 2s1/2 Eb = 48 eV 2 p1/2 Eb = 22 eV 2 p3/2 Eb = 22 eV
σ β γ δ σ β γ δ σ β γ δ
100 .3839+3 2.000 –.203–1 –.138–5 .6004+3 1.477 .791–1 .982–2 .1194+4 1.479 .793–1 .993–2
200 .1711+3 2.000 –.160–2 –.120–5 .1415+3 1.440 .166+0 .142–1 .2810+3 1.442 .166+0 .145–1
500 .3815+2 1.999 .172+0 –.630–6 .1288+2 1.167 .323+0 .307–1 .2549+2 1.170 .324+0 .310–1
1000 .9095+1 1.995 .425+0 –.355–6 .1557+1 0.851 .449+0 .609–1 .3075+1 0.854 .449+0 .611–1
E (eV) 1500 .3527+1 1.991 .620+0 –.175–6 .4103+0 0.671 .509+0 .885–1 .8086+0 0.674 .509+0 .885–1
2000 .1732+1 1.986 .784+0 –.854–8 .1529+0 0.546 .557+0 .114+0 .3008+0 0.551 .557+0 .114+0
3000 .6034+0 1.977 .105+1 .432–6 .3620–1 0.403 .626+0 .156+0 .7104–1 0.409 .625+0 .156+0
4000 .2763+0 1.966 .127+1 .102–5 .1254–1 0.310 .679+0 .192+0 .2455–1 0.318 .675+0 .192+0
5000 .1482+0 1.956 .146+1 .187–5 .5420–2 0.245 .734+0 .223+0 .1059–1 0.256 .729+0 .223+0
100 .1937+3 1.999 –.531–3 –.445–5 .3890+3 2.000 –.135–1 –.204–5 .7121+3 1.471 .721–1 .101–1 .1417+4 1.473 .724–1 .101–1 .2683+2 2.000 –.690–2 .507–6
200 .1582+3 1.998 .115+0 –.472–5 .1861+3 2.000 –.139–1 –.176–5 .1911+3 1.459 .155+0 .140–1 .3794+3 1.461 .155+0 .143–1 .1019+2 2.000 –.264–1 .385–6
500 .9272+2 1.995 .336+0 –.468–5 .4678+2 1.999 .136+0 –.957–6 .2049+2 1.236 .321+0 .283–1 .4056+2 1.239 .322+0 .286–1 .1905+1 1.999 .120+0 –.130–6
1000 .4529+2 1.991 .573+0 –.415–5 .1206+2 1.996 .380+0 –.520–6 .2712+1 0.942 .460+0 .555–1 .5353+1 0.945 .461+0 .557–1 .4362+0 1.996 .370+0 –.307–6
E (eV) 1500 .2543+2 1.986 .753+0 –.348–5 .4867+1 1.992 .578+0 –.333–6 .7427+0 0.750 .532+0 .819–1 .1462+1 0.754 .532+0 .820–1 .1683+0 1.992 .567+0 .110–7
2000 .1567+2 1.981 .902+0 –.274–5 .2447+1 1.987 .742+0 –.142–6 .2840+0 0.625 .581+0 .106+0 .5583+0 0.630 .581+0 .106+0 .8216–1 1.987 .736+0 –.566–7
3000 .7148+1 1.971 .115+1 –.121–5 .8781+0 1.978 .101+1 .338–6 .6938–1 0.464 .652+0 .148+0 .1360+0 0.471 .651+0 .148+0 .2868–1 1.978 .101+1 .318–6
4000 .3824+1 1.961 .136+1 .474–6 .4098+0 1.968 .123+1 .101–5 .2462–1 0.364 .706+0 .184+0 .4814–1 0.372 .704+0 .184+0 .1319–1 1.968 .123+1 .973–6
5000 .2272+1 1.950 .153+1 .228–5 .2227+0 1.958 .143+1 .188–5 .1081–1 0.293 .756+0 .215+0 .2109–1 0.303 .751+0 .215+0 .7102–2 1.958 .142+1 .171–5
100 .1632+3 1.999 –.203–1 –.545–5
200 .1374+3 1.998 .949–1 –.577–5
500 .8683+2 1.995 .320+0 –.581–5
1000 .4615+2 1.990 .560+0 –.534–5
E (eV) 1500 .2742+2 1.986 .741+0 –.467–5
2000 .1760+2 1.981 .890+0 –.392–5
3000 .8476+1 1.971 .114+1 –.228–5
4000 .4700+1 1.961 .134+1 –.450–6
5000 .2864+1 1.950 .152+1 .154–5
Na, Z = 11 Shell 1s1/2 Eb = 1075 eV 2s1/2 Eb = 66 eV 2 p1/2 Eb = 34 eV 2 p3/2 Eb = 34 eV 3s1/2 Eb = 5 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
Mg, Z = 12 Shell 1s1/2 Eb = 1308 eV
σ β γ δ
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TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Mg, Z = 12 (continued) Shell 2s1/2 Eb = 92 eV 2 p1/2 Eb = 54 eV 2 p3/2 Eb = 54 eV 3s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3760+3 1.999 –.291–2 –.263–5 .7617+3 1.460 .633–1 .102–1 .1516+4 1.462 .635–1 .102–1 .5502+2 2.000 .473–2 –.882–6
200 .1951+3 2.000 –.233–1 –.238–5 .2346+3 1.474 .148+0 .140–1 .4659+3 1.477 .148+0 .143–1 .1971+2 2.000 –.285–1 –.104–6
500 .5454+2 1.999 .106+0 –.144–5 .2924+2 1.290 .317+0 .267–1 .5783+2 1.294 .318+0 .270–1 .3969+1 2.000 .883–1 –.138–6
1000 .1520+2 1.997 .340+0 –.816–6 .4253+1 1.017 .469+0 .513–1 .8383+1 1.021 .470+0 .515–1 .9434+0 1.997 .322+0 –.200–6
E (eV) 1500 .6387+1 1.993 .537+0 –.541–6 .1217+1 0.828 .552+0 .760–1 .2393+1 0.833 .554+0 .761–1 .3730+0 1.993 .522+0 –.148–6
2000 .3291+1 1.988 .704+0 –.324–6 .4777+0 0.696 .607+0 .992–1 .9376+0 0.701 .607+0 .993–1 .1858+0 1.989 .691+0 –.101–6
3000 .1217+1 1.979 .977+0 .195–6 .1205+0 0.524 .680+0 .140+0 .2358+0 0.531 .679+0 .141+0 .6631–1 1.979 .966+0 .318–6
4000 .5787+0 1.969 .120+1 .916–6 .4368–1 0.417 .735+0 .176+0 .8523–1 0.426 .733+0 .176+0 .3093–1 1.969 .119+1 .916–6
5000 .3188+0 1.959 .139+1 .186–5 .1948–1 0.341 .782+0 .208+0 .3792–1 0.351 .777+0 .208+0 .1684–1 1.959 .139+1 .171–5
100 .1391+3 1.998 –.400–1 –.660–5 .3581+3 1.999 .111–1 –.325–5 .7773+3 1.444 .527–1 .102–1 .1548+4 1.447 .529–1 .102–1 .9121+2 1.999 .168–1 –.118–5 .7676+2 1.568 .296–1 .602–2
200 .1197+3 1.998 .748–1 –.694–5 .1995+3 2.000 –.279–1 –.308–5 .2703+3 1.482 .138+0 .138–1 .5366+3 1.485 .139+0 .141–1 .3316+2 2.000 –.288–1 –.495–6 .2074+2 1.574 .106+0 .921–2
500 .8043+2 1.995 .303+0 –.709–5 .6154+2 2.000 .785–1 –.206–5 .3896+2 1.333 .313+0 .254–1 .7701+2 1.338 .314+0 .257–1 .6984+1 2.000 .565–1 –.755–7 .2279+1 1.372 .292+0 .206–1
1000 .4595+2 1.990 .546+0 –.668–5 .1840+2 1.997 .303+0 –.122–5 .6204+1 1.081 .474+0 .477–1 .1222+2 1.086 .476+0 .479–1 .1716+1 1.997 .284+0 –.429–6 .3087+0 1.094 .463+0 .443–1
E (eV) 1500 .2871+2 1.985 .725+0 –.600–5 .8039+1 1.993 .495+0 –.840–6 .1857+1 0.904 .568+0 .710–1 .3647+1 0.909 .570+0 .711–1 .6949+0 1.994 .479+0 –.322–6 .8689–1 0.904 .561+0 .679–1
2000 .1912+2 1.981 .877+0 –.525–5 .4246+1 1.989 .663+0 –.571–6 .7487+0 0.767 .629+0 .930–1 .1467+1 0.773 .630+0 .930–1 .3524+0 1.990 .646+0 –.156–6 .3384–1 0.767 .626+0 .901–1
3000 .9701+1 1.971 .112+1 –.351–5 .1619+1 1.980 .937+0 –.165–8 .1951+0 0.587 .709+0 .133+0 .3811+0 0.594 .709+0 .133+0 .1285+0 1.980 .928+0 .153–6 .8474–2 0.585 .703+0 .131+0
4000 .5569+1 1.961 .133+1 –.161–5 .7840+0 1.970 .117+1 .769–6 .7218–1 0.470 .765+0 .168+0 .1406+0 0.479 .763+0 .168+0 .6082–1 1.971 .115+1 .809–6 .3070–2 0.470 .760+0 .167+0
5000 .3479+1 1.950 .151+1 .516–6 .4375+0 1.960 .136+1 .177–5 .3267–1 0.388 .811+0 .199+0 .6347–1 0.398 .808+0 .199+0 .3345–1 1.961 .135+1 .170–5 .1371–2 0.387 .807+0 .198+0
Al, Z = 13 Shell 1s1/2 Eb = 1564 eV 2s1/2 Eb = 121 eV 2 p1/2 Eb = 77 eV 2 p3/2 Eb = 77 eV 3s1/2 Eb = 10 eV 3 p1/2 Eb = 6 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
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TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Si, Z = 14 Shell 1s1/2 Eb = 1844 eV 2s1/2 Eb = 154 eV 2 p1/2 Eb = 104 eV 2 p3/2 Eb = 104 eV 3s1/2 Eb = 13 eV 3 p1/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1196+3 1.998 –.621–1 –.790–5 .3362+3 1.999 .296–1 –.392–5 .7692+3 1.424 .411–1 .102–1 .1532+4 1.427 .413–1 .101–1 .1242+3 1.999 .315–1 –.130–5 .1271+3 1.566 .149–1 .493–2
200 .1049+3 1.997 .545–1 –.833–5 .1999+3 2.000 –.286–1 –.389–5 .2982+3 1.482 .127+0 .137–1 .5922+3 1.487 .128+0 .140–1 .4560+2 2.000 –.254–1 –.822–6 .3615+2 1.593 .899–1 .827–2
500 .7405+2 1.995 .285+0 –.855–5 .6760+2 2.000 .530–1 –.283–5 .4935+2 1.369 .308+0 .243–1 .9750+2 1.374 .309+0 .247–1 .9892+1 2.000 .313–1 –.351–6 .4368+1 1.415 .275+0 .185–1
1000 .4500+2 1.990 .530+0 –.820–5 .2158+2 1.998 .267+0 –.177–5 .8553+1 1.139 .477+0 .447–1 .1682+2 1.145 .479+0 .450–1 .2525+1 1.998 .244+0 –.443–6 .6291+0 1.157 .462+0 .401–1
E (eV) 1500 .2941+2 1.985 .711+0 –.752–5 .9777+1 1.994 .455+0 –.125–5 .2675+1 0.968 .580+0 .665–1 .5247+1 0.975 .582+0 .665–1 .1042+1 1.995 .435+0 –.532–6 .1822+0 0.971 .565+0 .622–1
2000 .2026+2 1.980 .863+0 –.676–5 .5290+1 1.990 .621+0 –.912–6 .1109+1 0.834 .648+0 .874–1 .2170+1 0.841 .650+0 .874–1 .5367+0 1.991 .601+0 –.416–6 .7246–1 0.835 .635+0 .836–1
3000 .1079+2 1.970 .111+1 –.497–5 .2078+1 1.981 .897+0 –.276–6 .2986+0 0.650 .737+0 .127+0 .5821+0 0.657 .737+0 .126+0 .2001+0 1.982 .882+0 .406–7 .1863–1 0.646 .730+0 .123+0
4000 .6402+1 1.960 .132+1 –.294–5 .1025+1 1.971 .113+1 .545–6 .1127+0 0.525 .795+0 .161+0 .2190+0 0.534 .794+0 .161+0 .9598–1 1.972 .111+1 .687–6 .6854–2 0.522 .789+0 .159+0
5000 .4097+1 1.950 .150+1 –.659–6 .5795+0 1.962 .132+1 .161–5 .5173–1 0.437 .841+0 .192+0 .1003+0 0.447 .838+0 .192+0 .5332–1 1.962 .131+1 .162–5 .3098–2 0.432 .835+0 .190+0
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1036+3 1.998 –.865–1 –.937–5 .3122+3 1.999 .526–1 –.465–5 .7396+3 1.401 .289–1 .103–1 .1480+4 1.404 .289–1 .101–1
200 .9251+2 1.997 .333–1 –.993–5 .1969+3 1.999 –.254–1 –.480–5 .3173+3 1.478 .115+0 .137–1 .6319+3 1.483 .116+0 .139–1
500 .6793+2 1.994 .266+0 –.102–4 .7257+2 2.000 .298–1 –.376–5 .5983+2 1.397 .302+0 .234–1 .1183+3 1.403 .303+0 .238–1
1000 .4354+2 1.990 .514+0 –.992–5 .2465+2 1.998 .232+0 –.249–5 .1126+2 1.190 .480+0 .423–1 .2214+2 1.197 .482+0 .425–1
E (eV) 1500 .2960+2 1.985 .697+0 –.926–5 .1155+2 1.995 .417+0 –.180–5 .3673+1 1.027 .589+0 .626–1 .7198+1 1.034 .592+0 .626–1
2000 .2104+2 1.980 .850+0 –.850–5 .6396+1 1.991 .581+0 –.137–5 .1565+1 0.895 .664+0 .823–1 .3058+1 0.903 .666+0 .822–1
3000 .1172+2 1.970 .110+1 –.665–5 .2588+1 1.982 .857+0 –.646–6 .4356+0 0.710 .762+0 .120+0 .8479+0 0.718 .764+0 .120+0
4000 .7175+1 1.960 .130+1 –.453–5 .1301+1 1.973 .109+1 .230–6 .1677+0 0.581 .825+0 .154+0 .3253+0 0.590 .825+0 .154+0
5000 .4701+1 1.950 .149+1 –.216–5 .7447+0 1.963 .129+1 .136–5 .7810–1 0.486 .873+0 .184+0 .1511+0 0.497 .871+0 .184+0
P, Z = 15 Shell 1s1/2 Eb = 2148 eV 2s1/2 Eb = 191 eV 2 p1/2 Eb = 136 eV 2 p3/2 Eb = 135 eV
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TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables P, Z = 15 (continued) Shell 3s1/2 Eb = 16 eV 3 p1/2 Eb = 10 eV 3 p3/2 Eb = 10 eV
σ β γ δ σ β γ δ σ β γ δ
100 .1547+3 1.999 .481–1 –.149–5 .1768+3 1.555 .147–2 .379–2 .3525+3 1.555 .169–2 .377–2
200 .5819+2 1.999 –.194–1 –.107–5 .5329+2 1.606 .724–1 .732–2 .1057+3 1.609 .728–1 .740–2
500 .1289+2 2.000 .112–1 –.787–6 .6948+1 1.452 .257+0 .168–1 .1370+2 1.458 .259+0 .168–1
1000 .3410+1 1.998 .204+0 –.559–6 .1067+1 1.211 .454+0 .359–1 .2093+1 1.218 .456+0 .357–1
E (eV) 1500 .1433+1 1.995 .393+0 –.709–6 .3167+0 1.032 .567+0 .572–1 .6192+0 1.038 .569+0 .568–1
2000 .7473+0 1.992 .559+0 –.717–6 .1282+0 0.897 .643+0 .780–1 .2501+0 0.904 .645+0 .776–1
3000 .2843+0 1.983 .836+0 –.227–6 .3389–1 0.707 .748+0 .116+0 .6584–1 0.715 .749+0 .115+0
4000 .1382+0 1.974 .107+1 .463–6 .1266–1 0.576 .815+0 .150+0 .2452–1 0.585 .815+0 .150+0
5000 .7751–1 1.964 .127+1 .141–5 .5787–2 0.482 .863+0 .181+0 .1117–1 0.493 .861+0 .181+0
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .9033+2 1.998 –.113+0 –.110–4 .2880+3 1.998 .797–1 –.542–5 .7044+3 1.377 .157–1 .102–1 .1414+4 1.380 .157–1 .992–2 .1807+3 1.999 .662–1 –.175–5 .2268+3 1.536 –.895–2 .253–2 .4528+3 1.536 –.878–2 .249–2
200 .8194+2 1.997 .106–1 –.117–4 .1914+3 1.999 –.178–1 –.580–5 .3306+3 1.470 .101+0 .136–1 .6600+3 1.475 .101+0 .137–1 .7056+2 1.999 –.108–1 –.141–5 .7261+2 1.615 .538–1 .632–2 .1441+3 1.618 .543–1 .642–2
500 .6225+2 1.994 .246+0 –.121–4 .7643+2 2.000 .940–2 –.483–5 .7020+2 1.419 .293+0 .227–1 .1390+3 1.426 .294+0 .231–1 .1601+2 2.000 –.507–2 –.128–5 .1006+2 1.486 .239+0 .152–1 .1982+2 1.492 .240+0 .153–1
1000 .4176+2 1.989 .497+0 –.119–4 .2756+2 1.998 .198+0 –.339–5 .1431+2 1.235 .481+0 .401–1 .2813+2 1.242 .483+0 .403–1 .4362+1 1.999 .167+0 –.912–6 .1636+1 1.261 .442+0 .328–1 .3204+1 1.268 .445+0 .326–1
E (eV) 1500 .2940+2 1.984 .682+0 –.112–4 .1333+2 1.995 .379+0 –.253–5 .4853+1 1.079 .596+0 .591–1 .9505+1 1.087 .599+0 .591–1 .1870+1 1.996 .352+0 –.954–6 .4987+0 1.088 .569+0 .524–1 .9736+0 1.095 .572+0 .521–1
2000 .2149+2 1.980 .836+0 –.105–4 .7543+1 1.992 .541+0 –.197–5 .2122+1 0.951 .676+0 .777–1 .4144+1 0.960 .679+0 .776–1 .9869+0 1.992 .516+0 –.920–6 .2053+0 0.955 .654+0 .720–1 .3997+0 0.962 .657+0 .716–1
3000 .1248+2 1.970 .108+1 –.859–5 .3142+1 1.983 .816+0 –.113–5 .6110+0 0.766 .784+0 .114+0 .1187+1 0.775 .786+0 .113+0 .3818+0 1.984 .793+0 –.593–6 .5551–1 0.764 .763+0 .109+0 .1076+0 0.773 .765+0 .109+0
4000 .7871+1 1.960 .129+1 –.639–5 .1608+1 1.974 .105+1 –.194–6 .2400+0 0.635 .854+0 .147+0 .4647+0 0.644 .854+0 .147+0 .1881+0 1.975 .103+1 .142–6 .2108–1 0.630 .838+0 .143+0 .4073–1 0.640 .838+0 .142+0
5000 .5274+1 1.950 .147+1 –.390–5 .9324+0 1.964 .125+1 .993–6 .1133+0 0.535 .904+0 .177+0 .2187+0 0.546 .902+0 .176+0 .1065+0 1.965 .123+1 .120–5 .9739–2 0.531 .891+0 .173+0 .1875–1 0.542 .890+0 .173+0
S, Z = 16 Shell 1s1/2 Eb = 2476 eV 2s1/2 Eb = 232 eV 2 p1/2 Eb = 170 eV 2 p3/2 Eb = 168 eV 3s1/2 Eb = 20 eV 3 p1/2 Eb = 10 eV 3 p3/2 Eb = 10 eV
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TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Cl, Z = 17 Shell 1s1/2 Eb = 2829 eV 2s1/2 Eb = 277 eV 2 p1/2 Eb = 208 eV 2 p3/2 Eb = 206 eV 3s1/2 Eb = 24 eV 3 p1/2 Eb = 13 eV 3 p3/2 Eb = 13 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .7925+2 1.997 –.141+0 –.129–4 .2647+3 1.998 .111+0 –.624–5 .6620+3 1.351 .179–2 .100–1 .1328+4 1.354 .173–2 .971–2 .2028+3 1.999 .847–1 –.204–5 .2653+3 1.510 –.154–1 .131–2 .5302+3 1.509 –.154–1 .126–2
200 .7286+2 1.996 –.138–1 –.138–4 .1840+3 1.999 –.603–2 –.689–5 .3367+3 1.459 .861–1 .135–1 .6721+3 1.465 .864–1 .136–1 .8262+2 1.999 .692–3 –.185–5 .9195+2 1.617 .365–1 .542–2 .1825+3 1.620 .369–1 .553–2
500 .5704+2 1.994 .224+0 –.143–4 .7919+2 2.000 –.782–2 –.604–5 .7995+2 1.436 .282+0 .222–1 .1582+3 1.444 .284+0 .225–1 .1932+2 2.000 –.186–1 –.178–5 .1365+2 1.515 .222+0 .137–1 .2688+2 1.522 .223+0 .138–1
1000 .3978+2 1.989 .481+0 –.141–4 .3024+2 1.999 .166+0 –.450–5 .1761+2 1.272 .480+0 .383–1 .3460+2 1.281 .482+0 .385–1 .5381+1 1.999 .134+0 –.143–5 .2338+1 1.304 .431+0 .300–1 .4573+1 1.313 .434+0 .298–1
E (eV) 1500 .2889+2 1.984 .667+0 –.135–4 .1509+2 1.996 .343+0 –.346–5 .6208+1 1.126 .602+0 .560–1 .1214+2 1.135 .605+0 .560–1 .2350+1 1.997 .309+0 –.124–5 .7346+0 1.139 .569+0 .478–1 .1432+1 1.148 .572+0 .475–1
2000 .2165+2 1.979 .821+0 –.127–4 .8712+1 1.992 .503+0 –.277–5 .2783+1 1.003 .687+0 .736–1 .5424+1 1.012 .690+0 .734–1 .1255+1 1.993 .472+0 –.121–5 .3073+0 1.009 .659+0 .664–1 .5970+0 1.017 .662+0 .659–1
3000 .1307+2 1.969 .107+1 –.108–4 .3730+1 1.984 .776+0 –.176–5 .8278+0 0.820 .803+0 .108+0 .1606+1 0.830 .806+0 .108+0 .4932+0 1.985 .749+0 –.955–6 .8480–1 0.819 .779+0 .102+0 .1640+0 0.828 .782+0 .102+0
4000 .8477+1 1.960 .128+1 –.854–5 .1943+1 1.975 .101+1 –.753–6 .3319+0 0.685 .879+0 .140+0 .6412+0 0.696 .881+0 .140+0 .2457+0 1.976 .983+0 –.242–6 .3272–1 0.683 .859+0 .135+0 .6304–1 0.693 .860+0 .134+0
5000 .5804+1 1.950 .146+1 –.594–5 .1141+1 1.966 .121+1 .500–6 .1589+0 0.583 .933+0 .170+0 .3060+0 0.595 .933+0 .169+0 .1404+0 1.967 .119+1 .811–6 .1528–1 0.580 .917+0 .165+0 .2935–1 0.591 .916+0 .164+0
100 .6998+2 1.997 –.171+0 –.151–4 .2430+3 1.997 .145+0 –.711–5 .6149+3 1.325 –.129–1 .975–2
200 .6506+2 1.996 –.398–1 –.162–4 .1755+3 1.998 .991–2 –.810–5 .3361+3 1.446 .707–1 .135–1
500 .5231+2 1.993 .203+0 –.168–4 .8094+2 2.000 –.217–1 –.743–5 .8871+2 1.447 .270+0 .217–1
1000 .3771+2 1.988 .462+0 –.167–4 .3264+2 1.999 .134+0 –.581–5 .2108+2 1.305 .477+0 .367–1
E (eV) 1500 .2816+2 1.984 .650+0 –.161–4 .1679+2 1.996 .306+0 –.464–5 .7718+1 1.167 .606+0 .531–1
2000 .2159+2 1.979 .806+0 –.153–4 .9885+1 1.993 .464+0 –.379–5 .3544+1 1.050 .696+0 .699–1
3000 .1350+2 1.969 .106+1 –.133–4 .4343+1 1.985 .736+0 –.257–5 .1088+1 0.871 .820+0 .103+0
4000 .8991+1 1.959 .127+1 –.110–4 .2303+1 1.977 .968+0 –.146–5 .4453+0 0.736 .902+0 .134+0
5000 .6283+1 1.949 .145+1 –.831–5 .1370+1 1.967 .117+1 –.143–6 .2163+0 0.631 .961+0 .163+0
Ar, Z = 18 Shell 1s1/2 Eb = 3206 eV 2s1/2 Eb = 326 eV 2 p1/2 Eb = 251 eV
σ β γ δ σ β γ δ σ β γ δ
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TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Ar, Z = 18 (continued) Shell 2 p3/2 Eb = 248 eV 3s1/2 Eb = 29 eV 3 p1/2 Eb = 16 eV 3 p3/2 Eb = 16 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1237+4 1.328 –.130–1 .936–2 .2191+3 1.999 .104+0 –.236–5 .2958+3 1.479 –.170–1 .111–3 .5921+3 1.478 –.171–1 .290–4
200 .6721+3 1.452 .708–1 .135–1 .9369+2 1.999 .148–1 –.240–5 .1114+3 1.615 .201–1 .449–2 .2212+3 1.617 .206–1 .461–2
500 .1757+3 1.456 .271+0 .221–1 .2275+2 2.000 –.296–1 –.220–5 .1777+2 1.541 .202+0 .122–1 .3497+2 1.548 .204+0 .123–1
1000 .4140+2 1.315 .480+0 .370–1 .6457+1 1.999 .103+0 –.194–5 .3184+1 1.344 .417+0 .272–1 .6220+1 1.353 .420+0 .271–1
E (eV) 1500 .1508+2 1.178 .610+0 .531–1 .2866+1 1.997 .268+0 –.169–5 .1029+1 1.187 .561+0 .437–1 .2002+1 1.196 .564+0 .433–1
2000 .6900+1 1.060 .700+0 .697–1 .1549+1 1.994 .429+0 –.169–5 .4374+0 1.059 .660+0 .615–1 .8481+0 1.069 .664+0 .610–1
3000 .2107+1 0.881 .824+0 .103+0 .6181+0 1.986 .706+0 –.145–5 .1231+0 0.870 .790+0 .961–1 .2376+0 0.881 .794+0 .954–1
4000 .8585+0 0.747 .905+0 .133+0 .3112+0 1.978 .940+0 –.788–6 .4818–1 0.733 .875+0 .128+0 .9258–1 0.744 .877+0 .127+0
5000 .4155+0 0.643 .962+0 .162+0 .1794+0 1.969 .115+1 .352–6 .2277–1 0.629 .939+0 .157+0 .4360–1 0.640 .940+0 .157+0
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .6192+2 1.996 –.193+0 –.178–4 .2204+3 1.997 .164+0 –.813–5 .5511+3 1.312 –.235–1 .942–2 .1107+4 1.316 –.238–1 .905–2 .2371+3 1.999 .112+0 –.286–5 .3549+3 1.467 –.136–1 –.280–3
200 .5806+2 1.995 –.597–1 –.190–4 .1645+3 1.998 .235–1 –.934–5 .3217+3 1.435 .587–1 .134–1 .6428+3 1.442 .589–1 .134–1 .1065+3 1.999 .255–1 –.283–5 .1413+3 1.614 .895–2 .365–2
500 .4781+2 1.993 .186+0 –.197–4 .8098+2 2.000 –.307–1 –.893–5 .9455+2 1.454 .258+0 .214–1 .1871+3 1.464 .260+0 .217–1 .2709+2 2.000 –.360–1 –.262–5 .2426+2 1.560 .181+0 .108–1
1000 .3551+2 1.988 .446+0 –.195–4 .3449+2 1.999 .107+0 –.728–5 .2431+2 1.331 .472+0 .356–1 .4769+2 1.342 .476+0 .358–1 .7881+1 2.000 .767–1 –.253–5 .4560+1 1.378 .401+0 .249–1
E (eV) 1500 .2717+2 1.983 .637+0 –.189–4 .1829+2 1.997 .273+0 –.600–5 .9274+1 1.202 .607+0 .508–1 .1810+2 1.214 .612+0 .508–1 .3556+1 1.998 .233+0 –.236–5 .1518+1 1.226 .549+0 .402–1
2000 .2127+2 1.978 .790+0 –.182–4 .1099+2 1.994 .427+0 –.504–5 .4368+1 1.093 .704+0 .667–1 .8492+1 1.105 .709+0 .664–1 .1948+1 1.995 .386+0 –.227–5 .6585+0 1.106 .658+0 .568–1
3000 .1374+2 1.969 .104+1 –.162–4 .4958+1 1.986 .697+0 –.358–5 .1386+1 0.917 .834+0 .984–1 .2678+1 0.929 .839+0 .979–1 .7904+0 1.988 .663+0 –.199–5 .1896+0 0.918 .801+0 .900–1
4000 .9386+1 1.959 .125+1 –.138–4 .2676+1 1.978 .929+0 –.231–5 .5794+0 0.783 .922+0 .128+0 .1114+1 0.795 .926+0 .128+0 .4022+0 1.979 .898+0 –.135–5 .7522–1 0.780 .891+0 .121+0
5000 .6689+1 1.949 .143+1 –.110–4 .1612+1 1.969 .113+1 –.941–6 .2857+0 0.677 .986+0 .156+0 .5475+0 0.690 .988+0 .156+0 .2337+0 1.970 .110+1 –.307–6 .3594–1 0.673 .957+0 .150+0
K, Z = 19 Shell 1s1/2 Eb = 3611 eV 2s1/2 Eb = 381 eV 2 p1/2 Eb = 299 eV 2 p3/2 Eb = 296 eV 3s1/2 Eb = 37 eV 3 p1/2 Eb = 19 eV
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Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables K, Z = 19 (continued) Shell 3 p3/2 Eb = 19 eV 4s1/2 Eb = 4 eV
σ β γ δ σ β γ δ
100 .7126+3 1.466 –.138–1 –.407–3 .2033+2 1.999 .120+0 .105–5
200 .2813+3 1.616 .932–2 .378–2 .7321+1 1.999 .345–1 –.190–5
500 .4781+2 1.567 .183+0 .110–1 .1561+1 2.000 –.382–1 –.206–5
1000 .8918+1 1.388 .404+0 .248–1 .4201+0 2.000 .731–1 –.202–5
E (eV) 1500 .2954+1 1.237 .553+0 .399–1 .1845+0 1.998 .228+0 –.229–5
2000 .1277+1 1.116 .663+0 .562–1 .9966–1 1.995 .381+0 –.185–5
3000 .3658+0 0.930 .805+0 .892–1 .3982–1 1.988 .661+0 –.179–5
4000 .1445+0 0.792 .894+0 .120+0 .2010–1 1.979 .896+0 –.120–5
5000 .6877–1 0.686 .959+0 .149+0 .1162–1 1.970 .110+1 –.276–6
100 .5510+2 1.996 –.214+0 –.207–4 .1999+3 1.996 .181+0 –.919–5 .4914+3 1.303 –.350–1 .892–2 .9887+3 1.307 –.353–1 .855–2 .2537+3 1.998 .121+0 –.337–5 .3906+3 1.459 –.956–2 –.495–3 .7859+3 1.458 –.997–2 –.661–3 .3611+2 1.999 .121+0 –.720–6
200 .5205+2 1.995 –.800–1 –.221–4 .1537+3 1.998 .379–1 –.107–4 .3039+3 1.425 .464–1 .132–1 .6080+3 1.433 .464–1 .132–1 .1185+3 1.998 .363–1 –.359–5 .1646+3 1.610 .559–3 .307–2 .3282+3 1.613 .857–3 .320–2 .1376+2 1.998 .462–1 –.709–6
500 .4374+2 1.992 .169+0 –.230–4 .8020+2 2.000 –.370–1 –.106–4 .9874+2 1.458 .246+0 .211–1 .1955+3 1.469 .248+0 .214–1 .3156+2 1.999 –.398–1 –.330–5 .3074+2 1.576 .163+0 .970–2 .6062+2 1.584 .165+0 .988–2 .2940+1 1.999 –.414–1 –.234–5
1000 .3335+2 1.987 .430+0 –.228–4 .3599+2 1.999 .819–1 –.901–5 .2739+2 1.352 .466+0 .343–1 .5373+2 1.364 .469+0 .346–1 .9413+1 2.000 .540–1 –.329–5 .6080+1 1.407 .386+0 .227–1 .1189+2 1.418 .390+0 .226–1 .8008+0 2.000 .480–1 –.222–5
E (eV) 1500 .2609+2 1.983 .622+0 –.222–4 .1966+2 1.997 .239+0 –.762–5 .1089+2 1.235 .608+0 .488–1 .2124+2 1.247 .613+0 .488–1 .4308+1 1.998 .199+0 –.315–5 .2084+1 1.264 .539+0 .374–1 .4054+1 1.276 .544+0 .371–1 .3544+0 1.998 .193+0 –.267–5
2000 .2081+2 1.978 .777+0 –.215–4 .1205+2 1.994 .391+0 –.656–5 .5264+1 1.129 .709+0 .636–1 .1022+2 1.142 .715+0 .634–1 .2388+1 1.996 .347+0 –.301–5 .9227+0 1.145 .653+0 .526–1 .1788+1 1.157 .659+0 .520–1 .1930+0 1.996 .341+0 –.276–5
3000 .1386+2 1.968 .103+1 –.194–4 .5579+1 1.987 .659+0 –.486–5 .1724+1 0.960 .848+0 .942–1 .3326+1 0.973 .854+0 .935–1 .9854+0 1.989 .619+0 –.268–5 .2722+0 0.963 .808+0 .843–1 .5245+0 0.975 .814+0 .834–1 .7820–1 1.989 .615+0 –.242–5
4000 .9687+1 1.958 .124+1 –.169–4 .3062+1 1.979 .889+0 –.343–5 .7361+0 0.827 .940+0 .123+0 .1413+1 0.841 .945+0 .122+0 .5067+0 1.981 .854+0 –.207–5 .1095+0 0.825 .906+0 .115+0 .2101+0 0.838 .910+0 .114+0 .3983–1 1.981 .852+0 –.186–5
5000 .7033+1 1.948 .142+1 –.140–4 .1868+1 1.970 .109+1 –.189–5 .3686+0 0.719 .101+1 .150+0 .7047+0 0.734 .101+1 .149+0 .2966+0 1.972 .106+1 –.100–5 .5287–1 0.716 .975+0 .143+0 .1010+0 0.729 .978+0 .142+0 .2318–1 1.972 .106+1 –.802–6
Ca, Z = 20 Shell 1s1/2 Eb = 4041 eV 2s1/2 Eb = 441 eV 2 p1/2 Eb = 353 eV 2 p3/2 Eb = 349 eV 3s1/2 Eb = 46 eV 3 p1/2 Eb = 28 eV 3 p3/2 Eb = 28 eV 4s1/2 Eb = 6 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
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Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Sc, Z = 21 Shell 1s1/2 Eb = 4494 eV 2s1/2 Eb = 503 eV 2 p1/2 Eb = 408 eV 2 p3/2 Eb = 403 eV 3s1/2 Eb = 55 eV 3 p1/2 Eb = 33 eV 3 p3/2 Eb = 33 eV 3d3/2 Eb = 8 eV 4s1/2 Eb = 6 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .4945+2 1.995 –.245+0 –.242–4 .1838+3 1.996 .214+0 –.104–4 .4514+3 1.282 –.498–1 .819–2 .9095+3 1.287 –.503–1 .780–2 .2580+3 1.998 .138+0 –.387–5 .4065+3 1.429 –.732–3 –.859–3 .8196+3 1.428 –.143–2 –.109–2 .8991+3 1.178 .556–1 .181–1 .4017+2 1.999 .131+0 –.101–5
200 .4699+2 1.994 –.108+0 –.258–4 .1448+3 1.997 .594–1 –.123–4 .2924+3 1.411 .302–1 .129–1 .5858+3 1.419 .301–1 .129–1 .1262+3 1.998 .525–1 –.439–5 .1823+3 1.600 –.837–2 .229–2 .3639+3 1.603 –.821–2 .241–2 .1578+3 1.275 .143+0 .274–1 .1544+2 1.998 .616–1 –.655–6
500 .4018+2 1.992 .148+0 –.268–4 .7949+2 1.999 –.416–1 –.126–4 .1035+3 1.460 .231+0 .207–1 .2051+3 1.472 .232+0 .210–1 .3521+2 1.999 –.420–1 –.411–5 .3664+2 1.589 .142+0 .858–2 .7226+2 1.598 .143+0 .881–2 .1026+2 1.090 .314+0 .514–1 .3391+1 1.999 –.429–1 –.270–5
1000 .3137+2 1.987 .411+0 –.267–4 .3740+2 2.000 .574–1 –.110–4 .3072+2 1.371 .456+0 .333–1 .6026+2 1.385 .460+0 .335–1 .1076+2 2.000 .314–1 –.415–5 .7560+1 1.435 .368+0 .205–1 .1477+2 1.447 .372+0 .205–1 .9582+0 0.821 .457+0 .935–1 .9326+0 2.000 .264–1 –.320–5
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E (eV) 1500 .2501+2 1.982 .605+0 –.260–4 .2100+2 1.998 .206+0 –.955–5 .1268+2 1.263 .605+0 .469–1 .2470+2 1.278 .611+0 .469–1 .4983+1 1.999 .167+0 –.408–5 .2651+1 1.299 .527+0 .344–1 .5151+1 1.312 .532+0 .341–1 .2126+0 0.666 .547+0 .134+0 .4155+0 1.999 .161+0 –.323–5
2000 .2029+2 1.977 .761+0 –.252–4 .1312+2 1.995 .354+0 –.838–5 .6277+1 1.164 .712+0 .609–1 .1218+2 1.178 .719+0 .606–1 .2789+1 1.996 .308+0 –.395–5 .1194+1 1.185 .645+0 .487–1 .2310+1 1.198 .651+0 .482–1 .6890–1 0.562 .611+0 .171+0 .2279+0 1.996 .302+0 –.354–5
3000 .1389+2 1.968 .102+1 –.231–4 .6223+1 1.988 .620+0 –.647–5 .2118+1 1.000 .860+0 .901–1 .4080+1 1.015 .867+0 .894–1 .1168+1 1.990 .575+0 –.357–5 .3602+0 1.007 .812+0 .790–1 .6926+0 1.021 .819+0 .781–1 .1308–1 0.418 .671+0 .237+0 .9350–1 1.990 .571+0 –.324–5
4000 .9918+1 1.958 .123+1 –.205–4 .3470+1 1.980 .850+0 –.485–5 .9218+0 0.869 .958+0 .118+0 .1766+1 0.884 .964+0 .117+0 .6068+0 1.982 .810+0 –.295–5 .1468+0 0.870 .919+0 .108+0 .2809+0 0.883 .925+0 .107+0 .3893–2 0.336 .686+0 .294+0 .4803–1 1.982 .808+0 –.272–5
5000 .7328+1 1.948 .141+1 –.176–4 .2142+1 1.971 .105+1 –.316–5 .4681+0 0.762 .103+1 .144+0 .8928+0 0.777 .103+1 .143+0 .3578+0 1.973 .102+1 –.189–5 .7152–1 0.759 .993+0 .136+0 .1363+0 0.773 .997+0 .134+0 .1504–2 0.286 .697+0 .344+0 .2813–1 1.973 .101+1 –.177–5
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Ti, Z = 22 Shell 1s1/2 Eb = 4970 eV 2s1/2 Eb = 567 eV 2 p1/2 Eb = 465 eV 2 p3/2 Eb = 459 eV 3s1/2 Eb = 64 eV 3 p1/2 Eb = 39 eV 3 p3/2 Eb = 38 eV 3d3/2 Eb = 8 eV 4s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .4464+2 1.995 –.277+0 –.282–4 .1699+3 1.995 .248+0 –.116–4 .4171+3 1.260 –.645–1 .733–2 .8412+3 1.265 –.651–1 .692–2 .2592+3 1.998 .155+0 –.434–5 .4115+3 1.396 .119–1 –.881–3 .8377+3 1.394 .108–1 –.118–2 .1193+4 1.131 .448–1 .171–1 .4275+2 1.998 .142+0 –.122–5
200 .4263+2 1.994 –.137+0 –.300–4 .1366+3 1.997 .836–1 –.140–4 .2811+3 1.395 .131–1 .125–1 .5637+3 1.404 .128–1 .125–1 .1323+3 1.998 .701–1 –.525–5 .1963+3 1.587 –.144–1 .155–2 .3941+3 1.590 –.143–1 .165–2 .2235+3 1.264 .128+0 .265–1 .1656+2 1.998 .774–1 –.594–6
500 .3700+2 1.991 .124+0 –.312–4 .7846+2 1.999 –.430–1 –.148–4 .1075+3 1.460 .214+0 .204–1 .2131+3 1.473 .216+0 .207–1 .3866+2 1.999 –.413–1 –.507–5 .4256+2 1.600 .120+0 .758–2 .8409+2 1.609 .121+0 .785–2 .1538+2 1.124 .308+0 .493–1 .3752+1 1.999 –.411–1 –.304–5
1000 .2950+2 1.986 .391+0 –.311–4 .3857+2 2.000 .349–1 –.133–4 .3400+2 1.387 .445+0 .323–1 .6667+2 1.402 .449+0 .325–1 .1211+2 2.000 .109–1 –.514–5 .9165+1 1.461 .349+0 .186–1 .1791+2 1.474 .352+0 .186–1 .1490+1 0.863 .460+0 .892–1 .1047+1 2.000 .603–2 –.407–5
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E (eV) 1500 .2393+2 1.981 .586+0 –.304–4 .2223+2 1.998 .174+0 –.118–4 .1453+2 1.289 .600+0 .452–1 .2830+2 1.304 .606+0 .451–1 .5673+1 1.999 .135+0 –.516–5 .3285+1 1.331 .512+0 .316–1 .6378+1 1.345 .518+0 .313–1 .3383+0 0.705 .552+0 .128+0 .4694+0 1.999 .130+0 –.432–5
2000 .1970+2 1.977 .744+0 –.295–4 .1414+2 1.996 .317+0 –.105–4 .7366+1 1.196 .712+0 .584–1 .1427+2 1.212 .720+0 .581–1 .3203+1 1.997 .271+0 –.507–5 .1503+1 1.222 .636+0 .452–1 .2904+1 1.236 .642+0 .446–1 .1118+0 0.600 .620+0 .165+0 .2590+0 1.997 .265+0 –.434–5
3000 .1383+2 1.967 .100+1 –.273–4 .6868+1 1.989 .580+0 –.841–5 .2560+1 1.038 .869+0 .863–1 .4923+1 1.054 .877+0 .855–1 .1360+1 1.991 .531+0 –.468–5 .4633+0 1.048 .812+0 .740–1 .8892+0 1.063 .820+0 .730–1 .2171–1 0.452 .695+0 .230+0 .1074+0 1.991 .525+0 –.439–5
4000 .1008+2 1.957 .121+1 –.247–4 .3889+1 1.981 .810+0 –.660–5 .1135+1 0.909 .973+0 .113+0 .2170+1 0.926 .981+0 .112+0 .7134+0 1.983 .765+0 –.404–5 .1914+0 0.912 .928+0 .102+0 .3654+0 0.927 .935+0 .101+0 .6512–2 0.359 .720+0 .287+0 .5567–1 1.983 .762+0 –.371–5
5000 .7566+1 1.947 .140+1 –.216–4 .2427+1 1.973 .102+1 –.475–5 .5840+0 0.802 .105+1 .139+0 .1111+1 0.818 .106+1 .137+0 .4236+0 1.975 .975+0 –.297–5 .9409–1 0.800 .101+1 .129+0 .1788+0 0.816 .101+1 .127+0 .2524–2 0.301 .729+0 .336+0 .3280–1 1.975 .969+0 –.267–5
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables V, Z = 23 Shell 1s1/2 Eb = 5470 eV 2s1/2 Eb = 633 eV 2 p1/2 Eb = 525 eV 2 p3/2 Eb = 518 eV 3s1/2 Eb = 72 eV 3 p1/2 Eb = 44 eV 3 p3/2 Eb = 43 eV 3d3/2 Eb = 8 eV 4s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .4049+2 1.994 –.310+0 –.328–4 .1578+3 1.994 .283+0 –.129–4 .3863+3 1.238 –.786–1 .639–2 .7800+3 1.243 –.794–1 .597–2 .2598+3 1.998 .172+0 –.470–5 .4136+3 1.361 .278–1 –.451–3 .8439+3 1.358 .262–1 –.838–3 .1499+4 1.083 .361–1 .162–1 .4499+2 1.998 .151+0 –.120–5
200 .3883+2 1.993 –.167+0 –.348–4 .1291+3 1.996 .110+0 –.158–4 .2695+3 1.380 –.456–2 .119–1 .5410+3 1.389 –.502–2 .119–1 .1375+3 1.998 .882–1 –.612–5 .2086+3 1.572 –.168–1 .886–3 .4193+3 1.574 –.171–1 .959–3 .3002+3 1.247 .112+0 .256–1 .1747+2 1.998 .927–1 –.682–6
500 .3413+2 1.990 .993–1 –.362–4 .7718+2 1.999 –.414–1 –.173–4 .1105+3 1.459 .196+0 .201–1 .2193+3 1.472 .198+0 .204–1 .4198+2 1.999 –.378–1 –.618–5 .4857+2 1.608 .981–1 .666–2 .9597+2 1.617 .996–1 .698–2 .2191+2 1.153 .298+0 .474–1 .4063+1 1.999 –.359–1 –.346–5
1000 .2773+2 1.986 .371+0 –.361–4 .3950+2 2.000 .147–1 –.159–4 .3714+2 1.400 .431+0 .314–1 .7282+2 1.416 .436+0 .316–1 .1348+2 2.000 –.726–2 –.630–5 .1091+2 1.484 .327+0 .167–1 .2130+2 1.497 .331+0 .168–1 .2195+1 0.903 .462+0 .853–1 .1152+1 2.000 –.128–1 –.485–5
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E (eV) 1500 .2285+2 1.981 .568+0 –.353–4 .2334+2 1.999 .144+0 –.144–4 .1642+2 1.311 .592+0 .436–1 .3196+2 1.328 .599+0 .436–1 .6384+1 1.999 .106+0 –.642–5 .3991+1 1.361 .496+0 .290–1 .7739+1 1.376 .502+0 .287–1 .5086+0 0.742 .558+0 .123+0 .5199+0 1.999 .992–1 –.531–5
2000 .1907+2 1.976 .726+0 –.344–4 .1510+2 1.996 .281+0 –.130–4 .8516+1 1.225 .710+0 .562–1 .1649+2 1.242 .719+0 .559–1 .3632+1 1.997 .235+0 –.639–5 .1853+1 1.256 .624+0 .419–1 .3574+1 1.272 .631+0 .414–1 .1709+0 0.636 .627+0 .158+0 .2883+0 1.997 .227+0 –.552–5
3000 .1369+2 1.966 .986+0 –.321–4 .7508+1 1.990 .540+0 –.107–4 .3047+1 1.073 .876+0 .828–1 .5850+1 1.090 .886+0 .819–1 .1562+1 1.992 .488+0 –.602–5 .5830+0 1.087 .809+0 .693–1 .1116+1 1.103 .818+0 .683–1 .3401–1 0.485 .714+0 .222+0 .1207+0 1.992 .482+0 –.547–5
4000 .1016+2 1.957 .120+1 –.294–4 .4316+1 1.982 .769+0 –.873–5 .1375+1 0.947 .987+0 .109+0 .2624+1 0.965 .996+0 .108+0 .8268+0 1.985 .720+0 –.538–5 .2441+0 0.952 .934+0 .964–1 .4648+0 0.968 .943+0 .950–1 .1031–1 0.387 .751+0 .279+0 .6304–1 1.985 .715+0 –.506–5
5000 .7751+1 1.947 .138+1 –.262–4 .2723+1 1.974 .975+0 –.671–5 .7170+0 0.840 .107+1 .133+0 .1361+1 0.858 .108+1 .132+0 .4943+0 1.976 .930+0 –.430–5 .1211+0 0.841 .102+1 .122+0 .2295+0 0.857 .103+1 .121+0 .4012–2 0.319 .762+0 .328+0 .3738–1 1.977 .923+0 –.403–5
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Cr, Z = 24 Shell 1s1/2 Eb = 5995 eV 2s1/2 Eb = 702 eV 2 p1/2 Eb = 589 eV 2 p3/2 Eb = 580 eV 3s1/2 Eb = 80 eV 3 p1/2 Eb = 49 eV 3 p3/2 Eb = 48 eV 3d3/2 Eb = 8 eV 3d5/2 Eb = 8 eV 4s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3691+2 1.994 –.350+0 –.379–4 .1474+3 1.993 .333+0 –.141–4 .3624+3 1.207 –.932–1 .530–2 .7336+3 1.212 –.941–1 .483–2 .2537+3 1.997 .195+0 –.483–5 .3943+3 1.306 .524–1 .518–3 .8070+3 1.302 .499–1 –.166–4 .1640+4 1.015 .315–1 .162–1 .2438+4 1.021 .320–1 .161–1 .3464+2 1.998 .162+0 .612–6
200 .3554+2 1.993 –.204+0 –.405–4 .1226+3 1.995 .146+0 –.179–4 .2607+3 1.359 –.253–1 .112–1 .5244+3 1.368 –.260–1 .112–1 .1398+3 1.997 .112+0 –.704–5 .2140+3 1.549 –.155–1 .146–3 .4308+3 1.550 –.161–1 .177–3 .3537+3 1.216 .971–1 .251–1 .5244+3 1.217 .978–1 .251–1 .1347+2 1.998 .113+0 –.211–5
500 .3160+2 1.990 .697–1 –.420–4 .7594+2 1.998 –.362–1 –.201–4 .1137+3 1.455 .176+0 .198–1 .2260+3 1.470 .177+0 .201–1 .4468+2 1.998 –.311–1 –.746–5 .5384+2 1.614 .752–1 .574–2 .1063+3 1.623 .766–1 .611–2 .2701+2 1.176 .286+0 .460–1 .3987+2 1.170 .286+0 .463–1 .3240+1 1.998 –.268–1 –.504–5
1000 .2611+2 1.985 .345+0 –.417–4 .4033+2 2.000 –.434–2 –.189–4 .4038+2 1.412 .415+0 .307–1 .7923+2 1.430 .420+0 .309–1 .1469+2 2.000 –.240–1 –.763–5 .1260+2 1.506 .302+0 .151–1 .2456+2 1.520 .307+0 .152–1 .2759+1 0.944 .465+0 .821–1 .4056+1 0.938 .464+0 .829–1 .9352+0 2.000 –.280–1 –.628–5
120
E (eV) 1500 .2181+2 1.980 .544+0 –.410–4 .2439+2 1.999 .113+0 –.173–4 .1843+2 1.333 .582+0 .422–1 .3587+2 1.352 .590+0 .421–1 .7032+1 1.999 .766–1 –.788–5 .4694+1 1.391 .477+0 .264–1 .9083+1 1.407 .484+0 .262–1 .6476+0 0.780 .564+0 .118+0 .9494+0 0.776 .563+0 .119+0 .4259+0 1.999 .704–1 –.667–5
2000 .1842+2 1.975 .706+0 –.400–4 .1604+2 1.997 .245+0 –.159–4 .9763+1 1.252 .707+0 .544–1 .1889+2 1.271 .716+0 .540–1 .4028+1 1.998 .199+0 –.792–5 .2206+1 1.290 .611+0 .389–1 .4246+1 1.307 .619+0 .384–1 .2201+0 0.672 .636+0 .153+0 .3221+0 0.672 .635+0 .153+0 .2374+0 1.998 .190+0 –.656–5
3000 .1351+2 1.966 .969+0 –.377–4 .8153+1 1.991 .499+0 –.135–4 .3591+1 1.106 .882+0 .794–1 .6886+1 1.125 .892+0 .785–1 .1750+1 1.993 .445+0 –.765–5 .7069+0 1.123 .804+0 .648–1 .1350+1 1.141 .814+0 .637–1 .4468–1 0.520 .731+0 .215+0 .6512–1 0.527 .733+0 .216+0 .1002+0 1.993 .439+0 –.697–5
4000 .1020+2 1.956 .118+1 –.349–4 .4755+1 1.984 .728+0 –.113–4 .1649+1 0.983 .999+0 .104+0 .3142+1 1.002 .101+1 .103+0 .9345+0 1.986 .674+0 –.700–5 .2997+0 0.991 .938+0 .909–1 .5687+0 1.009 .947+0 .894–1 .1370–1 0.417 .778+0 .271+0 .1990–1 0.431 .784+0 .272+0 .5274–1 1.986 .669+0 –.650–5
5000 .7893+1 1.946 .137+1 –.316–4 .3032+1 1.975 .933+0 –.913–5 .8705+0 0.878 .108+1 .128+0 .1649+1 0.897 .109+1 .127+0 .5624+0 1.978 .882+0 –.597–5 .1500+0 0.883 .103+1 .116+0 .2831+0 0.901 .104+1 .115+0 .5358–2 0.343 .796+0 .320+0 .7761–2 0.362 .806+0 .320+0 .3145–1 1.978 .876+0 –.547–5
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Mn, Z = 25 Shell 1s1/2 Eb = 6544 eV 2s1/2 Eb = 775 eV 2 p1/2 Eb = 656 eV 2 p3/2 Eb = 645 eV 3s1/2 Eb = 89 eV 3 p1/2 Eb = 55 eV 3 p3/2 Eb = 53 eV 3d3/2 Eb = 9 eV 3d5/2 Eb = 9 eV 4s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3373+2 1.993 –.379+0 –.441–4 .1367+3 1.993 .359+0 –.157–4 .3328+3 1.193 –.104+0 .451–2 .6748+3 1.198 –.105+0 .404–2 .2550+3 1.997 .205+0 –.506–5 .4023+3 1.282 .658–1 .204–2 .8311+3 1.278 .625–1 .141–2 .2091+4 0.986 .241–1 .150–1 .3113+4 0.992 .246–1 .148–1 .4804+2 1.998 .164+0 –.593–6
200 .3256+2 1.992 –.231+0 –.467–4 .1154+3 1.994 .169+0 –.200–4 .2459+3 1.346 –.400–1 .105–1 .4956+3 1.356 –.410–1 .105–1 .1444+3 1.997 .126+0 –.799–5 .2252+3 1.536 –.110–1 –.438–4 .4562+3 1.537 –.119–1 –.557–4 .4812+3 1.201 .852–1 .240–1 .7145+3 1.202 .860–1 .240–1 .1876+2 1.997 .122+0 –.113–5
500 .2923+2 1.989 .457–1 –.484–4 .7385+2 1.998 –.291–1 –.231–4 .1139+3 1.451 .158+0 .194–1 .2266+3 1.467 .159+0 .198–1 .4794+2 1.998 –.231–1 –.890–5 .6021+2 1.617 .576–1 .499–2 .1193+3 1.627 .588–1 .540–2 .3981+2 1.193 .273+0 .443–1 .5885+2 1.186 .273+0 .446–1 .4569+1 1.998 –.183–1 –.504–5
1000 .2452+2 1.984 .326+0 –.483–4 .4065+2 2.000 –.184–1 –.222–4 .4280+2 1.420 .401+0 .301–1 .8402+2 1.439 .405+0 .303–1 .1619+2 1.999 –.358–1 –.923–5 .1475+2 1.522 .280+0 .136–1 .2878+2 1.537 .284+0 .138–1 .4268+1 0.976 .462+0 .786–1 .6281+1 0.968 .460+0 .794–1 .1338+1 1.999 –.404–1 –.693–5
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E (eV) 1500 .2075+2 1.980 .527+0 –.475–4 .2516+2 1.999 .876–1 –.207–4 .2018+2 1.348 .572+0 .410–1 .3928+2 1.368 .579+0 .409–1 .7847+1 1.999 .525–1 –.958–5 .5617+1 1.413 .458+0 .242–1 .1087+2 1.431 .464+0 .241–1 .1025+1 0.815 .568+0 .113+0 .1504+1 0.810 .567+0 .114+0 .6130+0 1.999 .452–1 –.787–5
2000 .1773+2 1.975 .689+0 –.464–4 .1682+2 1.997 .212+0 –.192–4 .1094+2 1.273 .700+0 .524–1 .2115+2 1.294 .710+0 .520–1 .4531+1 1.998 .167+0 –.972–5 .2678+1 1.317 .595+0 .358–1 .5152+1 1.335 .603+0 .354–1 .3540+0 0.704 .643+0 .147+0 .5183+0 0.703 .642+0 .148+0 .3433+0 1.998 .160+0 –.856–5
3000 .1325+2 1.965 .953+0 –.438–4 .8739+1 1.992 .461+0 –.166–4 .4142+1 1.135 .883+0 .766–1 .7933+1 1.155 .895+0 .755–1 .1991+1 1.994 .405+0 –.952–5 .8753+0 1.157 .797+0 .608–1 .1669+1 1.175 .807+0 .597–1 .7357–1 0.550 .742+0 .208+0 .1073+0 0.556 .744+0 .209+0 .1461+0 1.994 .398+0 –.856–5
4000 .1017+2 1.955 .117+1 –.409–4 .5173+1 1.985 .687+0 –.143–4 .1938+1 1.016 .101+1 .101+0 .3685+1 1.037 .102+1 .991–1 .1072+1 1.987 .630+0 –.892–5 .3761+0 1.027 .937+0 .857–1 .7126+0 1.046 .948+0 .842–1 .2291–1 0.446 .799+0 .263+0 .3330–1 0.459 .804+0 .264+0 .7742–1 1.987 .624+0 –.830–5
5000 .7974+1 1.945 .135+1 –.375–4 .3334+1 1.977 .890+0 –.120–4 .1036+1 0.915 .110+1 .124+0 .1960+1 0.936 .111+1 .122+0 .6497+0 1.979 .836+0 –.788–5 .1901+0 0.920 .104+1 .110+0 .3582+0 0.939 .105+1 .108+0 .9038–2 0.367 .825+0 .312+0 .1310–1 0.385 .834+0 .312+0 .4644–1 1.980 .829+0 –.740–5
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Fe, Z = 26 Shell 1s1/2 Eb = 7117 eV 2s1/2 Eb = 851 eV 2 p1/2 Eb = 727 eV 2 p3/2 Eb = 714 eV 3s1/2 Eb = 99 eV 3 p1/2 Eb = 61 eV 3 p3/2 Eb = 59 eV 3d3/2 Eb = 9 eV 3d5/2 Eb = 9 eV 4s1/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3095+2 1.992 –.415+0 –.510–4 .1276+3 1.992 .398+0 –.172–4 .3096+3 1.171 –.114+0 .369–2 .6287+3 1.175 –.116+0 .320–2 .2492+3 1.997 .222+0 –.497–5 .3911+3 1.239 .857–1 .419–2 .8104+3 1.235 .817–1 .341–2 .2368+4 0.937 .198–1 .145–1 .3526+4 0.944 .203–1 .142–1 .4856+2 1.998 .170+0 –.410–8
200 .2997+2 1.991 –.264+0 –.540–4 .1091+3 1.994 .202+0 –.224–4 .2343+3 1.329 –.574–1 .960–2 .4730+3 1.339 –.587–1 .963–2 .1458+3 1.997 .146+0 –.894–5 .2300+3 1.515 –.267–2 –.220–3 .4668+3 1.515 –.405–2 –.294–3 .5844+3 1.173 .738–1 .233–1 .8673+3 1.175 .747–1 .233–1 .1915+2 1.997 .136+0 –.145–5
500 .2714+2 1.988 .174–1 –.559–4 .7193+2 1.997 –.187–1 –.265–4 .1144+3 1.446 .138+0 .191–1 .2279+3 1.463 .139+0 .195–1 .5049+2 1.997 –.124–1 –.106–4 .6570+2 1.618 .397–1 .423–2 .1302+3 1.628 .408–1 .469–2 .5152+2 1.206 .257+0 .430–1 .7609+2 1.199 .257+0 .433–1 .4772+1 1.997 –.669–2 –.616–5
1000 .2306+2 1.984 .303+0 –.558–4 .4090+2 1.999 –.312–1 –.260–4 .4527+2 1.427 .384+0 .295–1 .8890+2 1.447 .388+0 .297–1 .1750+2 1.999 –.461–1 –.111–4 .1680+2 1.538 .255+0 .122–1 .3277+2 1.554 .259+0 .125–1 .5713+1 1.009 .457+0 .756–1 .8398+1 1.000 .456+0 .764–1 .1420+1 1.999 –.491–1 –.845–5
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E (eV) 1500 .1975+2 1.979 .506+0 –.549–4 .2587+2 1.999 .626–1 –.245–4 .2201+2 1.363 .559+0 .398–1 .4283+2 1.384 .567+0 .397–1 .8588+1 1.999 .289–1 –.116–4 .6532+1 1.436 .436+0 .220–1 .1263+2 1.455 .443+0 .220–1 .1394+1 0.852 .572+0 .109+0 .2043+1 0.846 .571+0 .110+0 .6563+0 1.999 .225–1 –.965–5
2000 .1705+2 1.974 .668+0 –.537–4 .1756+2 1.998 .180+0 –.230–4 .1218+2 1.294 .692+0 .509–1 .2353+2 1.316 .702+0 .504–1 .4996+1 1.999 .135+0 –.118–4 .3155+1 1.345 .578+0 .332–1 .6059+1 1.364 .587+0 .327–1 .4875+0 0.737 .650+0 .141+0 .7126+0 0.735 .648+0 .143+0 .3696+0 1.999 .128+0 –.104–4
3000 .1297+2 1.964 .936+0 –.509–4 .9321+1 1.993 .422+0 –.202–4 .4742+1 1.162 .884+0 .738–1 .9071+1 1.184 .897+0 .727–1 .2218+1 1.994 .366+0 –.117–4 .1049+1 1.188 .787+0 .569–1 .1997+1 1.209 .799+0 .559–1 .1032+0 0.580 .754+0 .201+0 .1503+0 0.585 .755+0 .202+0 .1585+0 1.995 .358+0 –.107–4
4000 .1010+2 1.955 .115+1 –.479–4 .5596+1 1.986 .646+0 –.178–4 .2259+1 1.047 .102+1 .968–1 .4288+1 1.070 .103+1 .952–1 .1204+1 1.988 .586+0 –.112–4 .4566+0 1.062 .935+0 .809–1 .8627+0 1.082 .947+0 .793–1 .3258–1 0.475 .818+0 .256+0 .4728–1 0.486 .822+0 .257+0 .8448–1 1.988 .579+0 –.104–4
5000 .8022+1 1.945 .134+1 –.443–4 .3644+1 1.978 .848+0 –.153–4 .1223+1 0.948 .111+1 .120+0 .2308+1 0.971 .113+1 .118+0 .7339+0 1.981 .790+0 –.102–4 .2328+0 0.956 .104+1 .105+0 .4374+0 0.976 .106+1 .103+0 .1297–1 0.393 .852+0 .304+0 .1876–1 0.410 .860+0 .305+0 .5095–1 1.981 .783+0 –.962–5
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Co, Z = 27 Shell 1s1/2 Eb = 7715 eV 2s1/2 Eb = 931 eV 2 p1/2 Eb = 800 eV 2 p3/2 Eb = 785 eV 3s1/2 Eb = 107 eV 3 p1/2 Eb = 68 eV 3 p3/2 Eb = 66 eV 3d3/2 Eb = 9 eV 3d5/2 Eb = 9 eV 4s1/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2850+2 1.991 –.451+0 –.588–4 .1193+3 1.991 .439+0 –.187–4 .2888+3 1.149 –.123+0 .302–2 .5875+3 1.153 –.125+0 .250–2 .2453+3 1.997 .236+0 –.456–5 .3757+3 1.195 .105+0 .698–2 .7813+3 1.190 .101+0 .603–2 .2615+4 0.890 .165–1 .140–1 .3893+4 0.898 .170–1 .137–1 .4925+2 1.998 .174+0 .814–6
200 .2767+2 1.990 –.299+0 –.623–4 .1032+3 1.993 .236+0 –.250–4 .2234+3 1.312 –.742–1 .867–2 .4517+3 1.322 –.758–1 .871–2 .1475+3 1.996 .165+0 –.978–5 .2320+3 1.492 .909–2 –.141–3 .4720+3 1.492 .709–2 –.295–3 .6929+3 1.143 .638–1 .227–1 .1028+4 1.146 .648–1 .226–1 .1955+2 1.997 .150+0 –.177–5
500 .2524+2 1.988 –.119–1 –.645–4 .6987+2 1.996 –.566–2 –.303–4 .1144+3 1.440 .118+0 .186–1 .2282+3 1.457 .119+0 .191–1 .5299+2 1.997 .167–3 –.124–4 .7077+2 1.618 .238–1 .352–2 .1403+3 1.628 .247–1 .402–2 .6518+2 1.214 .241+0 .419–1 .9618+2 1.207 .241+0 .421–1 .4964+1 1.997 .642–2 –.736–5
1000 .2171+2 1.983 .278+0 –.644–4 .4096+2 1.999 –.415–1 –.304–4 .4751+2 1.432 .365+0 .289–1 .9335+2 1.453 .370+0 .292–1 .1882+2 1.999 –.535–1 –.132–4 .1891+2 1.551 .230+0 .110–1 .3686+2 1.568 .234+0 .114–1 .7480+1 1.039 .450+0 .728–1 .1098+2 1.029 .449+0 .736–1 .1498+1 1.999 –.551–1 –.103–4
123
E (eV) 1500 .1879+2 1.978 .482+0 –.631–4 .2644+2 1.999 .394–1 –.288–4 .2379+2 1.376 .544+0 .389–1 .4629+2 1.400 .553+0 .388–1 .9344+1 1.999 .747–2 –.138–4 .7507+1 1.458 .413+0 .201–1 .1449+2 1.478 .420+0 .202–1 .1856+1 0.885 .574+0 .105+0 .2715+1 0.878 .572+0 .106+0 .6987+0 1.999 .171–2 –.117–4
2000 .1637+2 1.973 .648+0 –.619–4 .1822+2 1.998 .150+0 –.273–4 .1343+2 1.312 .682+0 .493–1 .2594+2 1.336 .693+0 .489–1 .5476+1 1.999 .105+0 –.142–4 .3673+1 1.370 .560+0 .306–1 .7043+1 1.391 .569+0 .302–1 .6558+0 0.770 .656+0 .136+0 .9572+0 0.766 .654+0 .138+0 .3956+0 1.999 .976–1 –.123–4
3000 .1266+2 1.964 .916+0 –.590–4 .9873+1 1.993 .383+0 –.245–4 .5373+1 1.187 .882+0 .713–1 .1027+2 1.212 .896+0 .701–1 .2454+1 1.995 .326+0 –.143–4 .1243+1 1.219 .777+0 .532–1 .2359+1 1.241 .789+0 .522–1 .1412+0 0.611 .765+0 .195+0 .2053+0 0.614 .765+0 .196+0 .1708+0 1.995 .318+0 –.131–4
4000 .9997+1 1.954 .113+1 –.558–4 .6011+1 1.987 .604+0 –.219–4 .2604+1 1.076 .102+1 .934–1 .4936+1 1.100 .104+1 .917–1 .1341+1 1.989 .543+0 –.138–4 .5472+0 1.094 .931+0 .763–1 .1031+1 1.116 .944+0 .747–1 .4516–1 0.503 .835+0 .248+0 .6542–1 0.513 .838+0 .249+0 .9155–1 1.990 .535+0 –.128–4
5000 .8033+1 1.944 .132+1 –.521–4 .3955+1 1.979 .806+0 –.193–4 .1428+1 0.979 .112+1 .115+0 .2689+1 1.004 .114+1 .113+0 .8226+0 1.982 .744+0 –.129–4 .2815+0 0.990 .105+1 .992–1 .5274+0 1.012 .106+1 .972–1 .1814–1 0.419 .875+0 .296+0 .2619–1 0.435 .882+0 .297+0 .5549–1 1.983 .737+0 –.121–4
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Ni, Z = 28 Shell 1s1/2 Eb = 8338 eV 2s1/2 Eb = 1015 eV 2 p1/2 Eb = 877 eV 2 p3/2 Eb = 860 eV 3s1/2 Eb = 117 eV 3 p1/2 Eb = 75 eV 3 p3/2 Eb = 73 eV 3d3/2 Eb = 10 eV 3d5/2 Eb = 10 eV 4s1/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2631+2 1.991 –.488+0 –.677–4 .1116+3 1.990 .481+0 –.202–4 .2697+3 1.127 –.131+0 .255–2 .5493+3 1.131 –.132+0 .200–2 .2387+3 1.996 .251+0 –.385–5 .3593+3 1.148 .123+0 .104–1 .7502+3 1.142 .117+0 .922–2 .2797+4 0.842 .140–1 .138–1 .4164+4 0.851 .145–1 .134–1 .4970+2 1.997 .176+0 .191–5
200 .2561+2 1.990 –.334+0 –.719–4 .9755+2 1.992 .272+0 –.278–4 .2128+3 1.294 –.903–1 .771–2 .4307+3 1.304 –.923–1 .777–2 .1476+3 1.996 .184+0 –.106–4 .2324+3 1.468 .239–1 .239–3 .4741+3 1.467 .212–1 –.103–4 .8005+3 1.112 .555–1 .222–1 .1187+4 1.116 .565–1 .221–1 .1990+2 1.997 .163+0 –.198–5
500 .2352+2 1.987 –.422–1 –.743–4 .6772+2 1.996 .998–2 –.345–4 .1138+3 1.432 .972–1 .182–1 .2272+3 1.451 .977–1 .187–1 .5511+2 1.997 .144–1 –.144–4 .7552+2 1.616 .990–2 .285–2 .1499+3 1.626 .106–1 .338–2 .8069+2 1.218 .225+0 .409–1 .1190+3 1.212 .226+0 .411–1 .5137+1 1.997 .208–1 –.866–5
1000 .2045+2 1.982 .253+0 –.741–4 .4085+2 1.999 –.491–1 –.353–4 .4946+2 1.435 .346+0 .284–1 .9724+2 1.458 .351+0 .287–1 .2007+2 1.998 –.583–1 –.156–4 .2106+2 1.563 .205+0 .981–2 .4105+2 1.580 .209+0 .103–1 .9595+1 1.066 .441+0 .704–1 .1407+2 1.056 .440+0 .712–1 .1573+1 1.998 –.585–1 –.125–4
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E (eV) 1500 .1787+2 1.977 .460+0 –.727–4 .2689+2 1.999 .186–1 –.338–4 .2548+2 1.387 .528+0 .380–1 .4958+2 1.412 .537+0 .379–1 .1009+2 1.999 –.114–1 –.164–4 .8540+1 1.477 .389+0 .183–1 .1647+2 1.497 .396+0 .185–1 .2420+1 0.917 .573+0 .101+0 .3536+1 0.909 .571+0 .102+0 .7396+0 1.999 –.171–1 –.140–4
2000 .1570+2 1.972 .627+0 –.714–4 .1880+2 1.998 .121+0 –.323–4 .1467+2 1.328 .670+0 .480–1 .2833+2 1.354 .682+0 .475–1 .5959+1 1.999 .775–1 –.169–4 .4233+1 1.393 .539+0 .282–1 .8104+1 1.415 .549+0 .279–1 .8645+0 0.801 .661+0 .132+0 .1260+1 0.796 .659+0 .133+0 .4209+0 1.999 .687–1 –.145–4
3000 .1233+2 1.963 .897+0 –.682–4 .1039+2 1.994 .346+0 –.293–4 .6027+1 1.210 .878+0 .689–1 .1150+2 1.237 .893+0 .677–1 .2696+1 1.996 .289+0 –.173–4 .1456+1 1.247 .764+0 .498–1 .2759+1 1.270 .777+0 .487–1 .1891+0 0.639 .775+0 .188+0 .2744+0 0.641 .775+0 .190+0 .1830+0 1.996 .280+0 –.157–4
4000 .9859+1 1.953 .112+1 –.650–4 .6413+1 1.988 .563+0 –.267–4 .2973+1 1.103 .102+1 .899–1 .5625+1 1.129 .104+1 .880–1 .1484+1 1.990 .500+0 –.170–4 .6485+0 1.124 .924+0 .717–1 .1219+1 1.148 .939+0 .700–1 .6122–1 0.531 .849+0 .241+0 .8851–1 0.539 .852+0 .242+0 .9859–1 1.991 .493+0 –.155–4
5000 .8011+1 1.943 .131+1 –.609–4 .4263+1 1.981 .764+0 –.238–4 .1651+1 1.008 .113+1 .111+0 .3102+1 1.035 .115+1 .109+0 .9152+0 1.984 .699+0 –.160–4 .3366+0 1.022 .105+1 .941–1 .6287+0 1.046 .106+1 .920–1 .2482–1 0.445 .895+0 .288+0 .3576–1 0.460 .902+0 .289+0 .6003–1 1.984 .691+0 –.149–4
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Cu, Z = 29 Shell 1s1/2 Eb = 8986 eV 2s1/2 Eb = 1103 eV 2 p1/2 Eb = 958 eV 2 p3/2 Eb = 938 eV 3s1/2 Eb = 127 eV 3 p1/2 Eb = 82 eV 3 p3/2 Eb = 80 eV 3d3/2 Eb = 11 eV 3d5/2 Eb = 10 eV 4s1/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2435+2 1.990 –.530+0 –.772–4 .1048+3 1.989 .538+0 –.213–4 .2542+3 1.096 –.135+0 .266–2 .5190+3 1.099 –.137+0 .203–2 .2278+3 1.996 .271+0 –.194–5 .3262+3 1.074 .145+0 .154–1 .6848+3 1.067 .138+0 .140–1 .2714+4 0.781 .143–1 .145–1 .4068+4 0.791 .147–1 .139–1 .3605+2 1.997 .174+0 .554–5
200 .2379+2 1.989 –.375+0 –.825–4 .9257+2 1.991 .320+0 –.306–4 .2044+3 1.271 –.108+0 .658–2 .4147+3 1.281 –.110+0 .663–2 .1456+3 1.995 .211+0 –.111–4 .2266+3 1.435 .469–1 .102–2 .4637+3 1.433 .432–1 .626–3 .8612+3 1.068 .494–1 .223–1 .1279+4 1.073 .502–1 .221–1 .1525+2 1.996 .183+0 –.265–5
500 .2198+2 1.986 –.777–1 –.856–4 .6576+2 1.995 .311–1 –.392–4 .1137+3 1.423 .734–1 .176–1 .2273+3 1.442 .734–1 .181–1 .5669+2 1.996 .329–1 –.166–4 .7932+2 1.611 –.333–2 .211–2 .1575+3 1.621 –.301–2 .266–2 .9315+2 1.217 .208+0 .403–1 .1371+3 1.212 .208+0 .405–1 .3982+1 1.996 .399–1 –.847–5
1000 .1929+2 1.981 .223+0 –.852–4 .4072+2 1.998 –.545–1 –.408–4 .5150+2 1.438 .324+0 .277–1 .1014+3 1.462 .329+0 .281–1 .2117+2 1.998 –.608–1 –.184–4 .2309+2 1.574 .177+0 .864–2 .4495+2 1.592 .182+0 .926–2 .1136+2 1.092 .431+0 .686–1 .1661+2 1.082 .430+0 .693–1 .1240+1 1.998 –.608–1 –.135–4
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E (eV) 1500 .1701+2 1.976 .436+0 –.840–4 .2730+2 1.999 –.131–2 –.397–4 .2724+2 1.396 .512+0 .371–1 .5302+2 1.422 .521+0 .371–1 .1077+2 1.999 –.292–1 –.195–4 .9547+1 1.493 .363+0 .166–1 .1838+2 1.515 .371+0 .169–1 .2898+1 0.947 .571+0 .975–1 .4221+1 0.937 .569+0 .988–1 .5871+0 1.999 –.340–1 –.164–4
2000 .1507+2 1.972 .604+0 –.821–4 .1934+2 1.999 .926–1 –.380–4 .1598+2 1.343 .657+0 .468–1 .3084+2 1.371 .670+0 .463–1 .6404+1 1.999 .503–1 –.201–4 .4789+1 1.415 .517+0 .259–1 .9149+1 1.439 .527+0 .258–1 .1043+1 0.832 .665+0 .127+0 .1515+1 0.825 .662+0 .128+0 .3363+0 1.999 .423–1 –.179–4
3000 .1199+2 1.962 .877+0 –.788–4 .1090+2 1.995 .309+0 –.349–4 .6728+1 1.232 .872+0 .668–1 .1283+2 1.260 .889+0 .655–1 .2924+1 1.996 .251+0 –.207–4 .1673+1 1.274 .749+0 .464–1 .3159+1 1.299 .764+0 .455–1 .2308+0 0.670 .786+0 .183+0 .3335+0 0.670 .785+0 .185+0 .1472+0 1.997 .242+0 –.187–4
4000 .9705+1 1.952 .110+1 –.753–4 .6815+1 1.989 .522+0 –.322–4 .3374+1 1.128 .102+1 .869–1 .6375+1 1.157 .104+1 .849–1 .1619+1 1.991 .457+0 –.206–4 .7526+0 1.155 .916+0 .675–1 .1410+1 1.180 .933+0 .659–1 .7543–1 0.558 .864+0 .234+0 .1086+0 0.565 .865+0 .236+0 .7973–1 1.992 .449+0 –.187–4
5000 .7968+1 1.942 .129+1 –.710–4 .4574+1 1.982 .721+0 –.292–4 .1896+1 1.037 .114+1 .108+0 .3556+1 1.065 .116+1 .105+0 .1003+1 1.985 .654+0 –.196–4 .3937+0 1.054 .104+1 .892–1 .7326+0 1.079 .106+1 .870–1 .3082–1 0.471 .915+0 .281+0 .4422–1 0.484 .920+0 .282+0 .4875–1 1.985 .645+0 –.185–4
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Zn, Z = 30 Shell 1s1/2 Eb = 9663 eV 2s1/2 Eb = 1198 eV 2 p1/2 Eb = 1048 eV 2 p3/2 Eb = 1025 eV 3s1/2 Eb = 141 eV 3 p1/2 Eb = 94 eV 3 p3/2 Eb = 91 eV 3d3/2 Eb = 12 eV 3d5/2 Eb = 11 eV 4s1/2 Eb = 9 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2260+2 1.989 –.562+0 –.890–4 .9777+2 1.988 .568+0 –.232–4 .2348+3 1.083 –.142+0 .235–2 .4801+3 1.087 –.144+0 .171–2 .2213+3 1.995 .284+0 –.102–5 .3167+3 1.048 .152+0 .191–1 .6707+3 1.041 .145+0 .174–1 .3023+4 0.751 .102–1 .135–1 .4541+4 0.762 .107–1 .129–1 .4951+2 1.997 .179+0 .501–5
200 .2210+2 1.988 –.406+0 –.950–4 .8710+2 1.990 .349+0 –.340–4 .1918+3 1.258 –.120+0 .586–2 .3897+3 1.269 –.123+0 .594–2 .1447+3 1.995 .226+0 –.118–4 .2253+3 1.415 .618–1 .210–2 .4641+3 1.413 .572–1 .159–2 .1010+4 1.046 .424–1 .215–1 .1504+4 1.053 .433–1 .212–1 .2034+2 1.996 .187+0 –.193–5
500 .2053+2 1.985 –.105+0 –.982–4 .6320+2 1.994 .486–1 –.443–4 .1108+3 1.415 .553–1 .171–1 .2219+3 1.436 .550–1 .177–1 .5837+2 1.995 .474–1 –.189–4 .8320+2 1.607 –.106–1 .166–2 .1658+3 1.617 –.106–1 .222–2 .1175+3 1.217 .193+0 .393–1 .1733+3 1.212 .194+0 .394–1 .5421+1 1.996 .528–1 –.110–4
1000 .1817+2 1.980 .199+0 –.976–4 .4015+2 1.998 –.565–1 –.468–4 .5241+2 1.439 .306+0 .275–1 .1032+3 1.465 .311+0 .279–1 .2238+2 1.998 –.601–1 –.215–4 .2532+2 1.581 .156+0 .779–2 .4937+2 1.600 .160+0 .850–2 .1502+2 1.111 .418+0 .664–1 .2199+2 1.100 .417+0 .672–1 .1707+1 1.997 –.584–1 –.172–4
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E (eV) 1500 .1615+2 1.976 .412+0 –.960–4 .2741+2 1.999 –.165–1 –.458–4 .2850+2 1.404 .495+0 .365–1 .5550+2 1.432 .505+0 .365–1 .1155+2 1.999 –.418–1 –.228–4 .1072+2 1.509 .338+0 .152–1 .2065+2 1.531 .346+0 .155–1 .3918+1 0.975 .566+0 .946–1 .5712+1 0.965 .564+0 .958–1 .8158+0 1.999 –.471–1 –.193–4
2000 .1441+2 1.971 .583+0 –.943–4 .1969+2 1.999 .687–1 –.444–4 .1705+2 1.355 .644+0 .456–1 .3291+2 1.384 .657+0 .452–1 .6928+1 1.999 .277–1 –.237–4 .5459+1 1.434 .494+0 .238–1 .1043+2 1.459 .505+0 .238–1 .1429+1 0.862 .666+0 .123+0 .2077+1 0.854 .663+0 .124+0 .4690+0 1.999 .201–1 –.205–4
3000 .1162+2 1.961 .858+0 –.905–4 .1131+2 1.995 .275+0 –.412–4 .7375+1 1.250 .866+0 .649–1 .1405+2 1.281 .883+0 .636–1 .3197+1 1.997 .217+0 –.246–4 .1942+1 1.298 .734+0 .434–1 .3664+1 1.325 .749+0 .425–1 .3216+0 0.696 .794+0 .177+0 .4651+0 0.694 .792+0 .179+0 .2069+0 1.997 .207+0 –.225–4
4000 .9510+1 1.951 .108+1 –.868–4 .7171+1 1.990 .483+0 –.384–4 .3765+1 1.151 .102+1 .843–1 .7103+1 1.182 .104+1 .822–1 .1783+1 1.992 .417+0 –.246–4 .8840+0 1.182 .907+0 .637–1 .1653+1 1.209 .924+0 .620–1 .1064+0 0.584 .876+0 .227+0 .1533+0 0.589 .876+0 .229+0 .1126+0 1.993 .408+0 –.228–4
5000 .7884+1 1.942 .127+1 –.822–4 .4861+1 1.983 .680+0 –.352–4 .2143+1 1.062 .114+1 .104+0 .4012+1 1.093 .116+1 .102+0 .1111+1 1.986 .611+0 –.238–4 .4666+0 1.083 .104+1 .846–1 .8665+0 1.110 .106+1 .823–1 .4390–1 0.495 .930+0 .273+0 .6301–1 0.507 .935+0 .275+0 .6912–1 1.987 .601+0 –.224–4
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Ga, Z = 31 Shell 1s1/2 Eb = 10371 eV 2s1/2 Eb = 1302 eV 2 p1/2 Eb = 1146 eV 2 p3/2 Eb = 1119 eV 3s1/2 Eb = 162 eV 3 p1/2 Eb = 111 eV 3 p3/2 Eb = 107 eV 3d3/2 Eb = 21 eV 3d5/2 Eb = 20 eV 4s1/2 Eb = 11 eV 4 p1/2 Eb = 6 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2101+2 1.988 –.591+0 –.103–3 .9100+2 1.987 .593+0 –.257–4 .2160+3 1.076 –.151+0 .188–2 .4424+3 1.079 –.153+0 .126–2 .2103+3 1.995 .301+0 –.305–6 .3053+3 1.035 .159+0 .226–1 .6511+3 1.028 .151+0 .206–1 .3081+4 0.727 .655–2 .132–1 .4633+4 0.740 .702–2 .125–1 .6789+2 1.996 .183+0 .468–5 .2193+2 0.747 .128+0 .110–1
200 .2055+2 1.987 –.436+0 –.110–3 .8164+2 1.989 .376+0 –.379–4 .1789+3 1.247 –.132+0 .522–2 .3642+3 1.258 –.135+0 .535–2 .1411+3 1.994 .243+0 –.127–4 .2212+3 1.397 .752–1 .338–2 .4583+3 1.394 .696–1 .276–2 .1107+4 1.027 .373–1 .213–1 .1648+4 1.035 .383–1 .210–1 .2813+2 1.996 .191+0 –.883–6 .1332+2 1.404 .102+0 –.776–3
500 .1919+2 1.984 –.131+0 –.113–3 .6044+2 1.993 .659–1 –.501–4 .1072+3 1.408 .387–1 .166–1 .2149+3 1.430 .380–1 .174–1 .5928+2 1.995 .614–1 –.217–4 .8604+2 1.603 –.154–1 .133–2 .1720+3 1.613 –.158–1 .190–2 .1411+3 1.216 .182+0 .386–1 .2082+3 1.211 .183+0 .387–1 .7544+1 1.995 .643–1 –.109–4 .4216+1 1.647 –.208–1 .377–4
1000 .1712+2 1.979 .176+0 –.112–3 .3936+2 1.997 –.566–1 –.536–4 .5280+2 1.439 .289+0 .271–1 .1041+3 1.466 .294+0 .277–1 .2342+2 1.997 –.579–1 –.251–4 .2742+2 1.587 .136+0 .701–2 .5354+2 1.607 .140+0 .783–2 .1909+2 1.128 .407+0 .648–1 .2797+2 1.116 .406+0 .656–1 .2402+1 1.997 –.548–1 –.189–4 .1180+1 1.615 .115+0 .518–2
127
E (eV) 1500 .1532+2 1.974 .391+0 –.110–3 .2735+2 1.999 –.292–1 –.529–4 .2951+2 1.409 .480+0 .359–1 .5749+2 1.439 .489+0 .360–1 .1228+2 1.999 –.520–1 –.267–4 .1191+2 1.521 .315+0 .139–1 .2295+2 1.545 .323+0 .144–1 .5115+1 1.000 .561+0 .918–1 .7461+1 0.988 .559+0 .931–1 .1156+1 1.998 –.550–1 –.225–4 .4838+0 1.540 .294+0 .117–1
2000 .1377+2 1.970 .563+0 –.108–3 .1991+2 1.999 .473–1 –.516–4 .1801+2 1.365 .631+0 .447–1 .3475+2 1.396 .644+0 .442–1 .7439+1 1.999 .791–2 –.279–4 .6158+1 1.451 .472+0 .220–1 .1176+2 1.477 .483+0 .220–1 .1896+1 0.889 .667+0 .119+0 .2756+1 0.880 .664+0 .121+0 .6689+0 1.999 .129–2 –.245–4 .2421+0 1.465 .455+0 .198–1
3000 .1124+2 1.960 .841+0 –.104–3 .1167+2 1.996 .244+0 –.484–4 .8000+1 1.266 .858+0 .632–1 .1523+2 1.298 .877+0 .618–1 .3475+1 1.997 .185+0 –.290–4 .2233+1 1.319 .718+0 .406–1 .4211+1 1.348 .734+0 .398–1 .4350+0 0.722 .802+0 .171+0 .6290+0 0.718 .799+0 .174+0 .2972+0 1.997 .175+0 –.265–4 .8459–1 1.329 .704+0 .381–1
4000 .9293+1 1.950 .106+1 –.996–4 .7494+1 1.991 .446+0 –.453–4 .4158+1 1.172 .102+1 .821–1 .7834+1 1.205 .104+1 .799–1 .1953+1 1.993 .379+0 –.292–4 .1030+1 1.207 .897+0 .604–1 .1923+1 1.236 .916+0 .587–1 .1458+0 0.606 .887+0 .221+0 .2099+0 0.610 .887+0 .223+0 .1626+0 1.993 .369+0 –.270–4 .3821–1 1.212 .885+0 .576–1
5000 .7775+1 1.941 .126+1 –.950–4 .5131+1 1.984 .640+0 –.421–4 .2398+1 1.086 .114+1 .101+0 .4481+1 1.118 .117+1 .982–1 .1224+1 1.987 .569+0 –.286–4 .5484+0 1.110 .103+1 .803–1 .1017+1 1.139 .105+1 .780–1 .6073–1 0.518 .946+0 .266+0 .8715–1 0.529 .949+0 .268+0 .1002+0 1.988 .558+0 –.269–4 .2009–1 1.114 .102+1 .777–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Ge, Z = 32 Shell 1s1/2 Eb = 11107 eV 2s1/2 Eb = 1413 eV 2 p1/2 Eb = 1251 eV 2 p3/2 Eb = 1220 eV 3s1/2 Eb = 184 eV 3 p1/2 Eb = 130 eV 3 p3/2 Eb = 125 eV 3d3/2 Eb = 33 eV 3d5/2 Eb = 32 eV 4s1/2 Eb = 14 eV 4 p1/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1958+2 1.987 –.622+0 –.118–3 .8475+2 1.986 .619+0 –.282–4 .1987+3 1.068 –.160+0 .128–2 .4076+3 1.071 –.163+0 .663–3 .2007+3 1.994 .320+0 .696–6 .2942+3 1.020 .166+0 .266–1 .6314+3 1.012 .157+0 .245–1 .3049+4 0.701 .258–2 .129–1 .4586+4 0.714 .308–2 .123–1 .8193+2 1.996 .186+0 .584–5 .3320+2 0.732 .122+0 .128–1
200 .1916+2 1.986 –.464+0 –.126–3 .7650+2 1.988 .402+0 –.423–4 .1668+3 1.237 –.143+0 .455–2 .3399+3 1.249 –.147+0 .473–2 .1378+3 1.994 .259+0 –.135–4 .2169+3 1.382 .893–1 .486–2 .4521+3 1.379 .826–1 .411–2 .1181+4 1.009 .316–1 .211–1 .1760+4 1.018 .327–1 .207–1 .3463+2 1.995 .198+0 –.131–5 .2011+2 1.390 .113+0 –.360–5
500 .1796+2 1.983 –.157+0 –.129–3 .5770+2 1.992 .841–1 –.565–4 .1032+3 1.401 .222–1 .161–1 .2072+3 1.423 .210–1 .170–1 .6015+2 1.994 .758–1 –.247–4 .8858+2 1.598 –.185–1 .107–2 .1777+3 1.608 –.193–1 .165–2 .1649+3 1.214 .172+0 .382–1 .2434+3 1.210 .173+0 .383–1 .9375+1 1.995 .765–1 –.122–4 .6470+1 1.648 –.215–1 –.280–3
1000 .1614+2 1.978 .153+0 –.128–3 .3845+2 1.997 –.548–1 –.613–4 .5286+2 1.438 .273+0 .268–1 .1043+3 1.467 .277+0 .275–1 .2445+2 1.997 –.541–1 –.291–4 .2949+2 1.593 .117+0 .631–2 .5769+2 1.613 .121+0 .722–2 .2363+2 1.143 .396+0 .634–1 .3462+2 1.131 .395+0 .642–1 .3010+1 1.997 –.502–1 –.218–4 .1859+1 1.624 .955–1 .438–2
128
E (eV) 1500 .1454+2 1.973 .371+0 –.126–3 .2717+2 1.999 –.400–1 –.612–4 .3034+2 1.414 .464+0 .352–1 .5912+2 1.446 .474+0 .354–1 .1301+2 1.998 –.603–1 –.313–4 .1313+2 1.532 .293+0 .126–1 .2532+2 1.557 .300+0 .133–1 .6507+1 1.022 .555+0 .890–1 .9491+1 1.010 .553+0 .904–1 .1458+1 1.998 –.621–1 –.262–4 .7757+0 1.554 .270+0 .104–1
2000 .1315+2 1.969 .543+0 –.124–3 .2005+2 1.999 .279–1 –.597–4 .1887+2 1.373 .617+0 .438–1 .3642+2 1.407 .631+0 .434–1 .7963+1 1.999 –.978–2 –.326–4 .6899+1 1.466 .450+0 .202–1 .1318+2 1.493 .461+0 .204–1 .2452+1 0.915 .667+0 .116+0 .3563+1 0.904 .664+0 .117+0 .8478+0 1.999 –.158–1 –.286–4 .3929+0 1.482 .429+0 .178–1
3000 .1085+2 1.959 .824+0 –.119–3 .1197+2 1.996 .214+0 –.566–4 .8607+1 1.280 .850+0 .616–1 .1637+2 1.315 .870+0 .601–1 .3766+1 1.997 .155+0 –.341–4 .2552+1 1.340 .700+0 .379–1 .4808+1 1.369 .717+0 .371–1 .5737+0 0.748 .810+0 .167+0 .8293+0 0.743 .807+0 .169+0 .3795+0 1.998 .145+0 –.309–4 .1395+0 1.350 .685+0 .352–1
4000 .9063+1 1.949 .105+1 –.115–3 .7790+1 1.992 .411+0 –.534–4 .4553+1 1.190 .102+1 .796–1 .8569+1 1.225 .104+1 .773–1 .2132+1 1.994 .343+0 –.345–4 .1191+1 1.230 .884+0 .567–1 .2222+1 1.260 .905+0 .551–1 .1947+0 0.631 .900+0 .215+0 .2802+0 0.633 .898+0 .217+0 .2086+0 1.994 .332+0 –.319–4 .6364–1 1.239 .872+0 .541–1
5000 .7648+1 1.940 .124+1 –.110–3 .5387+1 1.985 .601+0 –.502–4 .2661+1 1.107 .115+1 .978–1 .4963+1 1.142 .117+1 .947–1 .1344+1 1.988 .528+0 –.342–4 .6401+0 1.135 .103+1 .758–1 .1185+1 1.166 .105+1 .734–1 .8191–1 0.543 .962+0 .260+0 .1175+0 0.552 .964+0 .262+0 .1291+0 1.989 .517+0 –.317–4 .3372–1 1.141 .102+1 .737–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables As, Z = 33 Shell 1s1/2 Eb = 11871 eV 2s1/2 Eb = 1531 eV 2 p1/2 Eb = 1362 eV 2 p3/2 Eb = 1327 eV 3s1/2 Eb = 208 eV 3 p1/2 Eb = 151 eV 3 p3/2 Eb = 145 eV 3d3/2 Eb = 46 eV 3d5/2 Eb = 45 eV 4s1/2 Eb = 17 eV 4 p1/2 Eb = 9 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1829+2 1.986 –.653+0 –.136–3 .7896+2 1.985 .645+0 –.309–4 .1830+3 1.059 –.170+0 .564–3 .3757+3 1.062 –.173+0 –.454–4 .1914+3 1.993 .340+0 .200–5 .2830+3 1.006 .173+0 .311–1 .6108+3 0.997 .163+0 .287–1 .2983+4 0.673 –.159–2 .126–1 .4488+4 0.688 –.109–2 .118–1 .9519+2 1.995 .190+0 .747–5 .4445+2 0.708 .111+0 .149–1
200 .1790+2 1.985 –.492+0 –.144–3 .7169+2 1.987 .427+0 –.470–4 .1555+3 1.228 –.155+0 .382–2 .3172+3 1.240 –.159+0 .407–2 .1343+3 1.993 .275+0 –.143–4 .2123+3 1.368 .104+0 .658–2 .4448+3 1.364 .961–1 .568–2 .1241+4 0.990 .253–1 .207–1 .1851+4 1.000 .266–1 .203–1 .4087+2 1.995 .204+0 –.150–5 .2670+2 1.373 .124+0 .894–3
500 .1683+2 1.982 –.183+0 –.147–3 .5499+2 1.992 .103+0 –.637–4 .9911+2 1.394 .575–2 .156–1 .1992+3 1.417 .394–2 .166–1 .6084+2 1.994 .906–1 –.280–4 .9072+2 1.593 –.201–1 .901–3 .1827+3 1.603 –.214–1 .147–2 .1889+3 1.212 .162+0 .379–1 .2789+3 1.208 .164+0 .379–1 .1117+2 1.995 .885–1 –.140–4 .8697+1 1.648 –.202–1 –.528–3
1000 .1522+2 1.977 .129+0 –.147–3 .3745+2 1.996 –.516–1 –.701–4 .5265+2 1.437 .256+0 .265–1 .1040+3 1.467 .260+0 .272–1 .2542+2 1.996 –.492–1 –.337–4 .3150+2 1.597 .100+0 .565–2 .6174+2 1.618 .104+0 .667–2 .2861+2 1.156 .384+0 .619–1 .4192+2 1.144 .384+0 .627–1 .3620+1 1.996 –.445–1 –.249–4 .2562+1 1.632 .779–1 .370–2
129
E (eV) 1500 .1380+2 1.972 .349+0 –.144–3 .2690+2 1.998 –.489–1 –.702–4 .3099+2 1.417 .448+0 .348–1 .6042+2 1.451 .458+0 .350–1 .1373+2 1.998 –.664–1 –.362–4 .1436+2 1.542 .270+0 .116–1 .2774+2 1.568 .278+0 .123–1 .8102+1 1.044 .548+0 .867–1 .1181+2 1.030 .546+0 .882–1 .1763+1 1.998 –.670–1 –.304–4 .1086+1 1.566 .246+0 .920–2
2000 .1255+2 1.967 .523+0 –.141–3 .2010+2 1.999 .103–1 –.689–4 .1964+2 1.381 .604+0 .431–1 .3790+2 1.416 .618+0 .427–1 .8487+1 1.999 –.253–1 –.379–4 .7670+1 1.480 .427+0 .187–1 .1466+2 1.509 .439+0 .190–1 .3105+1 0.940 .665+0 .112+0 .4511+1 0.927 .662+0 .114+0 .1030+1 1.999 –.303–1 –.332–4 .5566+0 1.498 .404+0 .161–1
3000 .1047+2 1.958 .805+0 –.136–3 .1222+2 1.997 .185+0 –.658–4 .9194+1 1.294 .841+0 .602–1 .1748+2 1.331 .862+0 .587–1 .4063+1 1.998 .127+0 –.399–4 .2894+1 1.359 .682+0 .354–1 .5450+1 1.391 .699+0 .347–1 .7411+0 0.773 .816+0 .162+0 .1071+1 0.767 .813+0 .164+0 .4643+0 1.998 .117+0 –.361–4 .2007+0 1.371 .663+0 .325–1
4000 .8823+1 1.948 .103+1 –.131–3 .8058+1 1.992 .376+0 –.625–4 .4950+1 1.208 .101+1 .775–1 .9303+1 1.245 .104+1 .751–1 .2318+1 1.994 .308+0 –.406–4 .1368+1 1.253 .871+0 .534–1 .2548+1 1.285 .893+0 .518–1 .2547+0 0.655 .911+0 .209+0 .3663+0 0.656 .909+0 .212+0 .2565+0 1.995 .295+0 –.374–4 .9246–1 1.262 .857+0 .508–1
5000 .7507+1 1.938 .122+1 –.126–3 .5628+1 1.986 .562+0 –.592–4 .2930+1 1.128 .115+1 .951–1 .5456+1 1.165 .117+1 .919–1 .1470+1 1.989 .488+0 –.404–4 .7417+0 1.160 .102+1 .719–1 .1371+1 1.193 .104+1 .695–1 .1082+0 0.566 .977+0 .253+0 .1550+0 0.573 .978+0 .256+0 .1593+0 1.990 .477+0 –.377–4 .4935–1 1.166 .101+1 .695–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables As, Z = 33 (continued) Shell 4 p3/2 Eb = 9 eV
σ β γ δ
100 .9447+2 0.720 .108+0 .146–1
200 .5464+2 1.366 .117+0 .108–2
500 .1707+2 1.652 –.217–1 .492–4
1000 .4904+1 1.650 .815–1 .472–2
E (eV) 1500 .2051+1 1.590 .253+0 .100–1
2000 .1041+1 1.525 .416+0 .165–1
3000 .3703+0 1.402 .681+0 .319–1
4000 .1689+0 1.294 .879+0 .493–1
5000 .8944–1 1.199 .103+1 .672–1
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1711+2 1.985 –.684+0 –.155–3 .7359+2 1.984 .672+0 –.338–4 .1687+3 1.051 –.181+0 –.253–3 .3484+3 1.054 –.183+0 –.857–3 .1822+3 1.993 .361+0 .367–5 .2724+3 0.991 .179+0 .359–1 .5911+3 0.981 .168+0 .332–1 .2876+4 0.644 –.586–2 .121–1 .4327+4 0.660 –.537–2 .114–1
200 .1675+2 1.984 –.521+0 –.163–3 .6721+2 1.986 .453+0 –.522–4 .1450+3 1.220 –.168+0 .300–2 .2976+3 1.232 –.171+0 .331–2 .1307+3 1.992 .293+0 –.150–4 .2076+3 1.354 .119+0 .856–2 .4375+3 1.350 .110+0 .749–2 .1284+4 0.970 .189–1 .203–1 .1915+4 0.982 .202–1 .199–1
500 .1580+2 1.981 –.210+0 –.168–3 .5235+2 1.991 .123+0 –.718–4 .9500+2 1.387 –.107–1 .151–1 .1919+3 1.411 –.131–1 .162–1 .6134+2 1.993 .106+0 –.316–4 .9259+2 1.588 –.201–1 .807–3 .1872+3 1.597 –.220–1 .136–2 .2125+3 1.208 .153+0 .377–1 .3138+3 1.206 .155+0 .377–1
1000 .1438+2 1.976 .105+0 –.167–3 .3639+2 1.995 –.465–1 –.795–4 .5221+2 1.435 .239+0 .262–1 .1035+3 1.467 .242+0 .270–1 .2633+2 1.995 –.428–1 –.387–4 .3345+2 1.601 .840–1 .507–2 .6569+2 1.622 .871–1 .619–2 .3399+2 1.168 .374+0 .610–1 .4979+2 1.155 .374+0 .618–1
E (eV) 1500 .1311+2 1.971 .326+0 –.164–3 .2654+2 1.998 –.559–1 –.803–4 .3149+2 1.420 .432+0 .344–1 .6157+2 1.456 .441+0 .346–1 .1443+2 1.997 –.706–1 –.419–4 .1561+2 1.551 .249+0 .106–1 .3018+2 1.578 .256+0 .115–1 .9893+1 1.063 .540+0 .847–1 .1442+2 1.049 .538+0 .862–1
2000 .1198+2 1.966 .502+0 –.161–3 .2007+2 1.998 –.554–2 –.792–4 .2031+2 1.388 .590+0 .425–1 .3930+2 1.425 .603+0 .421–1 .9007+1 1.998 –.389–1 –.438–4 .8469+1 1.493 .405+0 .173–1 .1619+2 1.523 .416+0 .177–1 .3857+1 0.963 .662+0 .109+0 .5602+1 0.949 .659+0 .111+0
3000 .1009+2 1.957 .786+0 –.155–3 .1242+2 1.997 .158+0 –.762–4 .9755+1 1.306 .832+0 .589–1 .1856+2 1.345 .852+0 .573–1 .4366+1 1.998 .100+0 –.464–4 .3259+1 1.377 .662+0 .330–1 .6136+1 1.411 .680+0 .325–1 .9398+0 0.798 .822+0 .157+0 .1357+1 0.790 .818+0 .160+0
4000 .8578+1 1.947 .101+1 –.150–3 .8298+1 1.993 .343+0 –.728–4 .5344+1 1.224 .101+1 .756–1 .1005+2 1.264 .103+1 .731–1 .2511+1 1.995 .273+0 –.474–4 .1560+1 1.274 .857+0 .503–1 .2903+1 1.309 .880+0 .488–1 .3270+0 0.679 .922+0 .204+0 .4700+0 0.678 .920+0 .207+0
5000 .7355+1 1.937 .120+1 –.144–3 .5852+1 1.987 .525+0 –.692–4 .3204+1 1.148 .115+1 .931–1 .5963+1 1.188 .118+1 .896–1 .1600+1 1.990 .449+0 –.473–4 .8533+0 1.185 .101+1 .686–1 .1574+1 1.220 .103+1 .662–1 .1402+0 0.587 .991+0 .247+0 .2006+0 0.592 .991+0 .250+0
Se, Z = 34 Shell 1s1/2 Eb = 12662 eV 2s1/2 Eb = 1656 eV 2 p1/2 Eb = 1479 eV 2 p3/2 Eb = 1432 eV 3s1/2 Eb = 234 eV 3 p1/2 Eb = 173 eV 3 p3/2 Eb = 166 eV 3d3/2 Eb = 61 eV 3d5/2 Eb = 60 eV
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M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Se, Z = 34 (continued) Shell 4s1/2 Eb = 20 eV 4 p1/2 Eb = 10 eV 4 p3/2 Eb = 10 eV
σ β γ δ σ β γ δ σ β γ δ
100 .1076+3 1.995 .193+0 .948–5 .5522+2 0.678 .978–1 .170–1 .1183+3 0.693 .956–1 .167–1
200 .4702+2 1.995 .210+0 –.134–5 .3308+2 1.357 .135+0 .190–2 .6816+2 1.347 .127+0 .204–2
500 .1297+2 1.994 .100+0 –.162–4 .1089+2 1.646 –.171–1 –.718–3 .2147+2 1.650 –.192–1 –.163–3
1000 .4244+1 1.995 –.375–1 –.280–4 .3285+1 1.640 .615–1 .307–2 .6306+1 1.658 .648–1 .417–2
E (eV) 1500 .2076+1 1.997 –.698–1 –.348–4 .1413+1 1.578 .223+0 .808–2 .2674+1 1.603 .230+0 .906–2
2000 .1218+1 1.998 –.427–1 –.385–4 .7325+0 1.513 .379+0 .145–1 .1372+1 1.542 .391+0 .151–1
3000 .5530+0 1.998 .904–1 –.420–4 .2682+0 1.390 .640+0 .298–1 .4952+0 1.422 .659+0 .294–1
4000 .3069+0 1.995 .261+0 –.437–4 .1248+0 1.283 .839+0 .471–1 .2280+0 1.317 .862+0 .457–1
5000 .1913+0 1.991 .437+0 –.443–4 .6708–1 1.190 .993+0 .651–1 .1215+0 1.225 .102+1 .628–1
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1602+2 1.983 –.716+0 –.177–3 .6865+2 1.983 .700+0 –.368–4 .1557+3 1.043 –.191+0 –.117–2 .3206+3 1.046 –.194+0 –.178–2 .1731+3 1.992 .384+0 .576–5 .2615+3 0.976 .184+0 .411–1 .5701+3 0.966 .173+0 .381–1
200 .1571+2 1.982 –.551+0 –.187–3 .6307+2 1.985 .480+0 –.580–4 .1354+3 1.210 –.181+0 .214–2 .2771+3 1.223 –.185+0 .252–2 .1268+3 1.992 .312+0 –.155–4 .2025+3 1.338 .134+0 .109–1 .4287+3 1.333 .124+0 .959–2
500 .1485+2 1.979 –.237+0 –.192–3 .4981+2 1.990 .143+0 –.807–4 .9091+2 1.379 –.273–1 .145–1 .1833+3 1.405 –.304–1 .158–1 .6163+2 1.992 .122+0 –.355–4 .9403+2 1.581 –.186–1 .798–3 .1908+3 1.591 –.213–1 .132–2
1000 .1359+2 1.975 .808–1 –.190–3 .3530+2 1.995 –.401–1 –.902–4 .5159+2 1.433 .222+0 .259–1 .1021+3 1.466 .225+0 .269–1 .2717+2 1.995 –.355–1 –.444–4 .3529+2 1.604 .689–1 .453–2 .6946+2 1.626 .718–1 .575–2
E (eV) 1500 .1245+2 1.970 .304+0 –.186–3 .2612+2 1.997 –.611–1 –.916–4 .3183+2 1.423 .416+0 .340–1 .6216+2 1.460 .426+0 .344–1 .1510+2 1.997 –.732–1 –.482–4 .1685+2 1.560 .228+0 .970–2 .3261+2 1.588 .235+0 .108–1
2000 .1144+2 1.965 .481+0 –.183–3 .1998+2 1.998 –.196–1 –.907–4 .2090+2 1.393 .575+0 .419–1 .4036+2 1.433 .590+0 .417–1 .9519+1 1.998 –.504–1 –.505–4 .9282+1 1.505 .382+0 .160–1 .1776+2 1.537 .394+0 .166–1
3000 .9722+1 1.955 .766+0 –.177–3 .1258+2 1.997 .132+0 –.879–4 .1029+2 1.318 .821+0 .577–1 .1954+2 1.359 .844+0 .562–1 .4672+1 1.998 .754–1 –.537–4 .3645+1 1.394 .642+0 .309–1 .6858+1 1.429 .661+0 .304–1
4000 .8330+1 1.946 .994+0 –.171–3 .8511+1 1.993 .310+0 –.845–4 .5732+1 1.239 .100+1 .739–1 .1075+2 1.281 .103+1 .713–1 .2708+1 1.995 .240+0 –.551–4 .1766+1 1.295 .841+0 .474–1 .3283+1 1.331 .865+0 .460–1
5000 .7193+1 1.936 .119+1 –.164–3 .6060+1 1.988 .488+0 –.806–4 .3480+1 1.166 .114+1 .908–1 .6463+1 1.208 .118+1 .873–1 .1735+1 1.991 .411+0 –.552–4 .9747+0 1.207 .998+0 .650–1 .1796+1 1.244 .103+1 .627–1
Br, Z = 35 Shell 1s1/2 Eb = 13481 eV 2s1/2 Eb = 1787 eV 2 p1/2 Eb = 1602 eV 2 p3/2 Eb = 1556 eV 3s1/2 Eb = 262 eV 3 p1/2 Eb = 197 eV 3 p3/2 Eb = 189 eV
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M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Br, Z = 35 (continued) Shell 3d3/2 Eb = 77 eV 3d5/2 Eb = 76 eV 4s1/2 Eb = 24 eV 4 p1/2 Eb = 12 eV 4 p3/2 Eb = 12 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2758+4 0.616 –.101–1 .116–1 .4150+4 0.633 –.966–2 .108–1 .1180+3 1.994 .198+0 .121–4 .6479+2 0.645 .838–1 .192–1 .1399+3 0.662 .826–1 .187–1
200 .1314+4 0.949 .123–1 .199–1 .1962+4 0.962 .137–1 .194–1 .5288+2 1.994 .218+0 –.857–6 .3917+2 1.338 .145+0 .306–2 .8120+2 1.330 .137+0 .317–2
500 .2357+3 1.204 .143+0 .374–1 .3481+3 1.202 .146+0 .373–1 .1477+2 1.994 .112+0 –.187–4 .1307+2 1.644 –.124–1 –.860–3 .2586+2 1.646 –.153–1 –.334–3
1000 .3974+2 1.178 .363+0 .600–1 .5821+2 1.166 .364+0 .607–1 .4879+1 1.995 –.298–1 –.318–4 .4033+1 1.646 .465–1 .250–2 .7756+1 1.665 .495–1 .368–2
E (eV) 1500 .1188+2 1.081 .531+0 .829–1 .1732+2 1.066 .530+0 .843–1 .2401+1 1.997 –.713–1 –.396–4 .1761+1 1.589 .200+0 .709–2 .3336+1 1.615 .208+0 .822–2
2000 .4715+1 0.984 .658+0 .107+0 .6844+1 0.970 .655+0 .109+0 .1414+1 1.998 –.533–1 –.440–4 .9226+0 1.527 .355+0 .130–1 .1729+1 1.557 .366+0 .137–1
3000 .1173+1 0.822 .827+0 .153+0 .1692+1 0.813 .823+0 .156+0 .6457+0 1.998 .660–1 –.486–4 .3428+0 1.408 .618+0 .274–1 .6328+0 1.442 .636+0 .272–1
4000 .4133+0 0.703 .933+0 .198+0 .5933+0 0.699 .929+0 .202+0 .3600+0 1.996 .228+0 –.507–4 .1611+0 1.304 .821+0 .439–1 .2941+0 1.340 .845+0 .427–1
5000 .1787+0 0.609 .100+1 .241+0 .2556+0 0.612 .100+1 .244+0 .2252+0 1.992 .398+0 –.516–4 .8720–1 1.214 .980+0 .613–1 .1578+0 1.250 .101+1 .590–1
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1503+2 1.982 –.748+0 –.201–3 .6401+2 1.982 .728+0 –.400–4 .1439+3 1.035 –.202+0 –.217–2 .2968+3 1.037 –.205+0 –.279–2 .1643+3 1.991 .407+0 .833–5
200 .1475+2 1.981 –.580+0 –.211–3 .5915+2 1.984 .507+0 –.642–4 .1264+3 1.202 –.194+0 .115–2 .2592+3 1.215 –.199+0 .161–2 .1228+3 1.991 .331+0 –.159–4
500 .1398+2 1.978 –.265+0 –.218–3 .4734+2 1.988 .165+0 –.906–4 .8691+2 1.372 –.439–1 .139–1 .1756+3 1.398 –.477–1 .153–1 .6173+2 1.991 .139+0 –.398–4
1000 .1285+2 1.973 .563–1 –.216–3 .3415+2 1.994 –.324–1 –.102–3 .5081+2 1.430 .204+0 .255–1 .1007+3 1.465 .207+0 .267–1 .2793+2 1.994 –.272–1 –.506–4
E (eV) 1500 .1184+2 1.968 .281+0 –.211–3 .2563+2 1.997 –.648–1 –.104–3 .3205+2 1.424 .400+0 .336–1 .6264+2 1.463 .410+0 .342–1 .1575+2 1.996 –.742–1 –.552–4
2000 .1093+2 1.964 .459+0 –.207–3 .1983+2 1.998 –.320–1 –.104–3 .2140+2 1.398 .561+0 .414–1 .4135+2 1.440 .576+0 .412–1 .1002+2 1.997 –.601–1 –.581–4
3000 .9361+1 1.954 .746+0 –.201–3 .1270+2 1.997 .108+0 –.101–3 .1079+2 1.328 .810+0 .567–1 .2049+2 1.371 .834+0 .552–1 .4978+1 1.998 .522–1 –.619–4
4000 .8082+1 1.944 .975+0 –.194–3 .8694+1 1.994 .279+0 –.975–4 .6113+1 1.253 .996+0 .723–1 .1146+2 1.298 .103+1 .696–1 .2908+1 1.996 .208+0 –.637–4
5000 .7026+1 1.935 .117+1 –.187–3 .6248+1 1.989 .453+0 –.936–4 .3758+1 1.182 .114+1 .886–1 .6969+1 1.227 .118+1 .850–1 .1874+1 1.992 .375+0 –.641–4
Kr, Z = 36 Shell 1s1/2 Eb = 14327 eV 2s1/2 Eb = 1927 eV 2 p1/2 Eb = 1731 eV 2 p3/2 Eb = 1678 eV 3s1/2 Eb = 292 eV
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M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Kr, Z = 36 (continued) Shell 3 p1/2 Eb = 222 eV 3 p3/2 Eb = 214 eV 3d3/2 Eb = 95 eV 3d5/2 Eb = 94 eV 4s1/2 Eb = 27 eV 4 p1/2 Eb = 15 eV 4 p3/2 Eb = 14 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2511+3 0.961 .189+0 .465–1 .5482+3 0.951 .177+0 .433–1 .2623+4 0.588 –.143–1 .109–1 .3948+4 0.607 –.139–1 .100–1 .1282+3 1.993 .200+0 .151–4 .7276+2 0.610 .688–1 .213–1 .1597+3 0.628 .684–1 .206–1
200 .1972+3 1.324 .150+0 .134–1 .4187+3 1.318 .139+0 .120–1 .1329+4 0.928 .565–2 .194–1 .1985+4 0.942 .709–2 .189–1 .5882+2 1.993 .224+0 –.177–6 .4487+2 1.320 .156+0 .440–2 .9401+2 1.309 .145+0 .442–2
500 .9518+2 1.575 –.157–1 .877–3 .1936+3 1.584 –.192–1 .137–2 .2578+3 1.199 .133+0 .371–1 .3807+3 1.198 .136+0 .370–1 .1662+2 1.993 .124+0 –.211–4 .1524+2 1.641 –.627–2 –.943–3 .3032+2 1.642 –.987–2 –.454–3
1000 .3705+2 1.606 .550–1 .403–2 .7303+2 1.629 .575–1 .536–2 .4580+2 1.188 .353+0 .591–1 .6708+2 1.175 .354+0 .598–1 .5533+1 1.994 –.213–1 –.362–4 .4806+1 1.652 .329–1 .197–2 .9264+1 1.671 .355–1 .323–2
E (eV) 1500 .1807+2 1.567 .207+0 .887–2 .3501+2 1.596 .215+0 .101–1 .1406+2 1.098 .523+0 .812–1 .2048+2 1.082 .522+0 .826–1 .2738+1 1.996 –.715–1 –.450–4 .2130+1 1.600 .179+0 .614–2 .4039+1 1.626 .186+0 .741–2
2000 .1011+2 1.516 .360+0 .148–1 .1934+2 1.549 .372+0 .156–1 .5676+1 1.005 .653+0 .104+0 .8234+1 0.989 .650+0 .106+0 .1618+1 1.997 –.620–1 –.500–4 .1127+1 1.541 .330+0 .115–1 .2113+1 1.571 .342+0 .124–1
3000 .4048+1 1.410 .621+0 .288–1 .7613+1 1.447 .641+0 .285–1 .1442+1 0.846 .830+0 .149+0 .2079+1 0.835 .825+0 .152+0 .7428+0 1.998 .435–1 –.559–4 .4247+0 1.426 .594+0 .252–1 .7837+0 1.462 .613+0 .251–1
4000 .1986+1 1.314 .824+0 .446–1 .3688+1 1.352 .850+0 .433–1 .5147+0 0.726 .942+0 .193+0 .7383+0 0.721 .938+0 .197+0 .4161+0 1.996 .196+0 –.585–4 .2016+0 1.325 .801+0 .409–1 .3676+0 1.362 .826+0 .397–1
5000 .1106+1 1.228 .986+0 .616–1 .2034+1 1.268 .102+1 .593–1 .2246+0 0.631 .102+1 .235+0 .3208+0 0.632 .102+1 .238+0 .2611+0 1.992 .361+0 –.595–4 .1099+0 1.236 .965+0 .576–1 .1986+0 1.275 .994+0 .554–1
σ β γ δ σ β γ δ σ β γ δ
100 .1410+2 1.981 –.769+0 –.228–3 .5978+2 1.981 .736+0 –.456–4 .1325+3 1.040 –.215+0 –.354–2
200 .1386+2 1.980 –.603+0 –.240–3 .5553+2 1.983 .522+0 –.718–4 .1175+3 1.199 –.205+0 .364–3
500 .1317+2 1.977 –.287+0 –.247–3 .4500+2 1.988 .181+0 –.101–3 .8259+2 1.367 –.573–1 .134–1
1000 .1216+2 1.972 .343–1 –.243–3 .3300+2 1.993 –.243–1 –.115–3 .4967+2 1.428 .188+0 .251–1
E (eV) 1500 .1125+2 1.967 .261+0 –.240–3 .2510+2 1.996 –.667–1 –.118–3 .3201+2 1.425 .385+0 .333–1
2000 .1043+2 1.962 .440+0 –.235–3 .1962+2 1.998 –.421–1 –.118–3 .2173+2 1.402 .547+0 .410–1
3000 .9004+1 1.953 .727+0 –.228–3 .1277+2 1.997 .860–1 –.116–3 .1122+2 1.337 .798+0 .556–1
4000 .7828+1 1.943 .954+0 –.220–3 .8848+1 1.994 .249+0 –.112–3 .6466+1 1.267 .988+0 .710–1
5000 .6849+1 1.933 .115+1 –.213–3 .6417+1 1.990 .419+0 –.108–3 .4026+1 1.197 .114+1 .862–1
Rb, Z = 37 Shell 1s1/2 Eb = 15203 eV 2s1/2 Eb = 2068 eV 2 p1/2 Eb = 1867 eV
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M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Rb, Z = 37 (continued) Shell 2 p3/2 Eb = 1808 eV 3s1/2 Eb = 325 eV 3 p1/2 Eb = 251 eV 3 p3/2 Eb = 242 eV 3d3/2 Eb = 116 eV 3d5/2 Eb = 114 eV 4s1/2 Eb = 32 eV 4 p1/2 Eb = 16 eV 4 p3/2 Eb = 15 eV 5s1/2 Eb = 4 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2735+3 1.043 –.219+0 –.409–2 .1548+3 1.990 .422+0 .884–5 .2405+3 0.980 .196+0 .486–1 .5266+3 0.969 .184+0 .452–1 .2454+4 0.588 –.182–1 .102–1 .3709+4 0.607 –.178–1 .937–2 .1408+3 1.992 .203+0 .163–4 .9290+2 0.661 .695–1 .209–1 .2066+3 0.677 .690–1 .202–1 .1321+2 1.992 .183+0 .225–4
200 .2410+3 1.213 –.212+0 .940–3 .1179+3 1.990 .344+0 –.170–4 .1905+3 1.318 .158+0 .152–1 .4058+3 1.313 .146+0 .136–1 .1298+4 0.917 .567–4 .190–1 .1944+4 0.933 .156–2 .184–1 .6644+2 1.993 .227+0 –.279–6 .5656+2 1.318 .156+0 .531–2 .1201+3 1.306 .145+0 .527–2 .4951+1 1.993 .225+0 .458–5
500 .1670+3 1.394 –.618–1 .150–1 .6130+2 1.991 .151+0 –.443–4 .9517+2 1.570 –.123–1 .105–2 .1943+3 1.579 –.166–1 .151–2 .2732+3 1.195 .124+0 .366–1 .4041+3 1.194 .127+0 .365–1 .1907+2 1.993 .132+0 –.233–4 .1914+2 1.640 –.553–3 –.902–3 .3851+2 1.641 –.493–2 –.434–3 .1219+1 1.993 .137+0 –.195–4
1000 .9854+2 1.464 .191+0 .264–1 .2850+2 1.993 –.190–1 –.573–4 .3842+2 1.607 .434–1 .360–2 .7590+2 1.631 .456–1 .502–2 .5146+2 1.196 .342+0 .582–1 .7540+2 1.184 .344+0 .588–1 .6413+1 1.994 –.133–1 –.407–4 .6132+1 1.658 .218–1 .150–2 .1194+2 1.676 .239–1 .281–2 .3853+0 1.994 –.107–1 –.392–4
134
E (eV) 1500 .6259+2 1.466 .395+0 .340–1 .1631+2 1.995 –.740–1 –.631–4 .1917+2 1.573 .189+0 .813–2 .3717+2 1.603 .197+0 .951–2 .1626+2 1.112 .515+0 .795–1 .2369+2 1.096 .514+0 .809–1 .3195+1 1.995 –.706–1 –.506–4 .2756+1 1.609 .159+0 .522–2 .5275+1 1.636 .166+0 .663–2 .1878+0 1.995 –.702–1 –.484–4
2000 .4199+2 1.446 .563+0 .410–1 .1047+2 1.997 –.676–1 –.664–4 .1089+2 1.526 .339+0 .138–1 .2084+2 1.560 .351+0 .147–1 .6689+1 1.023 .648+0 .102+0 .9703+1 1.006 .645+0 .104+0 .1896+1 1.997 –.683–1 –.568–4 .1472+1 1.553 .307+0 .104–1 .2785+1 1.584 .319+0 .115–1 .1101+0 1.997 –.689–1 –.560–4
3000 .2130+2 1.383 .823+0 .542–1 .5272+1 1.998 .317–1 –.710–4 .4450+1 1.425 .600+0 .269–1 .8367+1 1.463 .620+0 .268–1 .1741+1 0.869 .832+0 .146+0 .2509+1 0.856 .827+0 .149+0 .8755+0 1.998 .239–1 –.641–4 .5628+0 1.442 .569+0 .231–1 .1047+1 1.479 .589+0 .232–1 .5028–1 1.998 .209–1 –.625–4
4000 .1211+2 1.314 .102+1 .683–1 .3105+1 1.996 .179+0 –.733–4 .2212+1 1.333 .807+0 .422–1 .4105+1 1.373 .833+0 .409–1 .6301+0 0.749 .950+0 .189+0 .9032+0 0.742 .945+0 .193+0 .4928+0 1.996 .166+0 –.673–4 .2698+0 1.345 .780+0 .380–1 .4958+0 1.384 .805+0 .370–1 .2812–1 1.996 .164+0 –.664–4
5000 .7455+1 1.244 .117+1 .825–1 .2013+1 1.993 .340+0 –.743–4 .1244+1 1.248 .972+0 .581–1 .2284+1 1.289 .100+1 .559–1 .2777+0 0.654 .103+1 .230+0 .3962+0 0.653 .103+1 .233+0 .3104+0 1.993 .325+0 –.689–4 .1482+0 1.257 .948+0 .540–1 .2697+0 1.297 .978+0 .520–1 .1765–1 1.993 .322+0 –.685–4
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Sr, Z = 38 Shell 1s1/2 Eb = 16108 eV 2s1/2 Eb = 2219 eV 2 p1/2 Eb = 2010 eV 2 p3/2 Eb = 1943 eV 3s1/2 Eb = 361 eV 3 p1/2 Eb = 283 eV 3 p3/2 Eb = 273 eV 3d3/2 Eb = 139 eV 3d5/2 Eb = 137 eV 4s1/2 Eb = 40 eV 4 p1/2 Eb = 23 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1324+2 1.979 –.794+0 –.260–3 .5578+2 1.980 .750+0 –.515–4 .1222+3 1.041 –.229+0 –.491–2 .2526+3 1.044 –.233+0 –.540–2 .1456+3 1.989 .440+0 .976–5 .2293+3 0.988 .202+0 .509–1 .5032+3 0.976 .189+0 .474–1 .2290+4 0.586 –.225–1 .937–2 .3458+4 0.607 –.222–1 .853–2 .1510+3 1.992 .211+0 .182–4 .1086+3 0.689 .700–1 .222–1
200 .1304+2 1.978 –.627+0 –.272–3 .5208+2 1.982 .538+0 –.803–4 .1092+3 1.196 –.218+0 –.452–3 .2244+3 1.210 –.225+0 .249–3 .1128+3 1.989 .359+0 –.182–4 .1832+3 1.312 .167+0 .170–1 .3916+3 1.306 .153+0 .153–1 .1258+4 0.906 –.591–2 .185–1 .1884+4 0.923 –.434–2 .179–1 .7311+2 1.992 .233+0 –.372–6 .6581+2 1.314 .161+0 .620–2
500 .1242+2 1.975 –.309+0 –.278–3 .4272+2 1.987 .197+0 –.113–3 .7842+2 1.362 –.706–1 .129–1 .1588+3 1.390 –.758–1 .146–1 .6063+2 1.990 .164+0 –.491–4 .9470+2 1.565 –.829–2 .129–2 .1940+3 1.575 –.134–1 .172–2 .2865+3 1.190 .115+0 .362–1 .4237+3 1.190 .119+0 .360–1 .2149+2 1.992 .141+0 –.260–4 .2259+2 1.639 .589–2 –.849–3
1000 .1151+2 1.970 .128–1 –.275–3 .3182+2 1.992 –.157–1 –.129–3 .4843+2 1.425 .173+0 .248–1 .9620+2 1.463 .176+0 .263–1 .2896+2 1.992 –.104–1 –.647–4 .3962+2 1.608 .332–1 .324–2 .7844+2 1.632 .350–1 .475–2 .5713+2 1.203 .333+0 .576–1 .8369+2 1.190 .335+0 .581–1 .7312+1 1.993 –.508–2 –.458–4 .7387+1 1.662 .125–1 .113–2
135
E (eV) 1500 .1070+2 1.966 .239+0 –.270–3 .2450+2 1.995 –.670–1 –.133–3 .3185+2 1.425 .370+0 .330–1 .6234+2 1.468 .379+0 .338–1 .1682+2 1.995 –.723–1 –.715–4 .2020+2 1.579 .172+0 .748–2 .3923+2 1.610 .179+0 .901–2 .1858+2 1.126 .507+0 .783–1 .2706+2 1.109 .506+0 .797–1 .3670+1 1.995 –.682–1 –.569–4 .3372+1 1.618 .140+0 .447–2
2000 .9953+1 1.961 .420+0 –.266–3 .1935+2 1.997 –.506–1 –.134–3 .2196+2 1.405 .533+0 .405–1 .4248+2 1.451 .548+0 .406–1 .1091+2 1.996 –.735–1 –.756–4 .1165+2 1.534 .319+0 .127–1 .2232+2 1.570 .331+0 .139–1 .7788+1 1.041 .642+0 .997–1 .1129+2 1.023 .639+0 .102+0 .2189+1 1.996 –.736–1 –.642–4 .1821+1 1.564 .285+0 .919–2
3000 .8657+1 1.951 .709+0 –.258–3 .1280+2 1.997 .658–1 –.132–3 .1161+2 1.344 .787+0 .548–1 .2204+2 1.393 .813+0 .534–1 .5561+1 1.998 .131–1 –.812–4 .4861+1 1.438 .579+0 .252–1 .9138+1 1.478 .600+0 .253–1 .2076+1 0.889 .832+0 .142+0 .2989+1 0.875 .827+0 .145+0 .1017+1 1.998 .623–2 –.730–4 .7063+0 1.457 .546+0 .211–1
4000 .7577+1 1.942 .939+0 –.250–3 .8970+1 1.995 .222+0 –.128–3 .6803+1 1.277 .980+0 .694–1 .1273+2 1.327 .101+1 .667–1 .3303+1 1.996 .151+0 –.841–4 .2448+1 1.349 .789+0 .396–1 .4541+1 1.391 .816+0 .385–1 .7625+0 0.771 .957+0 .184+0 .1092+1 0.761 .951+0 .188+0 .5750+0 1.996 .139+0 –.771–4 .3421+0 1.362 .759+0 .353–1
5000 .6669+1 1.932 .113+1 –.241–3 .6566+1 1.990 .387+0 –.124–3 .4289+1 1.211 .113+1 .848–1 .7933+1 1.261 .117+1 .809–1 .2154+1 1.993 .306+0 –.851–4 .1390+1 1.267 .958+0 .554–1 .2549+1 1.310 .991+0 .533–1 .3393+0 0.673 .104+1 .224+0 .4836+0 0.671 .104+1 .228+0 .3636+0 1.993 .291+0 –.789–4 .1894+0 1.278 .932+0 .510–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Sr, Z = 38 (continued) Shell 4 p3/2 Eb = 22 eV 5s1/2 Eb = 5 eV
σ β γ δ σ β γ δ
100 .2433+3 0.703 .696–1 .214–1 .2257+2 1.991 .180+0 .236–4
200 .1407+3 1.302 .150+0 .607–2 .9107+1 1.992 .232+0 .657–5
500 .4574+2 1.640 .695–3 –.413–3 .2184+1 1.992 .145+0 –.223–4
1000 .1446+2 1.681 .142–1 .250–2 .6882+0 1.993 –.229–2 –.435–4
E (eV) 1500 .6481+1 1.646 .147+0 .602–2 .3360+0 1.995 –.675–1 –.554–4
2000 .3456+1 1.597 .297+0 .105–1 .1976+0 1.996 –.745–1 –.637–4
3000 .1317+1 1.496 .566+0 .214–1 .9048–1 1.998 .400–2 –.709–4
4000 .6299+0 1.403 .785+0 .344–1 .5078–1 1.996 .137+0 –.763–4
5000 .3451+0 1.320 .964+0 .491–1 .3196–1 1.994 .289+0 –.780–4
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1246+2 1.978 –.825+0 –.293–3 .5220+2 1.979 .772+0 –.566–4 .1133+3 1.038 –.242+0 –.643–2 .2344+3 1.041 –.247+0 –.691–2 .1376+3 1.988 .464+0 .120–4 .2186+3 0.984 .208+0 .554–1 .4824+3 0.971 .194+0 .515–1 .2154+4 0.571 –.269–1 .828–2
200 .1228+2 1.976 –.654+0 –.307–3 .4895+2 1.981 .560+0 –.891–4 .1019+3 1.191 –.232+0 –.159–2 .2097+3 1.206 –.239+0 –.777–3 .1083+3 1.988 .377+0 –.189–4 .1764+3 1.303 .179+0 .196–1 .3794+3 1.297 .164+0 .176–1 .1229+4 0.889 –.126–1 .178–1
500 .1173+2 1.974 –.334+0 –.314–3 .4060+2 1.985 .217+0 –.126–3 .7466+2 1.355 –.856–1 .123–1 .1514+3 1.385 –.918–1 .142–1 .6001+2 1.989 .179+0 –.544–4 .9426+2 1.558 –.292–2 .162–2 .1940+3 1.568 –.909–2 .199–2 .3005+3 1.183 .105+0 .358–1
1000 .1092+2 1.969 –.104–1 –.312–3 .3069+2 1.991 –.564–2 –.145–3 .4723+2 1.422 .158+0 .246–1 .9394+2 1.462 .159+0 .263–1 .2941+2 1.992 –.636–3 –.732–4 .4079+2 1.609 .234–1 .290–2 .8103+2 1.633 .247–1 .451–2 .6317+2 1.208 .324+0 .570–1
E (eV) 1500 .1018+2 1.964 .218+0 –.307–3 .2391+2 1.995 –.668–1 –.151–3 .3166+2 1.425 .355+0 .328–1 .6202+2 1.470 .365+0 .338–1 .1732+2 1.994 –.703–1 –.815–4 .2124+2 1.584 .156+0 .686–2 .4133+2 1.616 .163+0 .856–2 .2111+2 1.138 .498+0 .767–1
2000 .9506+1 1.959 .399+0 –.300–3 .1907+2 1.997 –.580–1 –.151–3 .2217+2 1.408 .518+0 .401–1 .4289+2 1.456 .534+0 .403–1 .1134+2 1.996 –.784–1 –.860–4 .1243+2 1.543 .299+0 .118–1 .2384+2 1.579 .311+0 .132–1 .9002+1 1.057 .636+0 .977–1
3000 .8325+1 1.950 .689+0 –.291–3 .1280+2 1.997 .464–1 –.150–3 .1198+2 1.352 .775+0 .540–1 .2274+2 1.402 .801+0 .526–1 .5852+1 1.997 –.431–2 –.925–4 .5287+1 1.451 .558+0 .236–1 .9943+1 1.493 .579+0 .238–1 .2455+1 0.910 .832+0 .139+0
4000 .7331+1 1.940 .919+0 –.282–3 .9074+1 1.995 .195+0 –.147–3 .7134+1 1.288 .970+0 .682–1 .1334+2 1.340 .100+1 .654–1 .3504+1 1.996 .125+0 –.961–4 .2698+1 1.365 .769+0 .373–1 .5002+1 1.409 .798+0 .364–1 .9144+0 0.792 .962+0 .180+0
5000 .6490+1 1.931 .112+1 –.273–3 .6700+1 1.991 .354+0 –.142–3 .4553+1 1.224 .113+1 .831–1 .8410+1 1.277 .117+1 .791–1 .2299+1 1.994 .273+0 –.976–4 .1545+1 1.285 .943+0 .525–1 .2833+1 1.331 .976+0 .504–1 .4109+0 0.694 .105+1 .219+0
Y, Z = 39 Shell 1s1/2 Eb = 17042 eV 2s1/2 Eb = 2376 eV 2 p1/2 Eb = 2158 eV 2 p3/2 Eb = 2083 eV 3s1/2 Eb = 398 eV 3 p1/2 Eb = 316 eV 3 p3/2 Eb = 304 eV 3d3/2 Eb = 163 eV
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Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Y, Z = 39 (continued) Shell 3d5/2 Eb = 161 eV 4s1/2 Eb = 49 eV 4 p1/2 Eb = 30 eV 4 p3/2 Eb = 29 eV 4d3/2 Eb = 6 eV 5s1/2 Eb = 6 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3251+4 0.593 –.267–1 .744–2 .1554+3 1.991 .222+0 .222–4 .1165+3 0.680 .636–1 .242–1 .2630+3 0.693 .638–1 .232–1 .1765+3 0.056 .191–1 –.177–1 .2676+2 1.990 .183+0 .272–4
200 .1840+4 0.908 –.110–1 .172–1 .7816+2 1.991 .243+0 .417–6 .7242+2 1.303 .169+0 .762–2 .1558+3 1.290 .157+0 .742–2 .1363+3 0.882 –.161–1 .321–2 .1097+2 1.991 .235+0 .890–5
500 .4444+3 1.185 .109+0 .355–1 .2362+2 1.991 .151+0 –.288–4 .2542+2 1.636 .140–1 –.776–3 .5169+2 1.636 .784–2 –.377–3 .2874+2 1.266 .729–1 .247–1 .2650+1 1.991 .155+0 –.243–4
1000 .9250+2 1.196 .326+0 .575–1 .8125+1 1.992 .407–2 –.516–4 .8472+1 1.666 .385–2 .787–3 .1662+2 1.685 .509–2 .223–2 .5197+1 1.262 .285+0 .463–1 .8331+0 1.992 .706–2 –.483–4
E (eV) 1500 .3072+2 1.120 .498+0 .782–1 .4106+1 1.994 –.654–1 –.643–4 .3923+1 1.626 .123+0 .379–2 .7551+1 1.654 .130+0 .548–2 .1610+1 1.174 .467+0 .667–1 .4078+0 1.994 –.645–1 –.620–4
2000 .1304+2 1.039 .633+0 .999–1 .2460+1 1.996 –.777–1 –.724–4 .2141+1 1.575 .263+0 .807–2 .4066+1 1.609 .275+0 .955–2 .6543+0 1.081 .611+0 .882–1 .2403+0 1.996 –.786–1 –.711–4
3000 .3531+1 0.894 .826+0 .142+0 .1150+1 1.997 –.103–1 –.829–4 .8417+0 1.472 .523+0 .193–1 .1570+1 1.512 .543+0 .198–1 .1690+0 0.920 .811+0 .130+0 .1104+0 1.997 –.127–1 –.812–4
4000 .1308+1 0.781 .956+0 .184+0 .6528+0 1.997 .113+0 –.880–4 .4116+0 1.380 .737+0 .327–1 .7574+0 1.423 .764+0 .321–1 .6116–1 0.799 .946+0 .172+0 .6215–1 1.997 .111+0 –.862–4
5000 .5850+0 0.690 .105+1 .223+0 .4143+0 1.994 .258+0 –.904–4 .2295+0 1.297 .914+0 .478–1 .4179+0 1.341 .947+0 .460–1 .2696–1 0.698 .104+1 .212+0 .3924–1 1.994 .256+0 –.894–4
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1174+2 1.976 –.855+0 –.330–3 .4899+2 1.977 .794+0 –.623–4 .1053+3 1.033 –.255+0 –.795–2 .2182+3 1.037 –.260+0 –.842–2
200 .1159+2 1.975 –.682+0 –.346–3 .4612+2 1.979 .582+0 –.986–4 .9539+2 1.184 –.245+0 –.271–2 .1965+3 1.200 –.254+0 –.179–2
500 .1110+2 1.972 –.360+0 –.354–3 .3865+2 1.984 .237+0 –.141–3 .7113+2 1.349 –.101+0 .116–1 .1445+3 1.380 –.108+0 .138–1
1000 .1036+2 1.967 –.344–1 –.350–3 .2961+2 1.990 .559–2 –.162–3 .4603+2 1.418 .140+0 .241–1 .9166+2 1.460 .141+0 .260–1
E (eV) 1500 .9694+1 1.962 .196+0 –.345–3 .2332+2 1.994 –.648–1 –.170–3 .3141+2 1.424 .339+0 .325–1 .6160+2 1.471 .348+0 .337–1
2000 .9084+1 1.958 .377+0 –.338–3 .1877+2 1.996 –.641–1 –.171–3 .2231+2 1.410 .503+0 .398–1 .4320+2 1.460 .518+0 .401–1
3000 .8006+1 1.948 .668+0 –.328–3 .1278+2 1.997 .283–1 –.170–3 .1233+2 1.358 .761+0 .532–1 .2339+2 1.412 .788+0 .519–1
4000 .7091+1 1.939 .900+0 –.319–3 .9160+1 1.995 .169+0 –.167–3 .7452+1 1.298 .960+0 .670–1 .1393+2 1.353 .996+0 .643–1
5000 .6311+1 1.929 .110+1 –.309–3 .6822+1 1.991 .323+0 –.162–3 .4812+1 1.237 .112+1 .814–1 .8880+1 1.292 .116+1 .774–1
Zr, Z = 40 Shell 1s1/2 Eb = 18002 eV 2s1/2 Eb = 2536 eV 2 p1/2 Eb = 2311 eV 2 p3/2 Eb = 2227 eV
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M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Zr, Z = 40 (continued) Shell 3s1/2 Eb = 435 eV 3 p1/2 Eb = 349 eV 3 p3/2 Eb = 335 eV 3d3/2 Eb = 187 eV 3d5/2 Eb = 184 eV 4s1/2 Eb = 56 eV 4 p1/2 Eb = 35 eV 4 p3/2 Eb = 33 eV 4d3/2 Eb = 8 eV 5s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1306+3 1.987 .485+0 .148–4 .2089+3 0.978 .213+0 .599–1 .4636+3 0.964 .198+0 .557–1 .2039+4 0.556 –.310–1 .704–2 .3087+4 0.579 –.308–1 .618–2 .1599+3 1.990 .229+0 .268–4 .1237+3 0.667 .553–1 .258–1 .2834+3 0.681 .559–1 .245–1 .2001+3 −.024 .345–1 –.197–1 .2972+2 1.989 .186+0 .313–4
200 .1042+3 1.987 .395+0 –.194–4 .1703+3 1.291 .191+0 .223–1 .3683+3 1.285 .175+0 .201–1 .1202+4 0.872 –.195–1 .170–1 .1804+4 0.892 –.179–1 .163–1 .8303+2 1.991 .251+0 .173–5 .7856+2 1.289 .174+0 .900–2 .1709+3 1.276 .161+0 .870–2 .1675+3 0.856 –.174–1 .104–2 .1230+2 1.991 .238+0 .123–4
500 .5941+2 1.988 .195+0 –.599–4 .9380+2 1.551 .352–2 .203–2 .1940+3 1.561 –.379–2 .233–2 .3140+3 1.176 .952–1 .353–1 .4650+3 1.178 .991–1 .350–1 .2573+2 1.991 .162+0 –.315–4 .2819+2 1.633 .233–1 –.663–3 .5765+2 1.631 .160–1 –.308–3 .3743+2 1.266 .611–1 .231–1 .3013+1 1.991 .166+0 –.269–4
1000 .2983+2 1.991 .100–1 –.819–4 .4190+2 1.609 .143–1 .259–2 .8350+2 1.634 .149–1 .427–2 .6935+2 1.214 .312+0 .563–1 .1016+3 1.202 .315+0 .567–1 .8934+1 1.992 .138–1 –.575–4 .9548+1 1.670 –.362–2 .486–3 .1879+2 1.688 –.299–2 .197–2 .7017+1 1.273 .270+0 .445–1 .9444+0 1.992 .169–1 –.541–4
138
E (eV) 1500 .1781+2 1.993 –.667–1 –.921–4 .2225+2 1.588 .139+0 .624–2 .4340+2 1.621 .145+0 .811–2 .2379+2 1.150 .489+0 .755–1 .3463+2 1.132 .489+0 .768–1 .4540+1 1.993 –.612–1 –.722–4 .4478+1 1.634 .105+0 .314–2 .8634+1 1.662 .112+0 .497–2 .2219+1 1.190 .453+0 .643–1 .4633+0 1.993 –.600–1 –.700–4
2000 .1176+2 1.995 –.820–1 –.974–4 .1320+2 1.550 .278+0 .109–1 .2536+2 1.588 .290+0 .125–1 .1032+2 1.073 .629+0 .957–1 .1494+2 1.054 .627+0 .979–1 .2732+1 1.995 –.804–1 –.814–4 .2467+1 1.586 .241+0 .705–2 .4691+1 1.620 .252+0 .871–2 .9139+0 1.100 .600+0 .850–1 .2737+0 1.995 –.811–1 –.794–4
3000 .6141+1 1.997 –.201–1 –.105–3 .5725+1 1.464 .535+0 .220–1 .1077+2 1.507 .557+0 .225–1 .2875+1 0.931 .830+0 .136+0 .4134+1 0.913 .825+0 .139+0 .1284+1 1.997 –.254–1 –.935–4 .9828+0 1.487 .498+0 .175–1 .1833+1 1.529 .519+0 .182–1 .2400+0 0.944 .807+0 .126+0 .1262+0 1.997 –.274–1 –.914–4
4000 .3706+1 1.996 .994–1 –.109–3 .2958+1 1.380 .749+0 .351–1 .5483+1 1.426 .778+0 .344–1 .1086+1 0.814 .967+0 .176+0 .1553+1 0.801 .960+0 .180+0 .7317+0 1.996 .890–1 –.998–4 .4850+0 1.397 .714+0 .304–1 .8917+0 1.441 .742+0 .299–1 .8782–1 0.821 .947+0 .167+0 .7121–1 1.997 .862–1 –.985–4
5000 .2445+1 1.994 .241+0 –.111–3 .1710+1 1.302 .926+0 .497–1 .3132+1 1.350 .961+0 .477–1 .4928+0 0.715 .106+1 .214+0 .7009+0 0.708 .105+1 .218+0 .4659+0 1.994 .227+0 –.103–3 .2724+0 1.315 .894+0 .448–1 .4952+0 1.362 .928+0 .431–1 .3904–1 0.720 .105+1 .206+0 .4507–1 1.994 .224+0 –.101–3
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Nb, Z = 41 Shell 1s1/2 Eb = 18990 eV 2s1/2 Eb = 2702 eV 2 p1/2 Eb = 2469 eV 2 p3/2 Eb = 2375 eV 3s1/2 Eb = 473 eV 3 p1/2 Eb = 384 eV 3 p3/2 Eb = 367 eV 3d3/2 Eb = 212 eV 3d5/2 Eb = 209 eV 4s1/2 Eb = 62 eV 4 p1/2 Eb = 40 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1108+2 1.974 –.890+0 –.370–3 .4607+2 1.976 .824+0 –.671–4 .9836+2 1.023 –.267+0 –.951–2 .2041+3 1.026 –.272+0 –.100–1 .1244+3 1.985 .512+0 .198–4 .1992+3 0.959 .217+0 .668–1 .4456+3 0.944 .200+0 .619–1 .1947+4 0.533 –.345–1 .566–2 .2947+4 0.557 –.344–1 .479–2 .1613+3 1.988 .234+0 .344–4 .1239+3 0.620 .384–1 .278–1
200 .1095+2 1.973 –.715+0 –.389–3 .4354+2 1.978 .611+0 –.108–3 .8962+2 1.175 –.260+0 –.407–2 .1850+3 1.190 –.269+0 –.307–2 .1006+3 1.986 .419+0 –.188–4 .1642+3 1.275 .207+0 .260–1 .3581+3 1.267 .189+0 .235–1 .1184+4 0.848 –.270–1 .159–1 .1778+4 0.870 –.255–1 .153–1 .8676+2 1.990 .260+0 .449–5 .8195+2 1.264 .181+0 .109–1
500 .1052+2 1.970 –.389+0 –.399–3 .3684+2 1.983 .260+0 –.157–3 .6795+2 1.342 –.118+0 .108–1 .1382+3 1.374 –.127+0 .132–1 .5886+2 1.987 .214+0 –.657–4 .9327+2 1.542 .119–1 .258–2 .1941+3 1.552 .327–2 .277–2 .3287+3 1.166 .837–1 .348–1 .4869+3 1.170 .880–1 .344–1 .2765+2 1.990 .175+0 –.341–4 .3042+2 1.627 .349–1 –.509–3
1000 .9843+1 1.966 –.605–1 –.394–3 .2857+2 1.989 .186–1 –.182–3 .4490+2 1.414 .122+0 .236–1 .8954+2 1.458 .122+0 .258–1 .3023+2 1.990 .222–1 –.918–4 .4295+2 1.608 .573–2 .230–2 .8597+2 1.634 .554–2 .407–2 .7595+2 1.218 .300+0 .555–1 .1113+3 1.206 .304+0 .559–1 .9671+1 1.991 .248–1 –.640–4 .1047+2 1.673 –.102–1 .207–3
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E (eV) 1500 .9241+1 1.961 .170+0 –.387–3 .2274+2 1.993 –.611–1 –.190–3 .3116+2 1.424 .320+0 .321–1 .6117+2 1.472 .329+0 .335–1 .1828+2 1.992 –.615–1 –.103–3 .2326+2 1.592 .122+0 .565–2 .4549+2 1.626 .128+0 .768–2 .2670+2 1.163 .480+0 .746–1 .3884+2 1.144 .481+0 .759–1 .4936+1 1.993 –.555–1 –.803–4 .4965+1 1.641 .879–1 .255–2
2000 .8687+1 1.956 .354+0 –.381–3 .1846+2 1.995 –.690–1 –.193–3 .2243+2 1.412 .486+0 .393–1 .4347+2 1.464 .502+0 .399–1 .1218+2 1.994 –.844–1 –.110–3 .1398+2 1.557 .258+0 .100–1 .2692+2 1.597 .270+0 .118–1 .1176+2 1.089 .622+0 .939–1 .1702+2 1.068 .620+0 .961–1 .2981+1 1.994 –.820–1 –.912–4 .2761+1 1.596 .219+0 .609–2
3000 .7701+1 1.947 .647+0 –.370–3 .1275+2 1.997 .112–1 –.193–3 .1265+2 1.364 .747+0 .525–1 .2401+2 1.420 .775+0 .514–1 .6431+1 1.996 –.349–1 –.119–3 .6175+1 1.475 .513+0 .206–1 .1163+2 1.521 .535+0 .213–1 .3346+1 0.950 .828+0 .133+0 .4806+1 0.931 .822+0 .136+0 .1408+1 1.996 –.395–1 –.105–3 .1114+1 1.501 .474+0 .159–1
4000 .6858+1 1.937 .879+0 –.359–3 .9230+1 1.995 .143+0 –.189–3 .7763+1 1.307 .949+0 .660–1 .1450+2 1.365 .986+0 .632–1 .3911+1 1.996 .754–1 –.124–3 .3231+1 1.395 .728+0 .331–1 .5987+1 1.443 .758+0 .325–1 .1281+1 0.834 .970+0 .171+0 .1829+1 0.820 .963+0 .176+0 .8050+0 1.996 .657–1 –.113–3 .5541+0 1.413 .691+0 .281–1
5000 .6135+1 1.927 .108+1 –.348–3 .6931+1 1.992 .292+0 –.185–3 .5071+1 1.248 .111+1 .799–1 .9350+1 1.306 .116+1 .758–1 .2595+1 1.994 .210+0 –.127–3 .1884+1 1.319 .908+0 .470–1 .3449+1 1.369 .944+0 .452–1 .5866+0 0.736 .107+1 .209+0 .8333+0 0.727 .106+1 .214+0 .5140+0 1.995 .196+0 –.117–3 .3133+0 1.333 .873+0 .419–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Nb, Z = 41 (continued) Shell 4 p3/2 Eb = 38 eV 4d3/2 Eb = 7 eV 5s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ
100 .2864+3 0.637 .409–1 .264–1 .1769+3 −.178 .583–1 –.229–1 .2651+2 1.987 .187+0 .382–4
200 .1794+3 1.251 .167+0 .105–1 .1741+3 0.812 –.168–1 –.154–2 .1071+2 1.990 .238+0 .172–4
500 .6238+2 1.625 .263–1 –.208–3 .4164+2 1.262 .480–1 .214–1 .2705+1 1.990 .177+0 –.251–4
1000 .2061+2 1.691 –.103–1 .173–2 .8024+1 1.283 .254+0 .427–1 .8511+0 1.991 .283–1 –.602–4
E (eV) 1500 .9569+1 1.670 .938–1 .451–2 .2583+1 1.205 .438+0 .619–1 .4175+0 1.992 –.544–1 –.780–4
2000 .5243+1 1.631 .230+0 .796–2 .1076+1 1.119 .587+0 .818–1 .2471+0 1.994 –.827–1 –.883–4
3000 .2072+1 1.544 .495+0 .168–1 .2867+0 0.966 .802+0 .122+0 .1143+0 1.996 –.410–1 –.103–3
4000 .1016+1 1.460 .720+0 .278–1 .1060+0 0.843 .947+0 .162+0 .6464–1 1.996 .629–1 –.111–3
5000 .5677+0 1.382 .908+0 .404–1 .4747–1 0.742 .105+1 .200+0 .4100–1 1.995 .193+0 –.115–3
100 .1047+2 1.973 –.923+0 –.415–3 .4337+2 1.975 .848+0 –.732–4 .9191+2 1.017 –.280+0 –.112–1 .1910+3 1.020 –.285+0 –.117–1 .1186+3 1.984 .534+0 .241–4 .1916+3 0.949 .219+0 .716–1 .4293+3 0.933 .202+0 .666–1
200 .1036+2 1.972 –.745+0 –.436–3 .4113+2 1.977 .635+0 –.119–3 .8421+2 1.168 –.274+0 –.537–2 .1741+3 1.183 –.284+0 –.427–2 .9702+2 1.984 .438+0 –.184–4 .1593+3 1.261 .219+0 .292–1 .3481+3 1.254 .199+0 .264–1
500 .9969+1 1.969 –.416+0 –.448–3 .3513+2 1.982 .282+0 –.174–3 .6485+2 1.335 –.135+0 .100–1 .1321+3 1.368 –.144+0 .126–1 .5820+2 1.986 .231+0 –.717–4 .9281+2 1.534 .205–1 .319–2 .1937+3 1.544 .105–1 .329–2
1000 .9360+1 1.964 –.855–1 –.442–3 .2757+2 1.988 .317–1 –.203–3 .4370+2 1.411 .104+0 .231–1 .8728+2 1.455 .104+0 .256–1 .3056+2 1.989 .343–1 –.102–3 .4395+2 1.607 –.129–2 .207–2 .8815+2 1.633 –.230–2 .390–2
E (eV) 1500 .8813+1 1.959 .146+0 –.434–3 .2215+2 1.992 –.567–1 –.213–3 .3081+2 1.422 .303+0 .317–1 .6056+2 1.473 .311+0 .333–1 .1872+2 1.991 –.558–1 –.116–3 .2423+2 1.596 .106+0 .511–2 .4746+2 1.631 .112+0 .731–2
2000 .8309+1 1.954 .332+0 –.428–3 .1813+2 1.994 –.725–1 –.217–3 .2247+2 1.413 .470+0 .390–1 .4359+2 1.467 .486+0 .397–1 .1258+2 1.993 –.856–1 –.124–3 .1475+2 1.564 .239+0 .922–2 .2843+2 1.604 .250+0 .112–1
3000 .7407+1 1.945 .626+0 –.415–3 .1268+2 1.996 –.417–2 –.217–3 .1293+2 1.369 .733+0 .519–1 .2455+2 1.428 .761+0 .508–1 .6714+1 1.996 –.477–1 –.134–3 .6630+1 1.486 .491+0 .192–1 .1248+2 1.533 .513+0 .202–1
4000 .6630+1 1.935 .859+0 –.403–3 .9279+1 1.995 .120+0 –.214–3 .8052+1 1.316 .937+0 .649–1 .1504+2 1.376 .975+0 .622–1 .4113+1 1.996 .532–1 –.140–3 .3511+1 1.409 .707+0 .312–1 .6502+1 1.459 .737+0 .308–1
5000 .5959+1 1.926 .106+1 –.392–3 .7024+1 1.992 .263+0 –.210–3 .5319+1 1.259 .110+1 .784–1 .9800+1 1.320 .115+1 .742–1 .2744+1 1.994 .181+0 –.144–3 .2066+1 1.335 .888+0 .445–1 .3777+1 1.387 .926+0 .428–1
Mo, Z = 42 Shell 1s1/2 Eb = 20006 eV 2s1/2 Eb = 2872 eV 2 p1/2 Eb = 2631 eV 2 p3/2 Eb = 2526 eV 3s1/2 Eb = 511 eV 3 p1/2 Eb = 416 eV 3 p3/2 Eb = 399 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
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M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Mo, Z = 42 (continued) Shell 3d3/2 Eb = 236 eV 3d5/2 Eb = 234 eV 4s1/2 Eb = 68 eV 4 p1/2 Eb = 44 eV 4 p3/2 Eb = 41 eV 4d3/2 Eb = 8 eV 4d5/2 Eb = 8 eV 5s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1864+4 0.518 –.374–1 .432–2 .2811+4 0.543 –.376–1 .347–2 .1640+3 1.987 .239+0 .414–4 .1284+3 0.597 .270–1 .290–1 .3016+3 0.616 .304–1 .274–1 .1831+3 −.283 .775–1 –.228–1 .2810+3 −.212 .769–1 –.236–1 .2792+2 1.986 .185+0 .448–4
200 .1160+4 0.829 –.338–1 .147–1 .1738+4 0.853 –.324–1 .141–1 .9068+2 1.988 .267+0 .714–5 .8674+2 1.246 .184+0 .125–1 .1920+3 1.232 .169+0 .120–1 .1985+3 0.777 –.136–1 –.351–2 .2956+3 0.820 –.144–1 –.321–2 .1133+2 1.988 .240+0 .201–4
500 .3410+3 1.157 .724–1 .342–1 .5044+3 1.162 .771–1 .338–1 .2968+2 1.989 .186+0 –.366–4 .3304+2 1.622 .462–1 –.297–3 .6817+2 1.618 .362–1 –.495–4 .5064+2 1.259 .360–1 .198–1 .7393+2 1.268 .398–1 .197–1 .2903+1 1.989 .187+0 –.269–4
1000 .8235+2 1.221 .288+0 .549–1 .1205+3 1.210 .293+0 .552–1 .1048+2 1.990 .354–1 –.709–4 .1154+2 1.676 –.151–1 –.218–4 .2280+2 1.694 –.160–1 .152–2 .1007+2 1.292 .238+0 .410–1 .1452+2 1.279 .243+0 .412–1 .9155+0 1.990 .391–1 –.651–4
E (eV) 1500 .2967+2 1.173 .469+0 .734–1 .4312+2 1.154 .471+0 .747–1 .5373+1 1.992 –.494–1 –.895–4 .5534+1 1.648 .725–1 .203–2 .1068+2 1.677 .779–1 .411–2 .3301+1 1.220 .423+0 .596–1 .4731+1 1.199 .425+0 .608–1 .4494+0 1.992 –.478–1 –.862–4
2000 .1327+2 1.103 .613+0 .919–1 .1919+2 1.082 .612+0 .942–1 .3257+1 1.994 –.823–1 –.102–3 .3104+1 1.605 .198+0 .523–2 .5900+1 1.641 .209+0 .729–2 .1393+1 1.137 .575+0 .788–1 .1986+1 1.113 .574+0 .810–1 .2664+0 1.993 –.818–1 –.991–4
3000 .3854+1 0.969 .825+0 .130+0 .5530+1 0.948 .819+0 .133+0 .1546+1 1.996 –.517–1 –.118–3 .1268+1 1.514 .450+0 .143–1 .2358+1 1.558 .471+0 .155–1 .3769+0 0.987 .796+0 .118+0 .5333+0 0.964 .791+0 .122+0 .1237+0 1.996 –.538–1 –.115–3
4000 .1496+1 0.855 .972+0 .168+0 .2133+1 0.838 .964+0 .172+0 .8870+0 1.996 .441–1 –.127–3 .6361+0 1.429 .667+0 .259–1 .1165+1 1.477 .697+0 .259–1 .1407+0 0.865 .946+0 .157+0 .1979+0 0.847 .939+0 .162+0 .7012–1 1.996 .415–1 –.125–3
5000 .6916+0 0.757 .108+1 .204+0 .9811+0 0.746 .107+1 .209+0 .5679+0 1.995 .168+0 –.132–3 .3619+0 1.351 .851+0 .391–1 .6549+0 1.401 .888+0 .378–1 .6353–1 0.764 .105+1 .194+0 .8892–1 0.751 .105+1 .200+0 .4457–1 1.995 .164+0 –.130–3
σ β γ δ σ β γ δ
100 .9903+1 1.971 –.950+0 –.464–3 .4086+2 1.973 .865+0 –.813–4
200 .9804+1 1.970 –.773+0 –.488–3 .3886+2 1.975 .654+0 –.132–3
500 .9458+1 1.967 –.442+0 –.502–3 .3347+2 1.980 .301+0 –.193–3
1000 .8906+1 1.962 –.109+0 –.496–3 .2657+2 1.987 .446–1 –.226–3
E (eV) 1500 .8408+1 1.957 .124+0 –.487–3 .2155+2 1.991 –.514–1 –.238–3
2000 .7948+1 1.953 .310+0 –.479–3 .1778+2 1.994 –.743–1 –.243–3
3000 .7122+1 1.943 .604+0 –.465–3 .1259+2 1.996 –.178–1 –.244–3
4000 .6407+1 1.934 .839+0 –.452–3 .9303+1 1.995 .975–1 –.241–3
5000 .5784+1 1.924 .104+1 –.440–3 .7098+1 1.993 .235+0 –.237–3
Tc, Z = 43 Shell 1s1/2 Eb = 21050 eV 2s1/2 Eb = 3048 eV
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M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Tc, Z = 43 (continued) Shell 2 p1/2 Eb = 2800 eV 2 p3/2 Eb = 2683 eV 3s1/2 Eb = 551 eV 3 p1/2 Eb = 451 eV 3 p3/2 Eb = 432 eV 3d3/2 Eb = 263 eV 3d5/2 Eb = 259 eV 4s1/2 Eb = 74 eV 4 p1/2 Eb = 49 eV 4 p3/2 Eb = 45 eV 4d3/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .8583+2 1.015 –.294+0 –.129–1 .1786+3 1.018 –.299+0 –.134–1 .1128+3 1.983 .552+0 .272–4 .1837+3 0.949 .223+0 .746–1 .4134+3 0.933 .205+0 .693–1 .1761+4 0.514 –.407–1 .308–2 .2670+4 0.540 –.408–1 .223–2 .1681+3 1.986 .244+0 .467–4 .1361+3 0.605 .247–1 .299–1 .3244+3 0.623 .281–1 .281–1 .2273+3 −.310 .825–1 –.179–1
200 .7902+2 1.163 –.288+0 –.664–2 .1636+3 1.179 –.299+0 –.541–2 .9329+2 1.983 .454+0 –.187–4 .1538+3 1.253 .227+0 .317–1 .3377+3 1.245 .206+0 .287–1 .1120+4 0.816 –.400–1 .136–1 .1684+4 0.840 –.385–1 .129–1 .9484+2 1.987 .271+0 .921–5 .9249+2 1.235 .185+0 .137–1 .2071+3 1.220 .170+0 .131–1 .2442+3 0.753 –.886–2 –.469–2
500 .6176+2 1.329 –.149+0 .933–2 .1260+3 1.363 –.160+0 .122–1 .5730+2 1.985 .246+0 –.782–4 .9178+2 1.527 .285–1 .383–2 .1924+3 1.536 .172–1 .383–2 .3483+3 1.148 .620–1 .335–1 .5165+3 1.155 .668–1 .330–1 .3182+2 1.988 .195+0 –.394–4 .3594+2 1.617 .565–1 –.495–4 .7470+2 1.612 .451–1 .147–3 .6499+2 1.256 .259–1 .182–1
1000 .4241+2 1.407 .883–1 .227–1 .8483+2 1.453 .865–1 .254–1 .3077+2 1.987 .460–1 –.113–3 .4468+2 1.606 –.673–2 .190–2 .8992+2 1.632 –.860–2 .380–2 .8808+2 1.223 .277+0 .544–1 .1291+3 1.212 .282+0 .546–1 .1136+2 1.989 .454–1 –.780–4 .1276+2 1.678 –.183–1 –.203–3 .2532+2 1.695 –.200–1 .136–2 .1333+2 1.301 .223+0 .394–1
142
E (eV) 1500 .3036+2 1.421 .286+0 .314–1 .5974+2 1.474 .294+0 .332–1 .1909+2 1.990 –.495–1 –.129–3 .2507+2 1.599 .919–1 .463–2 .4923+2 1.634 .970–1 .699–2 .3255+2 1.182 .459+0 .723–1 .4734+2 1.163 .461+0 .736–1 .5851+1 1.991 –.429–1 –.994–4 .6182+1 1.653 .589–1 .158–2 .1197+2 1.683 .637–1 .377–2 .4455+1 1.235 .407+0 .575–1
2000 .2242+2 1.413 .454+0 .386–1 .4353+2 1.470 .469+0 .395–1 .1293+2 1.993 –.853–1 –.139–3 .1547+2 1.570 .220+0 .847–2 .2985+2 1.611 .231+0 .107–1 .1481+2 1.117 .605+0 .904–1 .2141+2 1.094 .604+0 .926–1 .3560+1 1.993 –.811–1 –.114–3 .3499+1 1.613 .178+0 .445–2 .6665+1 1.650 .189+0 .670–2 .1904+1 1.155 .561+0 .761–1
3000 .1315+2 1.374 .718+0 .513–1 .2498+2 1.435 .747+0 .503–1 .6983+1 1.995 –.587–1 –.151–3 .7075+1 1.496 .469+0 .180–1 .1333+2 1.545 .491+0 .192–1 .4391+1 0.987 .821+0 .127+0 .6298+1 0.965 .816+0 .131+0 .1700+1 1.995 –.621–1 –.132–3 .1447+1 1.526 .425+0 .129–1 .2695+1 1.572 .446+0 .143–1 .5237+0 1.008 .789+0 .114+0
4000 .8311+1 1.323 .925+0 .640–1 .1552+2 1.386 .964+0 .613–1 .4309+1 1.996 .329–1 –.158–3 .3791+1 1.422 .685+0 .293–1 .7020+1 1.474 .716+0 .292–1 .1728+1 0.874 .972+0 .164+0 .2463+1 0.856 .964+0 .169+0 .9786+0 1.996 .244–1 –.143–3 .7323+0 1.444 .644+0 .239–1 .1342+1 1.493 .674+0 .241–1 .1976+0 0.886 .944+0 .152+0
5000 .5552+1 1.269 .109+1 .771–1 .1022+2 1.333 .114+1 .728–1 .2891+1 1.994 .154+0 –.162–3 .2251+1 1.350 .869+0 .421–1 .4112+1 1.404 .908+0 .406–1 .8071+0 0.777 .108+1 .199+0 .1144+1 0.764 .107+1 .205+0 .6283+0 1.995 .141+0 –.149–3 .4194+0 1.367 .829+0 .365–1 .7588+0 1.419 .867+0 .354–1 .8990–1 0.785 .106+1 .189+0
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Tc, Z = 43 (continued) Shell 4d5/2 Eb = 8 eV 5s1/2 Eb = 7 eV
σ β γ δ σ β γ δ
100 .3507+3 −.235 .831–1 –.192–1 .3575+2 1.984 .184+0 .490–4
200 .3656+3 0.799 –.100–1 –.443–2 .1484+2 1.987 .241+0 .239–4
500 .9529+2 1.266 .297–1 .181–1 .3817+1 1.988 .196+0 –.289–4
1000 .1931+2 1.288 .228+0 .395–1 .1202+1 1.989 .492–1 –.729–4
E (eV) 1500 .6406+1 1.213 .410+0 .586–1 .5900+0 1.991 –.411–1 –.950–4
2000 .2724+1 1.130 .561+0 .782–1 .3503+0 1.993 –.809–1 –.110–3
3000 .7434+0 0.983 .784+0 .118+0 .1631+0 1.995 –.636–1 –.130–3
4000 .2787+0 0.866 .936+0 .157+0 .9271–1 1.996 .215–1 –.140–3
5000 .1262+0 0.770 .105+1 .195+0 .5904–1 1.995 .137+0 –.147–3
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .9378+1 1.969 –.988+0 –.517–3 .3858+2 1.972 .898+0 –.863–4 .8063+2 1.003 –.305+0 –.147–1 .1681+3 1.005 –.311+0 –.153–1 .1078+3 1.981 .581+0 .351–4 .1757+3 0.925 .223+0 .825–1 .3985+3 0.908 .204+0 .766–1 .1701+4 0.492 –.421–1 .188–2
200 .9295+1 1.968 –.808+0 –.545–3 .3682+2 1.974 .686+0 –.143–3 .7462+2 1.153 –.304+0 –.828–2 .1547+3 1.169 –.315+0 –.700–2 .9009+2 1.982 .480+0 –.164–4 .1485+3 1.234 .243+0 .364–1 .3286+3 1.225 .220+0 .329–1 .1102+4 0.790 –.468–1 .121–1
500 .8988+1 1.965 –.474+0 –.563–3 .3197+2 1.979 .328+0 –.213–3 .5912+2 1.321 –.168+0 .834–2 .1208+3 1.356 –.180+0 .114–1 .5657+2 1.983 .267+0 –.846–4 .9092+2 1.516 .405–1 .476–2 .1919+3 1.525 .273–1 .459–2 .3604+3 1.136 .496–1 .328–1
1000 .8485+1 1.960 –.137+0 –.556–3 .2564+2 1.985 .607–1 –.252–3 .4130+2 1.402 .691–1 .222–1 .8273+2 1.450 .662–1 .252–1 .3101+2 1.986 .607–1 –.126–3 .4546+2 1.604 –.121–1 .175–2 .9192+2 1.631 –.150–1 .370–2 .9480+2 1.225 .264+0 .537–1
E (eV) 1500 .8031+1 1.956 .985–1 –.547–3 .2097+2 1.990 –.447–1 –.266–3 .2997+2 1.419 .269+0 .310–1 .5906+2 1.474 .275+0 .332–1 .1947+2 1.989 –.420–1 –.145–3 .2595+2 1.601 .776–1 .415–2 .5113+2 1.638 .819–1 .669–2 .3582+2 1.190 .447+0 .711–1
2000 .7611+1 1.951 .286+0 –.537–3 .1743+2 1.993 –.753–1 –.272–3 .2240+2 1.414 .436+0 .382–1 .4353+2 1.473 .451+0 .394–1 .1330+2 1.992 –.842–1 –.156–3 .1621+2 1.575 .201+0 .773–2 .3136+2 1.618 .211+0 .102–1 .1654+2 1.130 .596+0 .887–1
3000 .6854+1 1.941 .581+0 –.521–3 .1250+2 1.995 –.309–1 –.274–3 .1338+2 1.378 .702+0 .507–1 .2543+2 1.441 .731+0 .499–1 .7258+1 1.995 –.692–1 –.169–3 .7539+1 1.506 .446+0 .167–1 .1422+2 1.556 .469+0 .182–1 .4996+1 1.005 .817+0 .124+0
4000 .6193+1 1.932 .817+0 –.507–3 .9320+1 1.995 .757–1 –.272–3 .8573+1 1.330 .912+0 .631–1 .1600+2 1.396 .952+0 .605–1 .4510+1 1.995 .132–1 –.177–3 .4086+1 1.434 .662+0 .276–1 .7568+1 1.489 .694+0 .277–1 .1991+1 0.894 .973+0 .160+0
5000 .5614+1 1.922 .102+1 –.493–3 .7165+1 1.993 .207+0 –.268–3 .5789+1 1.278 .108+1 .758–1 .1065+2 1.345 .113+1 .715–1 .3042+1 1.994 .127+0 –.183–3 .2447+1 1.365 .848+0 .398–1 .4468+1 1.421 .888+0 .386–1 .9385+0 0.797 .109+1 .195+0
Ru, Z = 44 Shell 1s1/2 Eb = 22123 eV 2s1/2 Eb = 3230 eV 2 p1/2 Eb = 2973 eV 2 p3/2 Eb = 2844 eV 3s1/2 Eb = 592 eV 3 p1/2 Eb = 488 eV 3 p3/2 Eb = 466 eV 3d3/2 Eb = 290 eV
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Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Ru, Z = 44 (continued) Shell 3d5/2 Eb = 286 eV 4s1/2 Eb = 81 eV 4 p1/2 Eb = 53 eV 4 p3/2 Eb = 49 eV 4d3/2 Eb = 8 eV 4d5/2 Eb = 8 eV 5s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2578+4 0.518 –.423–1 .101–2 .1655+3 1.984 .250+0 .599–4 .1330+3 0.544 .305–2 .313–1 .3203+3 0.566 .877–2 .294–1 .1804+3 −.513 .109+0 –.176–1 .2788+3 −.432 .112+0 –.199–1 .2956+2 1.982 .179+0 .611–4
200 .1657+4 0.816 –.456–1 .114–1 .9655+2 1.986 .282+0 .148–4 .9391+2 1.204 .186+0 .160–1 .2119+3 1.189 .171+0 .153–1 .2395+3 0.695 –.620–3 –.669–2 .3578+3 0.746 –.233–2 –.642–2 .1219+2 1.986 .245+0 .271–4
500 .5345+3 1.144 .548–1 .323–1 .3348+2 1.987 .210+0 –.416–4 .3793+2 1.608 .715–1 .291–3 .7910+2 1.602 .584–1 .421–3 .6951+2 1.246 .140–1 .165–1 .1016+3 1.260 .176–1 .164–1 .3223+1 1.987 .207+0 –.322–4
1000 .1389+3 1.214 .269+0 .538–1 .1208+2 1.988 .581–1 –.860–4 .1368+2 1.680 –.210–1 –.390–3 .2718+2 1.696 –.237–1 .119–2 .1466+2 1.308 .206+0 .377–1 .2114+2 1.297 .212+0 .378–1 .1022+1 1.988 .614–1 –.778–4
E (eV) 1500 .5207+2 1.171 .450+0 .723–1 .6247+1 1.990 –.353–1 –.111–3 .6692+1 1.659 .452–1 .113–2 .1296+2 1.689 .494–1 .346–2 .4970+1 1.248 .390+0 .553–1 .7114+1 1.226 .394+0 .564–1 .5028+0 1.990 –.326–1 –.105–3
2000 .2390+2 1.107 .596+0 .909–1 .3813+1 1.992 –.792–1 –.127–3 .3816+1 1.622 .158+0 .371–2 .7262+1 1.659 .168+0 .616–2 .2148+1 1.171 .546+0 .733–1 .3058+1 1.145 .547+0 .753–1 .2991+0 1.992 –.783–1 –.123–3
3000 .7160+1 0.981 .811+0 .128+0 .1829+1 1.995 –.720–1 –.147–3 .1597+1 1.538 .401+0 .115–1 .2967+1 1.585 .422+0 .132–1 .5991+0 1.028 .781+0 .110+0 .8459+0 1.002 .776+0 .114+0 .1397+0 1.994 –.730–1 –.144–3
4000 .2835+1 0.873 .964+0 .165+0 .1057+1 1.995 .523–2 –.160–3 .8144+0 1.458 .619+0 .219–1 .1488+1 1.510 .650+0 .224–1 .2280+0 0.908 .942+0 .148+0 .3199+0 0.885 .934+0 .153+0 .7959–1 1.995 .273–2 –.157–3
5000 .1329+1 0.782 .108+1 .201+0 .6800+0 1.995 .115+0 –.167–3 .4691+0 1.383 .806+0 .339–1 .8459+0 1.438 .845+0 .332–1 .1044+0 0.806 .106+1 .183+0 .1458+0 0.789 .105+1 .189+0 .5079–1 1.995 .111+0 –.164–3
σ β γ δ σ β γ δ σ β γ δ
100 .8889+1 1.967 –.102+1 –.576–3 .3644+2 1.970 .924+0 –.933–4 .7573+2 0.996 –.317+0 –.165–1
200 .8819+1 1.966 –.840+0 –.608–3 .3488+2 1.972 .712+0 –.157–3 .7039+2 1.145 –.318+0 –.980–2
500 .8545+1 1.963 –.503+0 –.628–3 .3051+2 1.977 .351+0 –.235–3 .5648+2 1.314 –.185+0 .739–2
1000 .8089+1 1.958 –.163+0 –.621–3 .2472+2 1.984 .764–1 –.279–3 .4011+2 1.398 .510–1 .216–1
E (eV) 1500 .7673+1 1.954 .735–1 –.611–3 .2038+2 1.988 –.369–1 –.297–3 .2950+2 1.417 .250+0 .306–1
2000 .7289+1 1.949 .262+0 –.601–3 .1706+2 1.992 –.748–1 –.304–3 .2230+2 1.414 .418+0 .378–1
3000 .6594+1 1.939 .559+0 –.582–3 .1238+2 1.995 –.422–1 –.307–3 .1356+2 1.382 .686+0 .501–1
4000 .5984+1 1.930 .795+0 –.566–3 .9315+1 1.995 .557–1 –.305–3 .8807+1 1.337 .898+0 .623–1
5000 .5447+1 1.921 .999+0 –.552–3 .7215+1 1.993 .180+0 –.302–3 .6010+1 1.287 .107+1 .746–1
Rh, Z = 45 Shell 1s1/2 Eb = 23225 eV 2s1/2 Eb = 3418 eV 2 p1/2 Eb = 3152 eV
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Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Rh, Z = 45 (continued) Shell 2 p3/2 Eb = 3010 eV 3s1/2 Eb = 634 eV 3 p1/2 Eb = 526 eV 3 p3/2 Eb = 501 eV 3d3/2 Eb = 318 eV 3d5/2 Eb = 313 eV 4s1/2 Eb = 87 eV 4 p1/2 Eb = 58 eV 4 p3/2 Eb = 53 eV 4d3/2 Eb = 9 eV 4d5/2 Eb = 9 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1581+3 0.997 –.324+0 –.172–1 .1029+3 1.980 .605+0 .419–4 .1682+3 0.912 .224+0 .882–1 .3840+3 0.894 .204+0 .818–1 .1632+4 0.479 –.436–1 .838–3 .2479+4 0.506 –.439–1 –.382–4 .1655+3 1.982 .254+0 .714–4 .1333+3 0.513 –.933–2 .322–1 .3265+3 0.538 –.238–2 .301–1 .1708+3 −.629 .119+0 –.124–1 .2647+3 −.546 .125+0 –.159–1
200 .1462+3 1.161 –.331+0 –.843–2 .8684+2 1.980 .501+0 –.147–4 .1433+3 1.220 .254+0 .402–1 .3192+3 1.210 .230+0 .364–1 .1073+4 0.770 –.528–1 .107–1 .1617+4 0.799 –.516–1 .995–2 .9891+2 1.985 .288+0 .199–4 .9635+2 1.182 .186+0 .178–1 .2202+3 1.167 .170+0 .170–1 .2541+3 0.650 .880–2 –.779–2 .3802+3 0.707 .670–2 –.758–2
500 .1156+3 1.350 –.198+0 .107–1 .5569+2 1.982 .286+0 –.912–4 .8975+2 1.507 .518–1 .572–2 .1905+3 1.516 .368–1 .539–2 .3685+3 1.124 .379–1 .320–1 .5472+3 1.134 .433–1 .314–1 .3528+2 1.986 .222+0 –.438–4 .4017+2 1.601 .851–1 .670–3 .8433+2 1.593 .703–1 .735–3 .7906+2 1.237 .427–2 .148–1 .1155+3 1.253 .770–2 .147–1
1000 .8048+2 1.447 .469–1 .250–1 .3116+2 1.985 .748–1 –.139–3 .4605+2 1.601 –.158–1 .165–2 .9352+2 1.629 –.199–1 .365–2 .1009+3 1.225 .250+0 .530–1 .1479+3 1.216 .256+0 .531–1 .1289+2 1.987 .700–1 –.940–4 .1475+2 1.681 –.219–1 –.529–3 .2940+2 1.697 –.257–1 .105–2 .1719+2 1.315 .190+0 .361–1 .2477+2 1.304 .196+0 .361–1
145
E (eV) 1500 .5821+2 1.474 .256+0 .331–1 .1980+2 1.988 –.335–1 –.161–3 .2673+2 1.603 .643–1 .373–2 .5283+2 1.640 .679–1 .643–2 .3901+2 1.198 .435+0 .702–1 .5672+2 1.179 .439+0 .713–1 .6690+1 1.989 –.271–1 –.122–3 .7280+1 1.664 .330–1 .751–3 .1413+2 1.694 .365–1 .318–2 .5920+1 1.260 .374+0 .534–1 .8467+1 1.238 .378+0 .544–1
2000 .4338+2 1.475 .433+0 .392–1 .1363+2 1.990 –.819–1 –.174–3 .1690+2 1.580 .182+0 .706–2 .3277+2 1.624 .193+0 .974–2 .1828+2 1.142 .586+0 .872–1 .2642+2 1.118 .586+0 .894–1 .4095+1 1.991 –.761–1 –.140–3 .4183+1 1.629 .139+0 .305–2 .7969+1 1.667 .149+0 .570–2 .2588+1 1.187 .531+0 .707–1 .3681+1 1.160 .532+0 .727–1
3000 .2578+2 1.447 .716+0 .495–1 .7520+1 1.994 –.780–1 –.190–3 .7992+1 1.515 .424+0 .156–1 .1509+2 1.567 .446+0 .173–1 .5632+1 1.021 .812+0 .122+0 .8067+1 0.996 .807+0 .126+0 .1975+1 1.994 –.799–1 –.164–3 .1771+1 1.550 .376+0 .102–1 .3290+1 1.598 .397+0 .122–1 .7330+0 1.047 .772+0 .106+0 .1034+1 1.019 .767+0 .110+0
4000 .1644+2 1.405 .939+0 .598–1 .4706+1 1.995 –.458–2 –.199–3 .4382+1 1.446 .640+0 .260–1 .8117+1 1.502 .673+0 .264–1 .2273+1 0.912 .972+0 .157+0 .3234+1 0.890 .963+0 .162+0 .1144+1 1.995 –.122–1 –.178–3 .9106+0 1.472 .594+0 .200–1 .1662+1 1.525 .625+0 .209–1 .2816+0 0.929 .939+0 .143+0 .3944+0 0.904 .931+0 .148+0
5000 .1105+2 1.356 .112+1 .703–1 .3190+1 1.994 .102+0 –.205–3 .2646+1 1.379 .827+0 .376–1 .4831+1 1.437 .868+0 .366–1 .1082+1 0.817 .109+1 .190+0 .1530+1 0.799 .108+1 .197+0 .7383+0 1.995 .901–1 –.187–3 .5277+0 1.399 .783+0 .315–1 .9500+0 1.455 .823+0 .310–1 .1299+0 0.827 .106+1 .178+0 .1810+0 0.808 .105+1 .184+0
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Rh, Z = 45 (continued) Shell 5s1/2 Eb = 7 eV
σ β γ δ
100 .2990+2 1.980 .176+0 .707–4
200 .1249+2 1.984 .248+0 .317–4
500 .3355+1 1.986 .218+0 –.340–4
1000 .1069+1 1.987 .732–1 –.865–4
E (eV) 1500 .5263+0 1.989 –.242–1 –.116–3
2000 .3133+0 1.991 –.751–1 –.135–3
3000 .1467+0 1.994 –.809–1 –.161–3
4000 .8380–1 1.995 –.146–1 –.175–3
5000 .5356–1 1.995 .866–1 –.183–3
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .8433+1 1.965 –.106+1 –.638–3 .3449+2 1.968 .960+0 –.978–4 .7132+2 0.982 –.328+0 –.185–1 .1492+3 0.982 –.335+0 –.194–1 .9844+2 1.978 .635+0 .527–4 .1611+3 0.886 .221+0 .969–1 .3703+3 0.866 .200+0 .899–1 .1587+4 0.460 –.435–1 .550–4 .2410+4 0.487 –.439–1 –.842–3
200 .8376+1 1.964 –.881+0 –.679–3 .3311+2 1.970 .749+0 –.169–3 .6661+2 1.132 –.334+0 –.116–1 .1386+3 1.147 –.347+0 –.102–1 .8388+2 1.979 .530+0 –.996–5 .1384+3 1.195 .268+0 .458–1 .3105+3 1.184 .241+0 .413–1 .1054+4 0.742 –.586–1 .896–2 .1588+4 0.772 –.577–1 .821–2
500 .8133+1 1.961 –.535+0 –.699–3 .2916+2 1.975 .378+0 –.258–3 .5408+2 1.307 –.204+0 .622–2 .1109+3 1.343 –.218+0 .984–2 .5486+2 1.980 .308+0 –.977–4 .8865+2 1.496 .659–1 .695–2 .1894+3 1.505 .490–1 .640–2 .3783+3 1.110 .251–1 .311–1 .5617+3 1.122 .307–1 .304–1
1000 .7719+1 1.956 –.192+0 –.693–3 .2385+2 1.982 .944–1 –.309–3 .3901+2 1.393 .313–1 .210–1 .7842+2 1.444 .258–1 .247–1 .3130+2 1.983 .909–1 –.153–3 .4664+2 1.598 –.187–1 .160–2 .9517+2 1.626 –.241–1 .362–2 .1075+3 1.225 .237+0 .526–1 .1575+3 1.216 .243+0 .525–1
E (eV) 1500 .7338+1 1.952 .465–1 –.682–3 .1982+2 1.987 –.275–1 –.329–3 .2905+2 1.415 .230+0 .301–1 .5741+2 1.473 .235+0 .329–1 .2012+2 1.987 –.236–1 –.178–3 .2750+2 1.604 .512–1 .332–2 .5456+2 1.642 .539–1 .618–2 .4244+2 1.205 .422+0 .694–1 .6168+2 1.186 .427+0 .703–1
2000 .6986+1 1.947 .236+0 –.670–3 .1670+2 1.990 –.730–1 –.338–3 .2219+2 1.413 .399+0 .373–1 .4323+2 1.477 .413+0 .391–1 .1396+2 1.989 –.783–1 –.194–3 .1759+2 1.585 .164+0 .640–2 .3420+2 1.630 .173+0 .933–2 .2018+2 1.154 .576+0 .859–1 .2914+2 1.129 .577+0 .880–1
3000 .6347+1 1.938 .536+0 –.651–3 .1225+2 1.994 –.527–1 –.344–3 .1373+2 1.385 .670+0 .496–1 .2612+2 1.453 .700+0 .492–1 .7781+1 1.993 –.858–1 –.212–3 .8456+1 1.524 .402+0 .145–1 .1599+2 1.577 .424+0 .165–1 .6329+1 1.037 .806+0 .119+0 .9057+1 1.011 .801+0 .123+0
4000 .5783+1 1.928 .775+0 –.633–3 .9302+1 1.994 .366–1 –.343–3 .9032+1 1.342 .884+0 .615–1 .1686+2 1.413 .927+0 .591–1 .4902+1 1.994 –.215–1 –.223–3 .4687+1 1.457 .618+0 .244–1 .8687+1 1.515 .651+0 .251–1 .2586+1 0.930 .970+0 .153+0 .3674+1 0.905 .962+0 .159+0
5000 .5283+1 1.919 .974+0 –.616–3 .7256+1 1.993 .154+0 –.338–3 .6227+1 1.296 .106+1 .735–1 .1145+2 1.368 .111+1 .693–1 .3340+1 1.994 .772–1 –.230–3 .2854+1 1.393 .804+0 .356–1 .5209+1 1.454 .847+0 .349–1 .1241+1 0.837 .109+1 .187+0 .1753+1 0.817 .108+1 .193+0
Pd, Z = 46 Shell 1s1/2 Eb = 24357 eV 2s1/2 Eb = 3611 eV 2 p1/2 Eb = 3337 eV 2 p3/2 Eb = 3180 eV 3s1/2 Eb = 677 eV 3 p1/2 Eb = 565 eV 3 p3/2 Eb = 537 eV 3d3/2 Eb = 347 eV 3d5/2 Eb = 342 eV
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M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Pd, Z = 46 (continued) Shell 4s1/2 Eb = 93 eV 4 p1/2 Eb = 63 eV 4 p3/2 Eb = 57 eV 4d3/2 Eb = 9 eV 4d5/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1631+3 1.979 .258+0 .901–4 .1286+3 0.443 –.325–1 .327–1 .3206+3 0.473 –.235–1 .305–1 .1252+3 −.811 .134+0 –.800–2 .1946+3 −.749 .149+0 –.137–1
200 .1003+3 1.983 .298+0 .290–4 .9658+2 1.139 .183+0 .205–1 .2236+3 1.125 .167+0 .195–1 .2423+3 0.579 .230–1 –.906–2 .3630+3 0.642 .205–1 –.892–2
500 .3693+2 1.984 .236+0 –.454–4 .4200+2 1.591 .102+0 .117–2 .8872+2 1.581 .851–1 .115–2 .8314+2 1.223 –.513–2 .130–1 .1211+3 1.242 –.202–2 .129–1
1000 .1365+2 1.986 .834–1 –.102–3 .1571+2 1.681 –.215–1 –.654–3 .3141+2 1.696 –.266–1 .907–3 .1860+2 1.320 .173+0 .346–1 .2667+2 1.310 .180+0 .346–1
E (eV) 1500 .7113+1 1.988 –.177–1 –.134–3 .7825+1 1.669 .214–1 .391–3 .1519+2 1.698 .240–1 .292–2 .6496+1 1.273 .357+0 .516–1 .9234+1 1.250 .362+0 .524–1
2000 .4365+1 1.990 –.719–1 –.155–3 .4527+1 1.637 .120+0 .243–2 .8623+1 1.675 .130+0 .527–2 .2869+1 1.203 .515+0 .682–1 .4054+1 1.176 .517+0 .701–1
3000 .2113+1 1.993 –.868–1 –.182–3 .1938+1 1.560 .352+0 .899–2 .3595+1 1.610 .373+0 .113–1 .8236+0 1.067 .761+0 .103+0 .1153+1 1.037 .757+0 .107+0
4000 .1229+1 1.994 –.286–1 –.199–3 .1004+1 1.485 .570+0 .182–1 .1829+1 1.540 .601+0 .194–1 .3191+0 0.948 .935+0 .138+0 .4438+0 0.921 .926+0 .144+0
5000 .7946+0 1.994 .661–1 –.209–3 .5852+0 1.415 .759+0 .292–1 .1050+1 1.473 .799+0 .290–1 .1481+0 0.850 .106+1 .173+0 .2049+0 0.828 .105+1 .180+0
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .8009+1 1.963 –.109+1 –.709–3 .3263+2 1.967 .979+0 –.108–3 .6703+2 0.979 –.342+0 –.204–1 .1405+3 0.979 –.349+0 –.213–1 .9365+2 1.976 .655+0 .590–4
200 .7959+1 1.962 –.907+0 –.751–3 .3139+2 1.969 .768+0 –.186–3 .6284+2 1.129 –.348+0 –.131–1 .1310+3 1.144 –.362+0 –.116–1 .8047+2 1.977 .547+0 –.917–5
500 .7743+1 1.959 –.563+0 –.778–3 .2783+2 1.974 .400+0 –.284–3 .5158+2 1.301 –.219+0 .533–2 .1060+3 1.338 –.235+0 .924–2 .5366+2 1.979 .325+0 –.105–3
1000 .7367+1 1.954 –.217+0 –.770–3 .2297+2 1.981 .110+0 –.342–3 .3778+2 1.389 .143–1 .204–1 .7606+2 1.441 .754–2 .245–1 .3123+2 1.982 .105+0 –.168–3
E (eV) 1500 .7017+1 1.950 .223–1 –.759–3 .1923+2 1.986 –.182–1 –.365–3 .2848+2 1.412 .213+0 .297–1 .5635+2 1.473 .217+0 .328–1 .2032+2 1.985 –.141–1 –.197–3
2000 .6694+1 1.945 .213+0 –.747–3 .1631+2 1.989 –.703–1 –.376–3 .2198+2 1.413 .382+0 .369–1 .4286+2 1.478 .395+0 .390–1 .1422+2 1.988 –.741–1 –.215–3
3000 .6107+1 1.935 .513+0 –.724–3 .1209+2 1.993 –.612–1 –.383–3 .1383+2 1.387 .654+0 .491–1 .2632+2 1.458 .684+0 .490–1 .8013+1 1.992 –.918–1 –.236–3
4000 .5585+1 1.926 .751+0 –.704–3 .9261+1 1.994 .194–1 –.382–3 .9214+1 1.347 .869+0 .608–1 .1720+2 1.421 .912+0 .585–1 .5084+1 1.994 –.362–1 –.248–3
5000 .5121+1 1.917 .956+0 –.688–3 .7276+1 1.993 .131+0 –.380–3 .6419+1 1.302 .105+1 .724–1 .1179+2 1.378 .110+1 .683–1 .3482+1 1.994 .555–1 –.257–3
Ag, Z = 47 Shell 1s1/2 Eb = 25520 eV 2s1/2 Eb = 3812 eV 2 p1/2 Eb = 3530 eV 2 p3/2 Eb = 3357 eV 3s1/2 Eb = 724 eV
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Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Ag, Z = 47 (continued) Shell 3 p1/2 Eb = 608 eV 3 p3/2 Eb = 577 eV 3d3/2 Eb = 379 eV 3d5/2 Eb = 373 eV 4s1/2 Eb = 101 eV 4 p1/2 Eb = 69 eV 4 p3/2 Eb = 63 eV 4d3/2 Eb = 11 eV 4d5/2 Eb = 10 eV 5s1/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1537+3 0.884 .225+0 .101+0 .3552+3 0.863 .202+0 .933–1 .1505+4 0.459 –.455–1 –.755–3 .2289+4 0.487 –.459–1 –.164–2 .1621+3 1.977 .264+0 .101–3 .1311+3 0.447 –.341–1 .335–1 .3297+3 0.476 –.248–1 .314–1 .1455+3 −.816 .109+0 .394–2 .2278+3 −.750 .128+0 –.270–2 .2965+2 1.974 .169+0 .947–4
200 .1329+3 1.190 .277+0 .489–1 .2998+3 1.178 .248+0 .441–1 .1013+4 0.730 –.636–1 .763–2 .1528+4 0.762 –.628–1 .688–2 .1016+3 1.981 .303+0 .342–4 .9917+2 1.131 .182+0 .218–1 .2316+3 1.117 .166+0 .207–1 .2738+3 0.550 .323–1 –.851–2 .4130+3 0.618 .296–1 –.851–2 .1284+2 1.981 .255+0 .447–4
500 .8686+2 1.487 .768–1 .803–2 .1866+3 1.496 .580–1 .731–2 .3802+3 1.100 .145–1 .303–1 .5652+3 1.113 .203–1 .295–1 .3849+2 1.983 .246+0 –.476–4 .4417+2 1.583 .114+0 .162–2 .9390+2 1.573 .956–1 .155–2 .9830+2 1.215 –.120–1 .115–1 .1440+3 1.236 –.917–2 .115–1 .3560+1 1.984 .239+0 –.352–4
1000 .4684+2 1.595 –.201–1 .162–2 .9599+2 1.623 –.267–1 .366–2 .1125+3 1.224 .223+0 .517–1 .1650+3 1.216 .230+0 .516–1 .1446+2 1.985 .949–1 –.111–3 .1685+2 1.682 –.199–1 –.727–3 .3381+2 1.695 –.262–1 .820–3 .2274+2 1.325 .157+0 .329–1 .3277+2 1.316 .164+0 .328–1 .1151+1 1.985 .981–1 –.103–3
148
E (eV) 1500 .2808+2 1.605 .405–1 .299–2 .5588+2 1.644 .423–1 .600–2 .4547+2 1.211 .410+0 .685–1 .6608+2 1.192 .415+0 .694–1 .7575+1 1.986 –.872–2 –.148–3 .8472+1 1.673 .122–1 .979–4 .1650+2 1.702 .140–1 .272–2 .8066+1 1.283 .341+0 .498–1 .1152+2 1.261 .346+0 .505–1 .5679+0 1.986 –.558–2 –.140–3
2000 .1817+2 1.588 .147+0 .582–2 .3542+2 1.635 .157+0 .898–2 .2196+2 1.164 .565+0 .845–1 .3171+2 1.139 .567+0 .865–1 .4664+1 1.989 –.671–1 –.172–3 .4937+1 1.643 .104+0 .189–2 .9423+1 1.682 .113+0 .491–2 .3604+1 1.217 .500+0 .660–1 .5116+1 1.189 .503+0 .678–1 .3382+0 1.988 –.652–1 –.163–3
3000 .8883+1 1.531 .381+0 .135–1 .1682+2 1.587 .403+0 .158–1 .7027+1 1.053 .800+0 .117+0 .1005+2 1.025 .796+0 .121+0 .2270+1 1.992 –.918–1 –.202–3 .2138+1 1.570 .328+0 .791–2 .3969+1 1.621 .349+0 .105–1 .1051+1 1.085 .750+0 .995–1 .1479+1 1.054 .747+0 .103+0 .1593+0 1.992 –.929–1 –.196–3
4000 .4980+1 1.468 .595+0 .230–1 .9233+1 1.528 .629+0 .240–1 .2908+1 0.948 .969+0 .150+0 .4128+1 0.922 .960+0 .156+0 .1325+1 1.994 –.428–1 –.220–3 .1117+1 1.498 .544+0 .166–1 .2034+1 1.554 .576+0 .181–1 .4115+0 0.969 .930+0 .134+0 .5747+0 0.940 .922+0 .140+0 .9140–1 1.994 –.456–1 –.217–3
5000 .3058+1 1.405 .783+0 .336–1 .5580+1 1.468 .826+0 .332–1 .1409+1 0.854 .109+1 .182+0 .1989+1 0.833 .108+1 .189+0 .8589+0 1.994 .447–1 –.233–3 .6549+0 1.428 .735+0 .270–1 .1175+1 1.489 .776+0 .271–1 .1924+0 0.870 .106+1 .168+0 .2671+0 0.845 .105+1 .175+0 .5864–1 1.994 .411–1 –.229–3
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Cd, Z = 48 Shell 1s1/2 Eb = 26715 eV 2s1/2 Eb = 4022 eV 2 p1/2 Eb = 3732 eV 2 p3/2 Eb = 3542 eV 3s1/2 Eb = 775 eV 3 p1/2 Eb = 655 eV 3 p3/2 Eb = 621 eV 3d3/2 Eb = 415 eV 3d5/2 Eb = 408 eV 4s1/2 Eb = 112 eV 4 p1/2 Eb = 78 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .7615+1 1.961 –.112+1 –.787–3 .3089+2 1.965 .999+0 –.119–3 .6304+2 0.977 –.356+0 –.223–1 .1323+3 0.976 –.363+0 –.233–1 .8890+2 1.975 .676+0 .661–4 .1462+3 0.882 .228+0 .104+0 .3394+3 0.860 .205+0 .965–1 .1415+4 0.457 –.479–1 –.162–2 .2154+4 0.487 –.484–1 –.251–2 .1594+3 1.975 .274+0 .114–3 .1321+3 0.453 –.345–1 .351–1
200 .7569+1 1.960 –.935+0 –.833–3 .2977+2 1.967 .789+0 –.204–3 .5929+2 1.124 –.362+0 –.146–1 .1237+3 1.140 –.377+0 –.129–1 .7699+2 1.975 .567+0 –.782–5 .1272+3 1.182 .285+0 .520–1 .2885+3 1.170 .254+0 .469–1 .9667+3 0.719 –.688–1 .630–2 .1460+4 0.753 –.681–1 .555–2 .1020+3 1.979 .311+0 .406–4 .1009+3 1.121 .183+0 .233–1
500 .7375+1 1.957 –.590+0 –.864–3 .2655+2 1.972 .421+0 –.312–3 .4917+2 1.295 –.235+0 .439–2 .1012+3 1.333 –.253+0 .860–2 .5231+2 1.977 .343+0 –.113–3 .8479+2 1.479 .879–1 .919–2 .1831+3 1.488 .670–1 .828–2 .3793+3 1.089 .411–2 .295–1 .5642+3 1.104 .102–1 .287–1 .3983+2 1.982 .256+0 –.501–4 .4613+2 1.576 .126+0 .212–2
1000 .7035+1 1.952 –.242+0 –.852–3 .2211+2 1.979 .126+0 –.376–3 .3654+2 1.384 –.237–2 .198–1 .7368+2 1.439 –.106–1 .242–1 .3106+2 1.981 .119+0 –.183–3 .4685+2 1.592 –.204–1 .168–2 .9642+2 1.620 –.285–1 .373–2 .1169+3 1.222 .210+0 .512–1 .1715+3 1.215 .218+0 .509–1 .1524+2 1.983 .106+0 –.121–3 .1798+2 1.681 –.171–1 –.768–3
149
E (eV) 1500 .6714+1 1.948 –.192–2 –.840–3 .1864+2 1.984 –.810–2 –.403–3 .2786+2 1.410 .195+0 .292–1 .5521+2 1.472 .198+0 .327–1 .2046+2 1.984 –.388–2 –.217–3 .2854+2 1.605 .308–1 .271–2 .5700+2 1.645 .316–1 .586–2 .4836+2 1.216 .399+0 .680–1 .7029+2 1.197 .405+0 .688–1 .8040+1 1.985 .625–3 –.161–3 .9135+1 1.676 .417–2 –.158–3
2000 .6417+1 1.943 .189+0 –.830–3 .1591+2 1.988 –.665–1 –.417–3 .2172+2 1.412 .365+0 .366–1 .4240+2 1.480 .378+0 .390–1 .1444+2 1.987 –.690–1 –.238–3 .1869+2 1.591 .132+0 .531–2 .3653+2 1.639 .141+0 .871–2 .2373+2 1.173 .555+0 .835–1 .3425+2 1.148 .558+0 .854–1 .4969+1 1.987 –.617–1 –.189–3 .5364+1 1.649 .891–1 .142–2
3000 .5876+1 1.933 .491+0 –.805–3 .1192+2 1.992 –.683–1 –.426–3 .1389+2 1.389 .638+0 .487–1 .2646+2 1.463 .668+0 .488–1 .8227+1 1.991 –.967–1 –.262–3 .9292+1 1.538 .360+0 .125–1 .1761+2 1.595 .382+0 .152–1 .7749+1 1.067 .794+0 .115+0 .1108+2 1.038 .791+0 .119+0 .2431+1 1.991 –.956–1 –.223–3 .2349+1 1.580 .306+0 .693–2
4000 .5394+1 1.924 .729+0 –.784–3 .9204+1 1.993 .363–2 –.426–3 .9372+1 1.352 .855+0 .601–1 .1750+2 1.429 .899+0 .580–1 .5258+1 1.993 –.496–1 –.276–3 .5269+1 1.478 .573+0 .216–1 .9774+1 1.540 .607+0 .229–1 .3249+1 0.965 .967+0 .147+0 .4608+1 0.937 .959+0 .153+0 .1425+1 1.993 –.556–1 –.244–3 .1238+1 1.510 .520+0 .150–1
5000 .4963+1 1.915 .935+0 –.766–3 .7280+1 1.993 .109+0 –.424–3 .6594+1 1.309 .103+1 .714–1 .1211+2 1.387 .109+1 .674–1 .3620+1 1.993 .349–1 –.287–3 .3263+1 1.416 .762+0 .318–1 .5953+1 1.482 .806+0 .317–1 .1590+1 0.872 .110+1 .179+0 .2241+1 0.848 .108+1 .186+0 .9264+0 1.993 .244–1 –.259–3 .7302+0 1.442 .711+0 .249–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Cd, Z = 48 (continued) Shell 4 p3/2 Eb = 71 eV 4d3/2 Eb = 14 eV 4d5/2 Eb = 13 eV 5s1/2 Eb = 9 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3372+3 0.481 –.249–1 .328–1 .1687+3 −.814 .818–1 .167–1 .2650+3 −.743 .104+0 .919–2 .3802+2 1.972 .175+0 .104–3
200 .2386+3 1.106 .166+0 .221–1 .3026+3 0.524 .417–1 –.744–2 .4585+3 0.596 .390–1 –.765–2 .1639+2 1.979 .252+0 .536–4
500 .9889+2 1.564 .106+0 .198–2 .1131+3 1.205 –.175–1 .101–1 .1662+3 1.229 –.151–1 .101–1 .4595+1 1.982 .245+0 –.343–4
1000 .3627+2 1.695 –.248–1 .756–3 .2704+2 1.329 .142+0 .314–1 .3908+2 1.321 .149+0 .312–1 .1499+1 1.984 .109+0 –.109–3
E (eV) 1500 .1786+2 1.705 .500–2 .254–2 .9749+1 1.294 .325+0 .482–1 .1396+2 1.271 .332+0 .488–1 .7418+0 1.985 .380–2 –.152–3
2000 .1027+2 1.688 .971–1 .462–2 .4405+1 1.231 .484+0 .640–1 .6268+1 1.202 .488+0 .657–1 .4428+0 1.987 –.597–1 –.181–3
3000 .4369+1 1.631 .327+0 .985–2 .1306+1 1.103 .738+0 .963–1 .1840+1 1.070 .735+0 .100+0 .2089+0 1.991 –.956–1 –.216–3
4000 .2256+1 1.568 .551+0 .169–1 .5164+0 0.989 .924+0 .130+0 .7224+0 0.957 .916+0 .136+0 .1202+0 1.993 –.577–1 –.239–3
5000 .1310+1 1.504 .753+0 .254–1 .2432+0 0.889 .106+1 .163+0 .3381+0 0.862 .105+1 .170+0 .7724–1 1.993 .212–1 –.254–3
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .7247+1 1.959 –.115+1 –.874–3 .2924+2 1.964 .102+1 –.132–3 .5930+2 0.976 –.371+0 –.241–1 .1246+3 0.975 –.379+0 –.251–1 .8421+2 1.973 .696+0 .726–4 .1385+3 0.884 .235+0 .107+0
200 .7203+1 1.957 –.963+0 –.928–3 .2822+2 1.965 .808+0 –.225–3 .5593+2 1.119 –.376+0 –.157–1 .1169+3 1.135 –.392+0 –.139–1 .7345+2 1.973 .585+0 –.638–5 .1213+3 1.173 .291+0 .544–1
500 .7029+1 1.955 –.615+0 –.958–3 .2532+2 1.970 .441+0 –.344–3 .4683+2 1.290 –.250+0 .353–2 .9649+2 1.329 –.269+0 .807–2 .5083+2 1.975 .359+0 –.122–3 .8238+2 1.472 .980–1 .103–1
1000 .6720+1 1.950 –.266+0 –.947–3 .2125+2 1.977 .142+0 –.416–3 .3528+2 1.380 –.182–1 .194–1 .7124+2 1.436 –.279–1 .241–1 .3078+2 1.979 .134+0 –.201–3 .4662+2 1.588 –.200–1 .179–2
E (eV) 1500 .6426+1 1.945 –.253–1 –.933–3 .1805+2 1.983 .224–2 –.446–3 .2721+2 1.407 .179+0 .289–1 .5398+2 1.471 .180+0 .327–1 .2052+2 1.982 .641–2 –.239–3 .2887+2 1.605 .224–1 .247–2
2000 .6153+1 1.941 .166+0 –.921–3 .1549+2 1.987 –.619–1 –.462–3 .2141+2 1.411 .348+0 .363–1 .4184+2 1.481 .360+0 .390–1 .1461+2 1.985 –.632–1 –.263–3 .1914+2 1.594 .118+0 .485–2
3000 .5654+1 1.931 .468+0 –.893–3 .1172+2 1.991 –.742–1 –.473–3 .1391+2 1.391 .622+0 .483–1 .2651+2 1.467 .652+0 .487–1 .8420+1 1.990 –.100+0 –.290–3 .9674+1 1.545 .340+0 .117–1
4000 .5208+1 1.922 .708+0 –.870–3 .9128+1 1.993 –.108–1 –.474–3 .9501+1 1.356 .840+0 .596–1 .1774+2 1.436 .885+0 .577–1 .5422+1 1.992 –.617–1 –.307–3 .5549+1 1.487 .552+0 .203–1
5000 .4807+1 1.912 .914+0 –.852–3 .7269+1 1.992 .875–1 –.474–3 .6752+1 1.315 .102+1 .706–1 .1240+2 1.396 .108+1 .666–1 .3752+1 1.993 .158–1 –.319–3 .3466+1 1.428 .741+0 .301–1
In, Z = 49 Shell 1s1/2 Eb = 27944 eV 2s1/2 Eb = 4242 eV 2 p1/2 Eb = 3943 eV 2 p3/2 Eb = 3735 eV 3s1/2 Eb = 830 eV 3 p1/2 Eb = 707 eV
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M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables In, Z = 49 (continued) Shell 3 p3/2 Eb = 669 eV 3d3/2 Eb = 455 eV 3d5/2 Eb = 447 eV 4s1/2 Eb = 126 eV 4 p1/2 Eb = 90 eV 4 p3/2 Eb = 82 eV 4d3/2 Eb = 21 eV 4d5/2 Eb = 20 eV 5s1/2 Eb = 10 eV 5 p1/2 Eb = 5 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3232+3 0.861 .209+0 .987–1 .1316+4 0.459 –.511–1 –.256–2 .2005+4 0.490 –.517–1 –.344–2 .1550+3 1.973 .288+0 .127–3 .1322+3 0.474 –.300–1 .374–1 .3414+3 0.499 –.203–1 .349–1 .1995+3 −.779 .610–1 .285–1 .3143+3 −.695 .852–1 .206–1 .4922+2 1.969 .177+0 .112–3 .1459+2 0.093 –.475–1 .169–1
200 .2766+3 1.161 .258+0 .489–1 .9155+3 0.714 –.740–1 .507–2 .1384+4 0.749 –.734–1 .433–2 .1013+3 1.978 .321+0 .475–4 .1018+3 1.112 .185+0 .245–1 .2433+3 1.096 .168+0 .231–1 .3277+3 0.514 .502–1 –.591–2 .4980+3 0.590 .476–1 –.634–2 .2167+2 1.977 .251+0 .615–4 .8057+1 0.973 .129+0 .193–1
500 .1789+3 1.480 .751–1 .924–2 .3749+3 1.079 –.574–2 .287–1 .5581+3 1.096 .583–3 .278–1 .4087+2 1.980 .266+0 –.530–4 .4776+2 1.569 .138+0 .261–2 .1032+3 1.556 .115+0 .240–2 .1269+3 1.196 –.216–1 .889–2 .1870+3 1.222 –.195–1 .893–2 .6080+1 1.981 .250+0 –.318–4 .3105+1 1.580 .152+0 .119–2
1000 .9640+2 1.617 –.296–1 .387–2 .1205+3 1.220 .198+0 .507–1 .1767+3 1.213 .206+0 .502–1 .1596+2 1.982 .118+0 –.131–3 .1905+2 1.680 –.137–1 –.795–3 .3865+2 1.693 –.228–1 .715–3 .3149+2 1.332 .128+0 .300–1 .4562+2 1.325 .136+0 .298–1 .1996+1 1.982 .119+0 –.117–3 .1116+1 1.698 –.108–1 –.118–2
151
E (eV) 1500 .5787+2 1.646 .222–1 .578–2 .5101+2 1.220 .388+0 .674–1 .7414+2 1.201 .394+0 .681–1 .8492+1 1.984 .994–2 –.176–3 .9792+1 1.679 –.246–2 –.383–3 .1923+2 1.708 –.264–2 .240–2 .1156+2 1.303 .310+0 .466–1 .1658+2 1.281 .317+0 .471–1 .9895+0 1.984 .130–1 –.166–3 .5475+0 1.693 –.773–2 –.773–3
2000 .3751+2 1.642 .126+0 .848–2 .2543+2 1.181 .546+0 .827–1 .3671+2 1.156 .549+0 .845–1 .5272+1 1.986 –.557–1 –.207–3 .5794+1 1.654 .753–1 .996–3 .1113+2 1.694 .826–1 .436–2 .5285+1 1.244 .470+0 .621–1 .7532+1 1.214 .475+0 .637–1 .5910+0 1.986 –.535–1 –.197–3 .3156+0 1.666 .669–1 .448–3
3000 .1837+2 1.603 .362+0 .147–1 .8484+1 1.081 .789+0 .113+0 .1212+2 1.050 .786+0 .117+0 .2594+1 1.990 –.981–1 –.246–3 .2567+1 1.589 .284+0 .605–2 .4784+1 1.641 .305+0 .926–2 .1593+1 1.120 .727+0 .936–1 .2248+1 1.085 .725+0 .975–1 .2794+0 1.990 –.980–1 –.238–3 .1361+0 1.596 .275+0 .526–2
4000 .1030+2 1.551 .586+0 .220–1 .3604+1 0.981 .966+0 .145+0 .5107+1 0.951 .957+0 .151+0 .1527+1 1.992 –.669–1 –.270–3 .1364+1 1.521 .496+0 .136–1 .2490+1 1.581 .528+0 .158–1 .6368+0 1.007 .918+0 .126+0 .8919+0 0.974 .910+0 .132+0 .1611+0 1.992 –.687–1 –.264–3 .7128–1 1.526 .487+0 .126–1
5000 .6324+1 1.495 .786+0 .303–1 .1781+1 0.890 .110+1 .175+0 .2507+1 0.864 .109+1 .182+0 .9958+0 1.993 .557–2 –.287–3 .8102+0 1.455 .687+0 .229–1 .1455+1 1.519 .730+0 .238–1 .3021+0 0.908 .106+1 .158+0 .4205+0 0.878 .105+1 .165+0 .1037+0 1.993 .262–2 –.281–3 .4194–1 1.461 .679+0 .220–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Sn, Z = 50 Shell 1s1/2 Eb = 29204 eV 2s1/2 Eb = 4469 eV 2 p1/2 Eb = 4160 eV 2 p3/2 Eb = 3933 eV 3s1/2 Eb = 888 eV 3 p1/2 Eb = 761 eV 3 p3/2 Eb = 719 eV 3d3/2 Eb = 498 eV 3d5/2 Eb = 489 eV 4s1/2 Eb = 141 eV 4 p1/2 Eb = 102 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .6905+1 1.956 –.118+1 –.969–3 .2771+2 1.962 .104+1 –.146–3 .5589+2 0.973 –.385+0 –.259–1 .1176+3 0.973 –.394+0 –.269–1 .7977+2 1.971 .719+0 .806–4 .1314+3 0.883 .239+0 .110+0 .3080+3 0.859 .211+0 .101+0 .1221+4 0.460 –.545–1 –.359–2 .1861+4 0.492 –.551–1 –.447–2 .1505+3 1.971 .302+0 .142–3 .1324+3 0.487 –.261–1 .398–1
200 .6862+1 1.955 –.989+0 –.102–2 .2678+2 1.964 .827+0 –.248–3 .5284+2 1.116 –.390+0 –.172–1 .1106+3 1.133 –.408+0 –.153–1 .7004+2 1.972 .604+0 –.562–5 .1157+3 1.169 .298+0 .573–1 .2652+3 1.155 .263+0 .514–1 .8656+3 0.706 –.796–1 .374–2 .1309+4 0.743 –.792–1 .300–2 .1004+3 1.976 .331+0 .548–4 .1027+3 1.107 .188+0 .260–1
500 .6704+1 1.952 –.641+0 –.106–2 .2415+2 1.969 .461+0 –.377–3 .4462+2 1.285 –.265+0 .255–2 .9209+2 1.325 –.286+0 .743–2 .4930+2 1.974 .377+0 –.132–3 .7997+2 1.464 .109+0 .116–1 .1746+3 1.472 .836–1 .103–1 .3691+3 1.069 –.156–1 .280–1 .5499+3 1.088 –.906–2 .270–1 .4181+2 1.979 .276+0 –.559–4 .4935+2 1.562 .149+0 .319–2
1000 .6423+1 1.948 –.290+0 –.105–2 .2043+2 1.976 .159+0 –.457–3 .3407+2 1.376 –.342–1 .188–1 .6888+2 1.433 –.455–1 .240–1 .3043+2 1.977 .148+0 –.219–3 .4631+2 1.585 –.188–1 .195–2 .9621+2 1.613 –.300–1 .403–2 .1235+3 1.217 .186+0 .502–1 .1813+3 1.212 .195+0 .497–1 .1667+2 1.981 .129+0 –.142–3 .2012+2 1.679 –.924–2 –.791–3
152
E (eV) 1500 .6154+1 1.943 –.490–1 –.103–2 .1747+2 1.981 .133–1 –.492–3 .2655+2 1.404 .162+0 .285–1 .5275+2 1.470 .162+0 .328–1 .2055+2 1.981 .173–1 –.263–3 .2914+2 1.605 .149–1 .227–2 .5863+2 1.646 .134–1 .572–2 .5354+2 1.223 .376+0 .669–1 .7781+2 1.204 .384+0 .674–1 .8948+1 1.983 .197–1 –.193–3 .1047+2 1.682 –.810–2 –.583–3
2000 .5902+1 1.938 .143+0 –.102–2 .1508+2 1.985 –.565–1 –.511–3 .2108+2 1.409 .332+0 .359–1 .4125+2 1.482 .343+0 .390–1 .1475+2 1.984 –.567–1 –.290–3 .1954+2 1.596 .104+0 .442–2 .3841+2 1.646 .111+0 .829–2 .2713+2 1.189 .535+0 .818–1 .3914+2 1.163 .540+0 .835–1 .5581+1 1.985 –.493–1 –.227–3 .6240+1 1.659 .625–1 .600–3
3000 .5441+1 1.929 .445+0 –.989–3 .1152+2 1.990 –.789–1 –.523–3 .1390+2 1.392 .606+0 .480–1 .2652+2 1.471 .636+0 .487–1 .8599+1 1.989 –.103+0 –.321–3 .1004+2 1.551 .321+0 .109–1 .1910+2 1.611 .342+0 .142–1 .9239+1 1.093 .783+0 .112+0 .1319+2 1.062 .780+0 .116+0 .2762+1 1.989 –.996–1 –.270–3 .2796+1 1.597 .264+0 .524–2
4000 .5028+1 1.920 .687+0 –.965–3 .9041+1 1.992 –.240–1 –.527–3 .9612+1 1.359 .827+0 .592–1 .1796+2 1.442 .873+0 .575–1 .5578+1 1.991 –.727–1 –.341–3 .5827+1 1.495 .532+0 .192–1 .1083+2 1.561 .566+0 .213–1 .3977+1 0.995 .963+0 .142+0 .5631+1 0.964 .954+0 .148+0 .1632+1 1.991 –.770–1 –.298–3 .1499+1 1.531 .473+0 .124–1
5000 .4655+1 1.910 .893+0 –.945–3 .7247+1 1.992 .676–1 –.527–3 .6897+1 1.320 .101+1 .697–1 .1266+2 1.405 .107+1 .659–1 .3881+1 1.992 –.210–2 –.354–3 .3670+1 1.438 .719+0 .285–1 .6697+1 1.508 .765+0 .290–1 .1984+1 0.907 .110+1 .172+0 .2791+1 0.878 .109+1 .179+0 .1068+1 1.992 –.119–1 –.318–3 .8955+0 1.467 .663+0 .211–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Sn, Z = 50 (continued) Shell 4 p3/2 Eb = 93 eV 4d3/2 Eb = 29 eV 4d5/2 Eb = 28 eV 5s1/2 Eb = 12 eV 5 p1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3460+3 0.510 –.166–1 .370–1 .2286+3 −.744 .420–1 .403–1 .3606+3 −.652 .682–1 .319–1 .5767+2 1.966 .179+0 .123–3 .2072+2 0.102 –.473–1 .178–1
200 .2482+3 1.090 .170+0 .245–1 .3491+3 0.496 .588–1 –.390–2 .5318+3 0.576 .564–1 –.460–2 .2586+2 1.975 .254+0 .675–4 .1153+2 0.968 .127+0 .198–1
500 .1076+3 1.548 .125+0 .291–2 .1400+3 1.185 –.250–1 .779–2 .2068+3 1.214 –.233–1 .786–2 .7314+1 1.979 .258+0 –.325–4 .4439+1 1.573 .163+0 .153–2
1000 .4108+2 1.691 –.198–1 .691–3 .3604+2 1.334 .114+0 .287–1 .5229+2 1.328 .122+0 .284–1 .2413+1 1.981 .129+0 –.127–3 .1608+1 1.698 –.537–2 –.122–2
E (eV) 1500 .2064+2 1.710 –.938–2 .227–2 .1346+2 1.311 .294+0 .450–1 .1934+2 1.289 .303+0 .455–1 .1200+1 1.983 .226–1 –.180–3 .7950+0 1.697 –.127–1 –.952–3
2000 .1203+2 1.699 .690–1 .414–2 .6231+1 1.256 .455+0 .602–1 .8888+1 1.226 .461+0 .617–1 .7180+0 1.985 –.467–1 –.216–3 .4608+0 1.672 .542–1 .562–4
3000 .5222+1 1.651 .284+0 .876–2 .1908+1 1.136 .715+0 .910–1 .2695+1 1.100 .714+0 .949–1 .3400+0 1.989 –.990–1 –.261–3 .2002+0 1.606 .254+0 .442–2
4000 .2738+1 1.593 .505+0 .150–1 .7712+0 1.024 .910+0 .122+0 .1081+1 0.988 .902+0 .128+0 .1965+0 1.991 –.782–1 –.290–3 .1056+0 1.538 .462+0 .113–1
5000 .1609+1 1.533 .706+0 .223–1 .3687+0 0.927 .105+1 .154+0 .5133+0 0.895 .104+1 .161+0 .1268+0 1.992 –.147–1 –.310–3 .6250–1 1.474 .654+0 .201–1
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .6585+1 1.954 –.121+1 –.107–2 .2630+2 1.960 .105+1 –.160–3 .5273+2 0.971 –.399+0 –.277–1 .1111+3 0.970 –.409+0 –.287–1 .7556+2 1.969 .741+0 .898–4
200 .6541+1 1.953 –.102+1 –.113–2 .2544+2 1.962 .847+0 –.272–3 .4997+2 1.113 –.405+0 –.188–1 .1047+3 1.130 –.424+0 –.167–1 .6675+2 1.970 .624+0 –.460–5
500 .6398+1 1.950 –.666+0 –.117–2 .2304+2 1.967 .481+0 –.414–3 .4254+2 1.280 –.280+0 .158–2 .8791+2 1.321 –.303+0 .682–2 .4776+2 1.972 .394+0 –.142–3
1000 .6143+1 1.945 –.315+0 –.116–2 .1964+2 1.974 .176+0 –.503–3 .3288+2 1.371 –.502–1 .183–1 .6658+2 1.431 –.632–1 .239–1 .3003+2 1.976 .163+0 –.240–3
E (eV) 1500 .5895+1 1.941 –.727–1 –.114–2 .1690+2 1.979 .250–1 –.542–3 .2588+2 1.401 .145+0 .280–1 .5149+2 1.469 .144+0 .327–1 .2052+2 1.979 .287–1 –.288–3
2000 .5663+1 1.936 .119+0 –.113–2 .1467+2 1.984 –.500–1 –.563–3 .2073+2 1.408 .314+0 .355–1 .4062+2 1.482 .324+0 .391–1 .1486+2 1.982 –.494–1 –.318–3
3000 .5238+1 1.927 .422+0 –.109–2 .1131+2 1.989 –.827–1 –.579–3 .1387+2 1.393 .590+0 .476–1 .2648+2 1.475 .620+0 .486–1 .8762+1 1.987 –.104+0 –.354–3
4000 .4855+1 1.917 .666+0 –.107–2 .8944+1 1.991 –.361–1 –.585–3 .9702+1 1.362 .813+0 .587–1 .1813+2 1.448 .859+0 .573–1 .5727+1 1.990 –.826–1 –.377–3
5000 .4508+1 1.908 .871+0 –.105–2 .7215+1 1.991 .488–1 –.586–3 .7027+1 1.325 .995+0 .690–1 .1290+2 1.413 .105+1 .653–1 .4006+1 1.991 –.188–1 –.393–3
Sb, Z = 51 Shell 1s1/2 Eb = 30496 eV 2s1/2 Eb = 4703 eV 2 p1/2 Eb = 4385 eV 2 p3/2 Eb = 4137 eV 3s1/2 Eb = 949 eV
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M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Sb, Z = 51 (continued) Shell 3 p1/2 Eb = 817 eV 3 p3/2 Eb = 771 eV 3d3/2 Eb = 542 eV 3d5/2 Eb = 533 eV 4s1/2 Eb = 157 eV 4 p1/2 Eb = 114 eV 4 p3/2 Eb = 104 eV 4d3/2 Eb = 38 eV 4d5/2 Eb = 37 eV 5s1/2 Eb = 15 eV 5 p1/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1247+3 0.880 .242+0 .113+0 .2936+3 0.855 .213+0 .103+0 .1134+4 0.459 –.578–1 –.468–2 .1726+4 0.493 –.587–1 –.556–2 .1460+3 1.968 .317+0 .159–3 .1328+3 0.497 –.219–1 .422–1 .3508+3 0.517 –.126–1 .391–1 .2574+3 −.705 .257–1 .515–1 .4063+3 −.605 .534–1 .426–1 .6532+2 1.963 .182+0 .137–3 .2709+2 0.105 –.472–1 .186–1
200 .1104+3 1.164 .304+0 .602–1 .2543+3 1.150 .268+0 .538–1 .8191+3 0.698 –.851–1 .234–2 .1238+4 0.737 –.850–1 .161–2 .9928+2 1.973 .342+0 .632–4 .1035+3 1.102 .191+0 .275–1 .2532+3 1.084 .171+0 .258–1 .3676+3 0.477 .670–1 –.142–2 .5612+3 0.561 .650–1 –.242–2 .2972+2 1.973 .258+0 .750–4 .1494+2 0.957 .125+0 .203–1
500 .7756+2 1.457 .119+0 .129–1 .1702+3 1.465 .918–1 .114–1 .3629+3 1.060 –.256–1 .271–1 .5403+3 1.080 –.188–1 .262–1 .4263+2 1.977 .287+0 –.588–4 .5086+2 1.555 .160+0 .377–2 .1119+3 1.539 .134+0 .341–2 .1524+3 1.174 –.274–1 .675–2 .2254+3 1.207 –.263–1 .686–2 .8514+1 1.978 .264+0 –.330–4 .5747+1 1.567 .173+0 .183–2
1000 .4592+2 1.580 –.169–1 .215–2 .9583+2 1.610 –.298–1 .423–2 .1263+3 1.214 .173+0 .498–1 .1852+3 1.209 .184+0 .492–1 .1736+2 1.979 .141+0 –.154–3 .2118+2 1.678 –.406–2 –.769–3 .4351+2 1.689 –.163–1 .682–3 .4067+2 1.335 .101+0 .275–1 .5907+2 1.331 .109+0 .271–1 .2829+1 1.979 .140+0 –.136–3 .2100+1 1.698 .870–3 –.125–2
154
E (eV) 1500 .2933+2 1.604 .814–2 .210–2 .5925+2 1.646 .539–2 .569–2 .5597+2 1.226 .363+0 .661–1 .8130+2 1.207 .372+0 .665–1 .9399+1 1.981 .297–1 –.210–3 .1115+2 1.684 –.127–1 –.755–3 .2209+2 1.712 –.152–1 .216–2 .1547+2 1.319 .278+0 .433–1 .2224+2 1.298 .287+0 .437–1 .1412+1 1.981 .325–1 –.195–3 .1046+1 1.700 –.168–1 –.113–2
2000 .1990+2 1.598 .914–1 .402–2 .3924+2 1.648 .973–1 .813–2 .2880+2 1.196 .525+0 .811–1 .4153+2 1.170 .531+0 .828–1 .5891+1 1.983 –.421–1 –.248–3 .6696+1 1.664 .505–1 .246–3 .1295+2 1.704 .560–1 .394–2 .7241+1 1.268 .441+0 .585–1 .1034+2 1.237 .447+0 .599–1 .8460+0 1.983 –.396–1 –.235–3 .6090+0 1.677 .424–1 –.297–3
3000 .1039+2 1.557 .302+0 .101–1 .1981+2 1.618 .323+0 .138–1 .1002+2 1.105 .776+0 .110+0 .1428+2 1.073 .775+0 .114+0 .2933+1 1.987 –.100+0 –.297–3 .3033+1 1.605 .243+0 .447–2 .5678+1 1.659 .263+0 .829–2 .2254+1 1.152 .703+0 .883–1 .3183+1 1.114 .703+0 .922–1 .4016+0 1.987 –.993–1 –.286–3 .2668+0 1.614 .233+0 .363–2
4000 .6099+1 1.503 .511+0 .181–1 .1134+2 1.572 .545+0 .205–1 .4369+1 1.010 .960+0 .140+0 .6178+1 0.977 .952+0 .146+0 .1740+1 1.990 –.858–1 –.328–3 .1639+1 1.541 .449+0 .111–1 .2999+1 1.604 .481+0 .141–1 .9207+0 1.042 .902+0 .119+0 .1290+1 1.004 .895+0 .125+0 .2325+0 1.990 –.866–1 –.319–3 .1416+0 1.549 .437+0 .997–2
5000 .3875+1 1.449 .698+0 .269–1 .7071+1 1.521 .744+0 .278–1 .2200+1 0.923 .110+1 .169+0 .3091+1 0.893 .109+1 .176+0 .1142+1 1.991 –.281–1 –.351–3 .9855+0 1.479 .639+0 .193–1 .1772+1 1.547 .682+0 .209–1 .4435+0 0.946 .105+1 .149+0 .6175+0 0.911 .104+1 .157+0 .1503+0 1.991 –.306–1 –.343–3 .8424–1 1.485 .629+0 .181–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Sb, Z = 51 (continued) Shell 5 p3/2 Eb = 8 eV
σ β γ δ
100 .6269+2 0.183 –.482–1 .191–1
200 .3384+2 0.970 .120+0 .206–1
500 .1178+2 1.545 .147+0 .201–2
1000 .4035+1 1.704 –.119–1 .891–4
E (eV) 1500 .1942+1 1.725 –.195–1 .167–2
2000 .1106+1 1.715 .479–1 .335–2
3000 .4697+0 1.667 .252+0 .747–2
4000 .2440+0 1.611 .470+0 .130–1
5000 .1427+0 1.553 .672+0 .199–1
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .6286+1 1.951 –.123+1 –.119–2 .2497+2 1.958 .108+1 –.175–3 .4978+2 0.967 –.414+0 –.295–1 .1050+3 0.966 –.424+0 –.305–1 .7166+2 1.966 .765+0 .100–3 .1182+3 0.877 .245+0 .115+0 .2799+3 0.851 .214+0 .106+0 .1051+4 0.458 –.611–1 –.581–2 .1602+4 0.493 –.621–1 –.669–2
200 .6241+1 1.950 –.104+1 –.125–2 .2417+2 1.960 .867+0 –.298–3 .4729+2 1.109 –.420+0 –.203–1 .9928+2 1.126 –.440+0 –.180–1 .6365+2 1.967 .645+0 –.266–5 .1053+3 1.156 .311+0 .630–1 .2439+3 1.142 .271+0 .563–1 .7740+3 0.690 –.907–1 .862–3 .1172+4 0.731 –.907–1 .138–3
500 .6110+1 1.947 –.692+0 –.129–2 .2200+2 1.965 .502+0 –.453–3 .4056+2 1.275 –.296+0 .583–3 .8396+2 1.317 –.320+0 .619–2 .4624+2 1.970 .412+0 –.153–3 .7512+2 1.449 .130+0 .143–1 .1658+3 1.457 .100+0 .125–1 .3555+3 1.050 –.357–1 .263–1 .5301+3 1.072 –.287–1 .252–1
1000 .5878+1 1.943 –.340+0 –.128–2 .1888+2 1.972 .193+0 –.553–3 .3172+2 1.367 –.663–1 .177–1 .6433+2 1.428 –.811–1 .238–1 .2960+2 1.974 .179+0 –.261–3 .4542+2 1.576 –.144–1 .239–2 .9528+2 1.606 –.291–1 .447–2 .1285+3 1.210 .161+0 .493–1 .1886+3 1.207 .172+0 .486–1
E (eV) 1500 .5651+1 1.938 –.967–1 –.126–2 .1634+2 1.978 .373–1 –.597–3 .2521+2 1.398 .129+0 .276–1 .5024+2 1.468 .126+0 .328–1 .2046+2 1.977 .406–1 –.315–3 .2946+2 1.603 .223–2 .196–2 .5975+2 1.645 –.189–2 .569–2 .5825+2 1.228 .350+0 .656–1 .8464+2 1.210 .360+0 .658–1
2000 .5437+1 1.933 .960–1 –.124–2 .1426+2 1.982 –.430–1 –.621–3 .2036+2 1.406 .298+0 .352–1 .3995+2 1.483 .306+0 .392–1 .1494+2 1.980 –.415–1 –.350–3 .2021+2 1.599 .794–1 .366–2 .3999+2 1.651 .843–1 .801–2 .3044+2 1.202 .514+0 .804–1 .4389+2 1.176 .521+0 .819–1
3000 .5043+1 1.924 .400+0 –.121–2 .1109+2 1.988 –.855–1 –.641–3 .1382+2 1.394 .575+0 .474–1 .2640+2 1.478 .604+0 .487–1 .8911+1 1.986 –.105+0 –.391–3 .1073+2 1.562 .284+0 .941–2 .2049+2 1.625 .304+0 .134–1 .1080+2 1.117 .769+0 .109+0 .1540+2 1.083 .768+0 .113+0
4000 .4688+1 1.915 .644+0 –.118–2 .8836+1 1.990 –.471–1 –.649–3 .9773+1 1.365 .797+0 .580–1 .1827+2 1.453 .843+0 .568–1 .5867+1 1.989 –.914–1 –.417–3 .6365+1 1.511 .489+0 .168–1 .1185+2 1.581 .524+0 .197–1 .4776+1 1.025 .956+0 .137+0 .6749+1 0.990 .949+0 .143+0
5000 .4365+1 1.906 .847+0 –.116–2 .7173+1 1.991 .310–1 –.647–3 .7144+1 1.331 .981+0 .685–1 .1311+2 1.421 .104+1 .649–1 .4127+1 1.991 –.343–1 –.433–3 .4078+1 1.459 .676+0 .256–1 .7446+1 1.533 .723+0 .269–1 .2428+1 0.940 .110+1 .166+0 .3408+1 0.907 .109+1 .174+0
Te, Z = 52 Shell 1s1/2 Eb = 31820 eV 2s1/2 Eb = 4945 eV 2 p1/2 Eb = 4618 eV 2 p3/2 Eb = 4347 eV 3s1/2 Eb = 1012 eV 3 p1/2 Eb = 876 eV 3 p3/2 Eb = 825 eV 3d3/2 Eb = 589 eV 3d5/2 Eb = 578 eV
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Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Te, Z = 52 (continued) Shell 4s1/2 Eb = 174 eV 4 p1/2 Eb = 127 eV 4 p3/2 Eb = 117 eV 4d3/2 Eb = 48 eV 4d5/2 Eb = 46 eV 5s1/2 Eb = 18 eV 5 p1/2 Eb = 9 eV 5 p3/2 Eb = 9 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1414+3 1.966 .333+0 .178–3 .1324+3 0.504 –.181–1 .448–1 .3519+3 0.522 –.919–2 .415–1 .2841+3 −.667 .110–1 .621–1 .4514+3 −.563 .399–1 .526–1 .7247+2 1.959 .186+0 .154–3 .3331+2 0.104 –.473–1 .193–1 .7845+2 0.184 –.478–1 .197–1
200 .9796+2 1.971 .354+0 .733–4 .1040+3 1.093 .193+0 .291–1 .2563+3 1.074 .173+0 .273–1 .3830+3 0.460 .753–1 .150–2 .5880+3 0.548 .736–1 .161–3 .3339+2 1.970 .261+0 .840–4 .1816+2 0.943 .122+0 .207–1 .4186+2 0.956 .117+0 .210–1
500 .4334+2 1.975 .298+0 –.617–4 .5221+2 1.548 .171+0 .439–2 .1157+3 1.530 .143+0 .396–2 .1640+3 1.163 –.291–1 .580–2 .2434+3 1.199 –.284–1 .593–2 .9694+1 1.976 .271+0 –.329–4 .6993+1 1.562 .183+0 .210–2 .1454+2 1.538 .155+0 .230–2
1000 .1801+2 1.977 .152+0 –.167–3 .2221+2 1.676 .188–2 –.727–3 .4586+2 1.686 –.121–1 .688–3 .4532+2 1.336 .876–1 .263–1 .6596+2 1.333 .966–1 .259–1 .3246+1 1.978 .150+0 –.146–3 .2580+1 1.698 .782–2 –.127–2 .5016+1 1.702 –.672–2 .290–4
E (eV) 1500 .9844+1 1.979 .402–1 –.228–3 .1182+2 1.685 –.163–1 –.905–3 .2353+2 1.713 –.201–1 .207–2 .1755+2 1.326 .262+0 .419–1 .2527+2 1.305 .272+0 .421–1 .1625+1 1.980 .426–1 –.211–3 .1293+1 1.703 –.198–1 –.129–2 .2427+1 1.728 –.238–1 .155–2
2000 .6202+1 1.982 –.345–1 –.271–3 .7157+1 1.668 .395–1 –.813–4 .1389+2 1.708 .441–1 .377–2 .8314+1 1.279 .426+0 .567–1 .1188+2 1.248 .433+0 .580–1 .9755+0 1.982 –.318–1 –.256–3 .7566+0 1.683 .314–1 –.626–3 .1388+1 1.720 .358–1 .315–2
3000 .3106+1 1.986 –.100+0 –.326–3 .3277+1 1.612 .224+0 .376–2 .6147+1 1.668 .243+0 .789–2 .2628+1 1.166 .691+0 .858–1 .3714+1 1.127 .691+0 .896–1 .4640+0 1.986 –.987–1 –.313–3 .3339+0 1.623 .213+0 .289–2 .5929+0 1.676 .232+0 .704–2
4000 .1851+1 1.989 –.935–1 –.362–3 .1785+1 1.551 .425+0 .985–2 .3270+1 1.615 .458+0 .132–1 .1085+1 1.059 .893+0 .115+0 .1521+1 1.019 .886+0 .121+0 .2691+0 1.989 –.940–1 –.350–3 .1784+0 1.559 .414+0 .881–2 .3096+0 1.622 .446+0 .122–1
5000 .1218+1 1.990 –.428–1 –.385–3 .1080+1 1.492 .614+0 .178–1 .1943+1 1.561 .658+0 .198–1 .5269+0 0.965 .105+1 .146+0 .7334+0 0.928 .104+1 .153+0 .1743+0 1.990 –.452–1 –.377–3 .1066+0 1.498 .603+0 .164–1 .1819+0 1.566 .647+0 .186–1
σ β γ δ σ β γ δ
100 .6006+1 1.949 –.126+1 –.131–2 .2373+2 1.956 .110+1 –.191–3
200 .5960+1 1.948 –.107+1 –.137–2 .2299+2 1.958 .889+0 –.326–3
500 .5839+1 1.945 –.717+0 –.141–2 .2101+2 1.963 .522+0 –.496–3
1000 .5627+1 1.940 –.365+0 –.141–2 .1815+2 1.970 .211+0 –.607–3
E (eV) 1500 .5419+1 1.936 –.121+0 –.139–2 .1580+2 1.976 .502–1 –.656–3
2000 .5221+1 1.931 .724–1 –.137–2 .1385+2 1.980 –.351–1 –.684–3
3000 .4857+1 1.922 .377+0 –.134–2 .1087+2 1.986 –.872–1 –.707–3
4000 .4527+1 1.912 .622+0 –.131–2 .8721+1 1.989 –.570–1 –.717–3
5000 .4227+1 1.903 .825+0 –.128–2 .7122+1 1.990 .145–1 –.716–3
I, Z = 53 Shell 1s1/2 Eb = 33176 eV 2s1/2 Eb = 5195 eV
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Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables I, Z = 53 (continued) Shell 2 p1/2 Eb = 4858 eV 2 p3/2 Eb = 4563 eV 3s1/2 Eb = 1078 eV 3 p1/2 Eb = 937 eV 3 p3/2 Eb = 881 eV 3d3/2 Eb = 638 eV 3d5/2 Eb = 626 eV 4s1/2 Eb = 193 eV 4 p1/2 Eb = 141 eV 4 p3/2 Eb = 131 eV 4d3/2 Eb = 58 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .4705+2 0.964 –.428+0 –.312–1 .9940+2 0.962 –.439+0 –.323–1 .6795+2 1.964 .789+0 .112–3 .1122+3 0.872 .246+0 .118+0 .2669+3 0.845 .213+0 .108+0 .9738+3 0.455 –.644–1 –.696–2 .1485+4 0.493 –.655–1 –.786–2 .1363+3 1.963 .351+0 .200–3 .1313+3 0.508 –.146–1 .475–1 .3514+3 0.523 –.607–2 .442–1 .3100+3 −.632 –.239–2 .718–1
200 .4482+2 1.105 –.435+0 –.220–1 .9422+2 1.122 –.457+0 –.195–1 .6069+2 1.965 .666+0 –.547–6 .1004+3 1.150 .317+0 .661–1 .2339+3 1.135 .275+0 .589–1 .7313+3 0.682 –.965–1 –.713–3 .1107+4 0.724 –.966–1 –.143–2 .9618+2 1.969 .368+0 .849–4 .1040+3 1.085 .196+0 .309–1 .2584+3 1.065 .175+0 .290–1 .3969+3 0.440 .828–1 .494–2
500 .3869+2 1.270 –.310+0 –.415–3 .8022+2 1.314 –.337+0 .557–2 .4473+2 1.968 .430+0 –.164–3 .7271+2 1.442 .140+0 .157–1 .1614+3 1.450 .108+0 .137–1 .3477+3 1.041 –.459–1 .252–1 .5186+3 1.064 –.387–1 .242–1 .4387+2 1.973 .309+0 –.647–4 .5339+2 1.541 .182+0 .501–2 .1192+3 1.523 .152+0 .450–2 .1751+3 1.153 –.298–1 .492–2
1000 .3060+2 1.362 –.826–1 .171–1 .6216+2 1.425 –.992–1 .237–1 .2912+2 1.972 .194+0 –.284–3 .4487+2 1.572 –.112–1 .269–2 .9460+2 1.601 –.278–1 .475–2 .1303+3 1.207 .148+0 .488–1 .1914+3 1.204 .160+0 .480–1 .1861+2 1.976 .165+0 –.180–3 .2318+2 1.673 .854–2 –.665–3 .4815+2 1.682 –.732–2 .709–3 .5003+2 1.336 .751–1 .251–1
157
E (eV) 1500 .2455+2 1.394 .112+0 .272–1 .4899+2 1.467 .108+0 .328–1 .2037+2 1.975 .531–1 –.345–3 .2953+2 1.601 –.288–2 .186–2 .6014+2 1.645 –.849–2 .572–2 .6038+2 1.229 .338+0 .651–1 .8774+2 1.212 .349+0 .652–1 .1027+2 1.978 .510–1 –.248–3 .1249+2 1.687 –.189–1 –.103–2 .2496+2 1.714 –.241–1 .199–2 .1972+2 1.333 .247+0 .405–1
2000 .1999+2 1.404 .281+0 .348–1 .3926+2 1.483 .288+0 .393–1 .1500+2 1.979 –.330–1 –.384–3 .2048+2 1.600 .681–1 .334–2 .4066+2 1.653 .719–1 .792–2 .3204+2 1.208 .503+0 .797–1 .4619+2 1.181 .511+0 .811–1 .6509+1 1.980 –.265–1 –.296–3 .7620+1 1.672 .295–1 –.378–3 .1484+2 1.712 .330–1 .363–2 .9449+1 1.289 .410+0 .550–1
3000 .1374+2 1.394 .558+0 .470–1 .2628+2 1.481 .587+0 .488–1 .9044+1 1.984 –.105+0 –.430–3 .1104+2 1.566 .265+0 .872–2 .2114+2 1.631 .286+0 .131–1 .1161+2 1.127 .762+0 .107+0 .1654+2 1.093 .761+0 .111+0 .3280+1 1.984 –.991–1 –.357–3 .3526+1 1.619 .205+0 .309–2 .6629+1 1.675 .224+0 .752–2 .3033+1 1.181 .678+0 .834–1
4000 .9826+1 1.367 .781+0 .575–1 .1838+2 1.459 .828+0 .567–1 .6000+1 1.988 –.990–1 –.460–3 .6625+1 1.518 .468+0 .158–1 .1235+2 1.590 .503+0 .190–1 .5198+1 1.039 .953+0 .135+0 .7340+1 1.002 .946+0 .141+0 .1962+1 1.987 –.100+0 –.397–3 .1935+1 1.560 .402+0 .875–2 .3550+1 1.626 .434+0 .125–1 .1266+1 1.076 .883+0 .112+0
5000 .7248+1 1.335 .967+0 .679–1 .1330+2 1.429 .103+1 .645–1 .4243+1 1.990 –.487–1 –.478–3 .4280+1 1.468 .655+0 .242–1 .7819+1 1.545 .702+0 .259–1 .2668+1 0.955 .110+1 .163+0 .3740+1 0.921 .109+1 .171+0 .1296+1 1.989 –.563–1 –.424–3 .1178+1 1.503 .589+0 .162–1 .2121+1 1.574 .634+0 .187–1 .6192+0 0.983 .104+1 .141+0
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables I, Z = 53 (continued) Shell 4d5/2 Eb = 56 eV 5s1/2 Eb = 20 eV 5 p1/2 Eb = 10 eV 5 p3/2 Eb = 10 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .4922+3 −.523 .276–1 .620–1 .7981+2 1.955 .188+0 .172–3 .3945+2 0.098 –.475–1 .200–1 .9425+2 0.180 –.480–1 .203–1
200 .6101+3 0.532 .818–1 .322–2 .3712+2 1.967 .264+0 .941–4 .2130+2 0.927 .119+0 .212–1 .4982+2 0.944 .115+0 .214–1
500 .2602+3 1.191 –.298–1 .508–2 .1088+2 1.974 .276+0 –.331–4 .8205+1 1.554 .192+0 .238–2 .1727+2 1.530 .163+0 .260–2
1000 .7287+2 1.334 .843–1 .247–1 .3672+1 1.976 .161+0 –.156–3 .3059+1 1.697 .155–1 –.127–2 .6002+1 1.700 –.923–3 –.155–4
E (eV) 1500 .2841+2 1.312 .257+0 .406–1 .1843+1 1.978 .530–1 –.228–3 .1542+1 1.706 –.217–1 –.143–2 .2917+1 1.729 –.273–1 .143–2
2000 .1350+2 1.258 .419+0 .562–1 .1108+1 1.980 –.236–1 –.278–3 .9068+0 1.688 .214–1 –.926–3 .1674+1 1.725 .248–1 .297–2
3000 .4286+1 1.140 .679+0 .871–1 .5283+0 1.984 –.973–1 –.342–3 .4030+0 1.631 .194+0 .220–2 .7196+0 1.685 .212+0 .665–2
4000 .1773+1 1.034 .877+0 .118+0 .3069+0 1.987 –.100+0 –.384–3 .2166+0 1.569 .390+0 .768–2 .3777+0 1.633 .423+0 .115–1
5000 .8615+0 0.944 .103+1 .149+0 .1991+0 1.989 –.582–1 –.412–3 .1301+0 1.509 .578+0 .148–1 .2229+0 1.580 .622+0 .174–1
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .5740+1 1.946 –.130+1 –.144–2 .2257+2 1.954 .112+1 –.207–3 .4450+2 0.959 –.442+0 –.330–1 .9415+2 0.957 –.453+0 –.341–1 .6434+2 1.961 .815+0 .126–3 .1064+3 0.867 .248+0 .122+0
200 .5697+1 1.945 –.110+1 –.151–2 .2189+2 1.955 .910+0 –.356–3 .4251+2 1.100 –.449+0 –.236–1 .8950+2 1.118 –.473+0 –.210–1 .5778+2 1.963 .690+0 .256–5 .9576+2 1.142 .322+0 .692–1
500 .5583+1 1.942 –.743+0 –.155–2 .2007+2 1.961 .543+0 –.542–3 .3693+2 1.265 –.326+0 –.146–2 .7669+2 1.309 –.354+0 .492–2 .4316+2 1.965 .449+0 –.176–3 .7031+2 1.434 .151+0 .172–1
1000 .5390+1 1.937 –.391+0 –.155–2 .1745+2 1.968 .229+0 –.665–3 .2951+2 1.358 –.989–1 .165–1 .6004+2 1.422 –.118+0 .236–1 .2858+2 1.969 .211+0 –.309–3 .4423+2 1.567 –.729–2 .303–2
E (eV) 1500 .5199+1 1.933 –.145+0 –.153–2 .1527+2 1.974 .638–1 –.719–3 .2389+2 1.391 .953–1 .268–1 .4774+2 1.466 .893–1 .329–1 .2022+2 1.973 .662–1 –.377–3 .2953+2 1.600 –.721–2 .179–2
2000 .5016+1 1.928 .485–1 –.151–2 .1346+2 1.978 –.264–1 –.752–3 .1960+2 1.402 .264+0 .345–1 .3855+2 1.483 .270+0 .394–1 .1501+2 1.977 –.237–1 –.421–3 .2070+2 1.601 .576–1 .304–2
3000 .4678+1 1.919 .354+0 –.147–2 .1065+2 1.985 –.879–1 –.779–3 .1365+2 1.394 .542+0 .467–1 .2613+2 1.483 .570+0 .488–1 .9157+1 1.982 –.104+0 –.473–3 .1134+2 1.570 .248+0 .807–2
4000 .4372+1 1.910 .599+0 –.144–2 .8599+1 1.988 –.658–1 –.791–3 .9862+1 1.369 .766+0 .571–1 .1846+2 1.464 .813+0 .566–1 .6121+1 1.986 –.105+0 –.507–3 .6876+1 1.525 .448+0 .148–1
5000 .4092+1 1.901 .803+0 –.141–2 .7064+1 1.989 –.905–3 –.792–3 .7338+1 1.338 .953+0 .673–1 .1347+2 1.435 .102+1 .642–1 .4353+1 1.988 –.620–1 –.527–3 .4479+1 1.477 .633+0 .229–1
Xe, Z = 54 Shell 1s1/2 Eb = 34565 eV 2s1/2 Eb = 5452 eV 2 p1/2 Eb = 5106 eV 2 p3/2 Eb = 4785 eV 3s1/2 Eb = 1149 eV 3 p1/2 Eb = 1001 eV
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TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Xe, Z = 54 (continued) Shell 3 p3/2 Eb = 939 eV 3d3/2 Eb = 689 eV 3d5/2 Eb = 676 eV 4s1/2 Eb = 213 eV 4 p1/2 Eb = 157 eV 4 p3/2 Eb = 147 eV 4d3/2 Eb = 69 eV 4d5/2 Eb = 67 eV 5s1/2 Eb = 23 eV 5 p1/2 Eb = 13 eV 5 p3/2 Eb = 12 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2545+3 0.838 .212+0 .111+0 .9035+3 0.452 –.676–1 –.814–2 .1378+4 0.491 –.688–1 –.905–2 .1312+3 1.960 .369+0 .226–3 .1292+3 0.509 –.115–1 .507–1 .3479+3 0.523 –.331–2 .472–1 .3331+3 −.600 –.147–1 .809–1 .5282+3 −.488 .162–1 .709–1 .8597+2 1.951 .191+0 .194–3 .4467+2 0.089 –.485–1 .208–1 .1090+3 0.172 –.490–1 .210–1
200 .2244+3 1.126 .278+0 .614–1 .6909+3 0.674 –.102+0 –.237–2 .1046+4 0.719 –.103+0 –.307–2 .9426+2 1.966 .383+0 .985–4 .1033+3 1.075 .200+0 .328–1 .2589+3 1.054 .178+0 .308–1 .4079+3 0.422 .901–1 .882–2 .6277+3 0.519 .901–1 .669–2 .4061+2 1.964 .267+0 .106–3 .2417+2 0.910 .117+0 .219–1 .5754+2 0.929 .113+0 .219–1
500 .1571+3 1.442 .116+0 .149–1 .3394+3 1.031 –.562–1 .242–1 .5065+3 1.056 –.488–1 .231–1 .4428+2 1.971 .321+0 –.672–4 .5432+2 1.533 .194+0 .572–2 .1222+3 1.513 .162+0 .513–2 .1853+3 1.141 –.298–1 .415–2 .2758+3 1.183 –.304–1 .434–2 .1205+2 1.972 .283+0 –.325–4 .9364+1 1.546 .202+0 .266–2 .1995+2 1.520 .170+0 .290–2
1000 .9378+2 1.597 –.261–1 .506–2 .1318+3 1.202 .135+0 .484–1 .1936+3 1.201 .148+0 .474–1 .1918+2 1.974 .177+0 –.194–3 .2409+2 1.671 .159–1 –.583–3 .5032+2 1.679 –.195–2 .745–3 .5471+2 1.335 .630–1 .240–1 .7976+2 1.335 .725–1 .235–1 .4102+1 1.975 .172+0 –.165–3 .3535+1 1.696 .240–1 –.128–2 .6996+1 1.697 .547–2 –.553–4
159
E (eV) 1500 .6043+2 1.643 –.144–1 .578–2 .6238+2 1.230 .325+0 .646–1 .9064+2 1.213 .337+0 .646–1 .1069+2 1.976 .622–1 –.269–3 .1313+2 1.688 –.205–1 –.114–2 .2637+2 1.715 –.273–1 .192–2 .2196+2 1.339 .231+0 .392–1 .3164+2 1.318 .242+0 .392–1 .2064+1 1.976 .635–1 –.246–3 .1793+1 1.709 –.227–1 –.155–2 .3417+1 1.731 –.297–1 .132–2
2000 .4126+2 1.654 .601–1 .787–2 .3359+2 1.213 .492+0 .790–1 .4842+2 1.186 .500+0 .803–1 .6812+1 1.978 –.179–1 –.322–3 .8078+1 1.675 .204–1 –.647–3 .1579+2 1.715 .228–1 .351–2 .1064+2 1.299 .394+0 .533–1 .1521+2 1.267 .404+0 .544–1 .1244+1 1.979 –.149–1 –.301–3 .1060+1 1.692 .127–1 –.117–2 .1968+1 1.729 .149–1 .284–2
3000 .2176+2 1.637 .267+0 .128–1 .1242+2 1.138 .754+0 .106+0 .1768+2 1.102 .754+0 .110+0 .3455+1 1.983 –.973–1 –.390–3 .3778+1 1.626 .187+0 .246–2 .7120+1 1.683 .205+0 .720–2 .3468+1 1.195 .664+0 .810–1 .4899+1 1.153 .667+0 .847–1 .5943+0 1.983 –.953–1 –.373–3 .4747+0 1.638 .175+0 .153–2 .8511+0 1.693 .193+0 .627–2
4000 .1284+2 1.599 .482+0 .185–1 .5635+1 1.052 .948+0 .133+0 .7949+1 1.014 .942+0 .139+0 .2075+1 1.986 –.105+0 –.435–3 .2090+1 1.569 .380+0 .772–2 .3840+1 1.636 .412+0 .118–1 .1462+1 1.093 .873+0 .109+0 .2048+1 1.049 .868+0 .115+0 .3458+0 1.986 –.105+0 –.420–3 .2566+0 1.579 .367+0 .660–2 .4489+0 1.644 .399+0 .108–1
5000 .8190+1 1.556 .681+0 .250–1 .2920+1 0.970 .110+1 .160+0 .4088+1 0.934 .109+1 .168+0 .1375+1 1.988 –.686–1 –.465–3 .1280+1 1.513 .565+0 .148–1 .2306+1 1.587 .610+0 .177–1 .7207+0 1.001 .104+1 .137+0 .1002+1 0.959 .103+1 .146+0 .2247+0 1.988 –.702–1 –.452–3 .1550+0 1.521 .552+0 .134–1 .2660+0 1.593 .597+0 .164–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
PHOTOELECTRON ANGULAR DISTRIBUTION PARAMETERS FOR ELEMENTS Z = 1 TO Z = 54 IN THE PHOTOELECTRON ENERGY RANGE 100–5000 eV M. B. TRZHASKOVSKAYA Petersburg Nuclear Physics Institute, 188300 Gatchina, Russia and V. I. NEFEDOV and V. G. YARZHEMSKY Kurnakov Institute of General and Inorganic Chemistry of the Russian Academy of Sciences, 31 Leninsky, 117907 Moscow, Russia
Parameters of the angular distribution of photoelectrons along with the subshell photoionization cross sections calculated for all subshells of atoms with 1 ≤ Z ≤ 54 are presented in the Table for nine photoelectron energies in the range 100–5000 eV. Relativistic treatment of the photoeffect is used. The calculations have been performed within the quadrupole approximation with the central Dirac–Fock–Slater potential. The hole left by the emitted electron has been taken into account in the framework of the frozen orbital approximation. Applications of nondipolar parameters to photoelectron angular distribution in solids, to quantitative x-ray photoelectron spectroscopy analysis, and to the x-ray standing wave method are discussed. ° 2001 Academic Press C
0092-640X/01 $35.00 C 2001 by Academic Press Copyright ° All rights of reproduction in any form reserved.
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Photoelectron Angular Distribution
CONTENTS INTRODUCTION .................................................................. Method of Calculation........................................................ Applications of Nondipolar Parameters.................................... Photoelectron Angular Distribution in Solids ....................... X-ray Photoelectron Spectroscopy ................................... X-ray Standing Wave Method .........................................
98 100 102 102 103 103
EXPLANATION OF TABLE ..................................................... Example ........................................................................
106 106
TABLE Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 ...................................
107
INTRODUCTION In photoeffect studies it is common to consider the angular distribution of photoelectrons within the electric dipole approximation (see, for example, [1–3] and references given therein). In this case the differential photoionization cross section for circularly polarized and unpolarized photons can be written as ¸ · σi β dσi (1) = 1 − P2 (cos θ ) , dÄ 4π 2
dipole approximation has also been demonstrated in recent experiments [18–20] where the photoionization of Ne, Ar, and Kr has been studied at photoelectron energies E ≤ 3000 eV.
characterized by the energy- and subshell-dependent asymmetry parameter β of the photoelectron angular distribution. Here σi is the photoionization cross section for the ith atomic subshell, P2 (cos θ ) is the second order Legendre polynomial, and θ is the angle between the vectors of photon (k) and photoelectron (p) propagation (Fig. 1). In keeping with Eq. (1), the currently available tables which may be used for estimation of the photoelectron angular distribution contain values of the photoionization cross sections σi and of the dipole parameter β [3–5]. However, there exist many investigations [6–17] where the angular distribution has been shown to differ significantly from that calculated within the dipole approximation, even for low photoelectron kinetic energies just above the photoionization threshold. In [6–11] the influence of quadrupole terms on the angular distribution has been studied using a nonrelativistic treatment of the photoeffect. Relativistic calculations have been carried out for a number of atoms using the quadrupole approximation [14, 15] as well as taking into account all multipoles of the radiation field [12, 13]. The breakdown of the
FIG. 1. Angles and directions. k and p represent the photon and photoelectron directions, respectively, ε gives the photon polarization direction, and S the direction normal to the solid taget.
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Photoelectron Angular Distribution
The angular distribution parameters have been calculated in the quadrupole approximation. The subshell photoionization cross sections σi have been computed including all multipoles L of the radiation field. Advantage has been taken of experimental values of the electron binding energies [27–29]. The electron wavefunctions have been computed by the use of the central Dirac–Fock–Slater (DFS) potential [30, 31] with allowance made for the hole in the atomic subshell from which an electron has been emitted. It is well known that relativistic effects may change the calculated photoelectron angular distribution parameters even at low energies. As shown in Refs. [14, 15, 32], the β parameter for s shells, which is equal to 2 within the nonrelativistic approximation, may differ considerably from this value. For outer s shells of heavy atoms, the parameter β obtained in relativistic calculations changes drastically with energy, even reversing sign near the photoionization threshold. As to the nondipolar parameters γ and δ, the comparison of our DFS results with nonrelativistic calculations [9] obtained by the use of the Hartree–Fock–Slater potential shows that the difference may also be substantial. The present relativistic parameters γ and δ for the 4s, 4 p, and 3d shells of Xe are listed in Table A along with the nonrelativistic values from [9]. In both works, the atomic model based on the statistical consideration of the exchange has been used. We present in this Table relativistic calculations for two cases: without regard for the hole (nh) and with allowance made for the hole (h). As is obvious from Table A, there is a large difference between relativistic values γ (R) and nonrelativistic values γ (NR) for the 3d shell in the energy range E < ∼ 500 eV. For the 4s shell the parameter γ (R) differs from γ (NR) appreciably, occasionally by several multiples, at energies E > ∼ 1000 eV. For the 4 p shell the parameters δ(R) and δ(NR), even though small in magnitude, differ from one another by several multiples over the entire energy range considered. It should also be pointed out that at energies E < ∼ 100 eV there is a significant discrepancy between the relativistic values of γ (R) obtained for the 4 p and 3d shells with and without regard for the hole (see Table A and Refs. [14, 15]). The peculiarities of the angular distribution parameters for different shells of atoms with different Z have been studied in [12, 14, 15]. The energy dependence of the parameters may be seen from Fig. 2, where the values of β and γ , as well as the values of δ multiplied by 10, are plotted for the 1s, 2 p3/2 , 3d5/2 , 4d5/2 , 5s, and 5 p3/2 shells of Xe over a wide energy range 5 eV ≤ E ≤ 50,000 eV. As indicated in Fig. 2, the nondipolar parameter γ is comparable in magnitude with the dipole parameter β in some energy regions; occasionally, |γ | > |β|. The small parameter δ increases considerably at energies E > ∼ 10,000 eV for p and d shells. Of special interest
In Ref. [9], simple expressions have been presented which describe adequately the angular distribution in various cases of photon polarization by the use of two additional nondipolar parameters γ and δ along with the dipole parameter β. According to Ref. [9], the photoelectron angular distribution for circular polarized and unpolarized photons may be written as µ ¶ · ¸ γ σi β dσi = 1− P2 (cos θ ) + sin2 θ + δ cos θ . (2) dÄ 4π 2 2 For linearly polarized photons the angular distribution may be represented as σi dσi = [1 + β P2 (cos θ) + (δ + γ cos2 θ) sin θ cos ϕ], dÄ 4π (3) where θ is the angle between the vector p and the photon polarization direction ε, the vector ε being coincident with the z axis; ϕ is the angle between the vector k and the plane passing through the z axis and the vector p. The angular distribution for the case of partially polarized photons is [21] ½ σi β 3 3 dσi = 1+ + Pβ cos 2θ + (P −1)β sin2 θ cos2 ϕ dÄ 4π 4 4 4 ¸ ¾ ½ · (P − 1) (1 − sin2 θ cos2 ϕ) + δ + γ P cos2 θ − 2 ¾ × sin θ cos ϕ , (4) where P is the fraction of photons polarized in the z direction. Calculations of the nondipolar parameters γ and δ have been performed only for several atoms. The atomic potential based either on the approximate consideration of the electron exchange interaction [7–13] or on the exact treatment of the exchange [6, 14, 15] has been used. The electron correlation effects have been considered in the framework of the random phase approximation for Ar [22] and Ne [23]. Currently, the most extensive calculations of the nondipolar parameters are given in Refs. [9] and [24] for the noble gases Ne, Ar, Kr, and Xe and in [25] for atoms with atomic numbers 3 ≤ Z ≤ 18. The present work provides the parameters of the photoelectron angular distribution for all elements 1 ≤ Z ≤ 54. The Table contains values of the three angular distribution parameters β, γ , and δ together with the subshell photoionization cross sections σi for nine photoelectron energies in the range 100 eV ≤ E ≤ 5000 eV. Relativistic treatment of the photoeffect [26] has been used. The calculations have been carried out in the one-electron approximation for a free atom. 99
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Photoelectron Angular Distribution
TABLE A
Relativistic (R) and Nonrelativistic (NR) [9] Calculations of the Parameters γ and δ vs Photoelectron Energy, E, for Xe, Z = 54 4s shell
4 p shell
3d shell
E b (NR) = 193 eV E b (4s1/2 ) = 213 eV
E b (NR) = 149 eV E b (4 p1/2 ) = 157 eV, E b (4 p3/2 ) = 147 eV
E b (NR) = 693 eV E b (3d3/2 ) = 689 eV , E b (3d5/2 ) = 676 eV
γ NR E (eV)
γ R
NR
nh
h
100
0.35
0.37
0.37
0.05
200
0.36
0.41
0.38
0.27
500
0.28
0.35
0.32
0.23
1000
0.12
0.19
0.17
0.02
2000
−0.05
−0.01
−0.02
0.03
4000
−0.08
−0.11
−0.10
0.37
5000
−0.01
−0.07
−0.07
0.54
δ R
γ
NR
nh
h
−0.09 −0.08 0.17 0.15 0.22 0.19 0.02 0.00 0.02 0.02 0.38 0.41 0.56 0.61
−0.01 0.00 0.20 0.18 0.19 0.16 0.02 0.00 0.02 0.02 0.38 0.41 0.56 0.61
0.02 0.01 −0.01 −0.01 0.00 0.03 0.04
R
NR
nh
h
0.05 0.05 0.04 0.04 0.01 0.01 0.00 0.00 0.00 0.00 0.01 0.01 0.01 0.02
0.05 0.05 0.03 0.03 0.01 0.01 0.00 0.00 0.00 0.00 0.01 0.01 0.01 0.02
−0.02 −0.04 −0.01 0.16 0.46 0.82 0.93
δ R
NR
nh
h
−0.05 −0.05 −0.09 −0.09 −0.06 −0.05 0.12 0.14 0.49 0.49 0.95 0.94 1.10 1.09
−0.07 −0.07 −0.10 −0.10 −0.06 −0.05 0.14 0.15 0.49 0.50 0.95 0.94 1.10 1.09
−0.01 −0.01 0.02 0.05 0.09 0.17 0.21
R nh
h
0.00 0.00 0.00 0.00 0.03 0.03 0.05 0.05 0.08 0.08 0.13 0.14 0.16 0.17
−0.01 −0.01 0.00 0.00 0.02 0.02 0.05 0.05 0.08 0.08 0.13 0.14 0.16 0.17
Note. E b (NR) is the binding energy given in [9], E b (n`j) is the experimental binding energy used in the present paper. In the relativistic case two values for shells with j = ` − 1/2 (upper) and with j = ` + 1/2 (lower) are listed. Relativistic values are presented for the cases where (i) no allowance is made for the hole (nh), and (ii) the hole is taken into account in the frozen orbital approximation (h).
is the oscillating character of all three curves β(E), γ (E), and δ(E) for outer 5 p3/2 and 4d5/2 shells as well as of γ (E) for the 5s shell. The comparison of our calculations with relativistic computations [24] performed in the independent particle approximation reveals that values of the β, γ , and δ parameters agree to within several percent or better, exclusive of regions where the parameters change rapidly with energy. All oscillatory features like the ones seen in Fig. 2 are usually well reproduced, although the curves may be shifted in energy. These deviations appear to arise from possible differences in the details of the physical assumptions. As discussed in detail in the literature [1, 2, 14, 15, 24], theoretical model assumptions underlying calculations of the photoionization parameters, like a different consideration of the exchange interaction, taking into account the hole, and including the correlation effects, may affect the values of the parameters. The influence of these physical assumptions may be important in two cases: (i) at low photoelectron energies E< ∼ 100 eV and (ii) at those E where a parameter becomes small in magnitude. In these energy regions a more rigorous treatment of photoionization may be required.
Method of Calculation The differential cross section in the ith atomic subshell for circularly polarized and unpolarized photons in the quadrupole approximation can be written as " # 4 X σi dσi = 1+ Bn Pn (cos θ) . dÄ 4π n=1
(5)
We use a relativistic formalism [3, 26] in studies of photoionization. All formulae below are given in relativistic units, in which the Compton wavelength h--/m 0 c is defined as the unit of length, and the electron rest mass m 0 c2 is the unit of energy, that is, h-- = m 0 = c = 1. The subshell photoionization cross section σi in Eq. (5) is defined by the following expression: σi =
4π 2 α X X {(2L + 1)[Q 3=L ,L (κ)]2 k κ L + L[Q 3=L+1,L (κ)]2 + (L + 1)[Q 3=L−1,L (κ)]2 p − 2 L(L + 1)Q 3=L−1,L (κ)Q 3=L+1,L (κ)}. (6)
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Photoelectron Angular Distribution
¤ − 3Q 11 (κ1 )Q 11 (κ2 ) − Q 21 (κ1 )Q 21 (κ2 ) √ £√ + 30W (12 j1 j2 ; 2 ji ) 10Q 01 (κ1 )Q 22 (κ2 ) − Q 11 (κ1 ) √ √ ¤ × [3Q 12 (κ2 ) − 6Q 32 (κ2 )] − 5Q 21 (κ1 )Q 22 (κ2 ) 5 − √ W (22 j1 j2 ; 2 ji )[Q 12 (κ1 )[3Q 12 (κ2 ) 14 √ − 2 6Q 32 (κ2 )] + 5Q 22 (κ1 )Q 22 (κ2 ) ) + 2Q 32 (κ1 )Q 32 (κ2 )] ,
B3 =
B4 = FIG. 2. Photoelectron angular distribution parameters β (solid line), γ (dashed line), and δ × 10 (dot-dashed line) versus photoelectron energy E for Xe.
The coefficients B1 , B2 , B3 , and B4 may be represented as follows: B1 =
B2 =
p 4π 2 α X (−1) j1 + j2 +|κi | |κ1 ||κ2 | C 10 j1 1/2 j2 −1/2 kσi κ1 ,κ2 ¡ ¢© √ × sin δκ1 − δκ2 3 6W (11 j1 j2 ; 1 ji ) √ × [ 2Q 01 (κ1 )Q 11 (κ2 ) + Q 11 (κ1 )Q 21 (κ2 )] √ √ £ + 3 2W (12 j1 j2 ; 1 ji ) Q 01 (κ1 )[ 6Q 12 (κ2 ) √ − 2Q 32 (κ2 )] + 15Q 11 (κ1 )Q 22 (κ2 ) − Q 21 (κ1 ) √ √ ¤ × [ 3Q 12 (κ2 ) − 2Q 32 (κ2 )] √ − 5W (22 j1 j2 ; 1 ji )[ 6 Q 12 (κ1 )Q 22 (κ2 ) ª + 2Q 22 (κ1 )Q 32 (κ2 )] ,
(8)
p 4π 2 α X (−1) j1 + j2 +|κi | |κ1 ||κ2 | C 30 j1 1/2 j2 −1/2 kσi κ1 ,κ2 ¡ £ ¢© √ × sin δκ1 − δκ2 2 3W (12 j1 j2 ; 3 ji ) Q 01 (κ1 ) √ √ × [ 6Q 12 (κ2 ) − 2Q 32 (κ2 )] + 15Q 11 (κ1 )Q 22 (κ2 ) √ √ ¤ − Q 21 (κ1 )[ 3Q 12 (κ2 ) − 2Q 32 (κ2 )] √ √ + 10 2W (22 j1 j2 ; 3 ji )[ 3Q 12 (κ1 )Q 22 (κ2 ) √ ª (9) + 2Q 22 (κ1 )Q 32 (κ2 )] , p 4π 2 α X (−1) j1 + j2 +|κi | |κ1 ||κ2 | C 40 j1 1/2 j2 −1/2 kσi κ1 ,κ2 ( r ¡ ¢ 10 W (22 j1 j2 ; 4 ji ) × cos δκ1 − δκ2 2 7 √ £ × Q 12 (κ1 )[−3Q 12 (κ2 ) + 2 6Q 32 (κ2 )] ) ¤ − 5Q 22 (κ1 )Q 22 (κ2 ) − 2Q 32 (κ1 )Q 32 (κ2 ) .
(10)
The coefficients B1 , B2 , and B3 are related to the parameters β, γ , and δ describing the photoelectron angular distribution in accordance with Eqs. (2)–(4), in the following way: β = –2B2 , γ = –5B3 , δ = B1 + B3 .
(11)
The coefficient B4 , which is small in magnitude in the energy range considered, does not enter into expressions for the parameters β, γ , and δ. Equation (10) for B4 is presented here for completeness in line with the exact formula (5) for the differential cross section in the quadrupole approximation. In Eqs. (6–10) κ = (` – j)(2 j + 1) is the relativistic quantum number, ` and j are quantum numbers of the orbital and total angular momenta of the electron, k is the photon energy, α = e2 / h-- c is the fine-structure constant, C jJ1M m 1 j2 m 2 is the Clebsch–Gordan coefficient, W (L 1 L 2 j1 j2 ; n ji ) is the Racah coefficient, and (δκ1 − δκ2 ) is the corresponding phase shift for the two possible final continuum states characterized by
(7)
p 4π 2 α X (−1) j1 + j2 +|κi | |κ1 ||κ2 | C 20 j1 1/2 j2 −1/2 kσi κ1 ,κ2 (r ¡ ¢ 3 W (11 j1 j2 ; 2 ji ) × cos δκ1 − δκ2 2 √ £ × 2Q 01 (κ1 )[−Q 01 (κ2 ) + 2Q 21 (κ2 )] 101
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κ1 and κ2 . The reduced matrix element Q ΛL (κ) has the form
The continuum wavefunctions are normalized per unit energy range so that at large distances
Q ΛL (κ) = [(2`¯ + 1)(2`i + 1)/(2Λ + 1)]1/2 `¯ 1/2 j Λ0 × C`0` 1/2 ji R1Λ ¯ i 0 A`i Λ
1
1
s G κ (r ) → and
Λ
1
j1
(12)
where E here √ is the total electron energy including the rest mass, p = E 2 − 1. The computational accuracy of our calculations is better than 0.1%. This accuracy does not include possible uncertainties due to the physical approximations mentioned above. It should be pointed out that in the Table the values of the subshell cross section σi are always given for completely filled shells. To obtain σi for a partially filled atomic subshell i, the value from the Table should be divided by 2 ji + 1 and multiplied by the actual occupation number of the ith subshell.
j2 L
G i (r )Fκ (r ) jΛ (kr ) dr 0
Applications of Nondipolar Parameters (13)
∞
R2Λ =
Photoelectron Angular Distribution in Solids
Fi (r )G κ (r ) jΛ (kr ) dr. 0
Accounting for the photoelectron elastic scattering in the solid results in the following expressions for nonpolarized and linearly polarized excitation sources:
Here jΛ (kr ) is the spherical Bessel function of order Λ, G(r ) = rg(r ) and F(r ) = r f (r ) are the large and small components of the Dirac radial electron wavefunction. Indices i and κ refer to bound and continuum states, respectively. Electron wavefunctions are calculated in the DFS atomic field, the exchange term of the potential being written as Vex = −Cα
· ¸1/3 3 3 ρ(r ) , 2 π
for nonpolarized photons µ ¶ · ¸ β γ aσi dσi = D1 − P2 (cos θ) + sin2 θ + δ cos θ , dÄ 4π 4 2 (17)
(14) for linearly polarized photons · aσi β dσi = D1 + P2 (cos θ ) dÄ 4π 2 ¶ ¸ µ γ cos2 θ + δ sin θ cos ϕ . + 2
where ρ(r ) is the total radial electron density. The coefficient C = 1 is chosen according to Ref. [30]. The wavefunctions of the initial bound states are computed in the self-consistent DFS field of a neutral atom. Continuum wavefunctions are calculated in the frozen orbital approximation where the DFS field of the ion with the hole produced after photoionization is considered, the ion potential being computed by the use of the bound wavefunctions of the neutral atom. The bound electron wavefunctions are normalized so that Z
∞ 0
£
E −1 cos( pr + δκ ), πp
∞
R1Λ = Z
κ |κ|
s
L
is the normalized coefficient of recoupling of four angular momenta. The radial integrals R1Λ and R2Λ can be written as Z
(16) Fκ (r ) →
where `¯ = 2 j − ` and `1 1/2 A`2 1/2
E +1 sin( pr + δκ ) πp
L
+ [(2` + 1)(2`¯i + 1)/(2Λ + 1)]1/2 ` 1/2 j ¯ Λ0 × C`0 1/2 ji R2Λ , `¯i 0 A`i Λ
Photoelectron Angular Distribution
¤ G i2 (r ) + Fi2 (r ) dr = 1.
(18)
Here a = 1 − ω, where ω is the single scattering albedo, D1 = H (ω, α)a −0.5 , H (ω, α) is the Chandrasekhar function, and α is the emission angle of the photoelectron relative to the direction normal to the surface (Fig. 1). Formulae (17) and (18) are obtained using the transport theory approach and the results are in good agreement with the Monte Carlo calculations [16, 17].
(15)
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In contrast to the dipole angular distribution parameter β, the nondipolar parameters γ and δ make the angular distribution dependent on the direction of the photon propagation vector k. Specifically, if the projection of the photoelectron propagation vector p on the photon direction k is positive, i.e., for the back side of the solid sample, the intensity increases in comparison with the dipole approximation. Conversely, for the front side of the solid sample the intensity decreases [25] (see Fig.3). Experimental determination of the γ and δ values has been carried out in [19, 20] based on the photoelectron angular dependence. Our calculations [15, 25] are in good agreement with experimental values for Ar 1s and for Kr 2s and 2 p lines.
Photoelectron Angular Distribution
FIG. 4. Dependence of the q-values of 1s lines on the atomic number for a photon energy 1486.6 eV. The side of the sample facing the photon beam is considered, where cos θ< 0, q < 0 (see Eq. (19) for θ = 125.6◦ ).
X-ray Photoelectron Spectroscopy 54.4◦ since there is no β dependence of the intensity at this angle and, in the dipole approximation, the XPS intensities are proportional to the subshell photoionization cross sections. However, this is not the case when the nondipolar parameters are taken into account. In [33] the q-value is calculated as
The nondipolar parameters γ and δ are important for quantitative x-ray photoelectron spectroscopy (XPS) analysis. Some commercial spectrometers are set at an angle θ =
q=
γ (1 − cos2 θ) cos θ 2
(19)
for all the intense XPS lines used for quantitative analysis in the case of θ = 54.4◦ . The q-value is known to be approximately equal to the percent contribution of nondipolar transitions to the intensity calculated in the dipole approximation. The q-value is shown to be as large as 15% in some cases. As an example, results for 1s lines are given for a photon energy of 1486.6 eV in Fig. 4 [25]. X-ray Standing Wave Method The importance of nondipolar parameters for the interpretation of x-ray standing wave measurements is discussed in [34]. In that paper the parameter Q is introduced which takes into account nondipolar contributions to the intensities of photoelectron lines. In Table B the experimental TABLE B
Experimental and Theoretical Q-Parameters (see text) Line: k (eV): Q exp : Q theor :
FIG. 3. Intensity dependence of Be 1s line (arbitrary units) on the emission angle for a photon energy 1253.6 eV. (A) Linearly polarized excitation. (B) Unpolarized excitation. (1) Dipole approximation. (2) Dipolar and nondipolar contributions for the front sample side. (3) Dipolar and nondipolar contributions for the back sample side.
a b
103
I 3p 2355 0.03a 0.04
I 3d 2355 0.21a 0.23
O 1s 2975 0.27b 0.26
F 1s 2975 0.25b 0.26
Ref. [34]. Ref. [35].
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
15. M. B. Trzhaskovskaya, Yu. I. Kharitonov, V. I. Nefedov, and V. G. Yarzhemsky, Optica i Spectroscopia 88, 547 (2000) [in Russian]
Q-parameters for lines in iodine, oxygen, and fluorine are compared with the calculated ones. The calculations are performed in the approximation used in this paper at the photon energies given in Table B.
16. V. I. Nefedov and I. S. Nefedova, J. Electr. Spectrosc. 107, 131 (2000)
Acknowledgments
17. V. I. Nefedov and I. S. Nefedova, J. Electr. Spectrosc. (to be published)
This work is supported by Grant of Russian Foundation for Basic Research No 99-03-32640. The authors are grateful to the referee for useful comments.
18. B. Kr¨assig, M. Jung, D. S. Gemmell, E. P. Kanter, T. LeBrun, S. H. Southworth, and L. Young, Phys. Rev. Lett. 75, 4736 (1995)
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19. M. Jung, B. Kr¨assig, D. S. Gemmell, E. P. Kanter, T. LeBrun, S. H. Southworth, and L. Young, Phys. Rev. A 54, 2127 (1996)
2. M. Ya. Amusia, Atomic Photoeffect (Plenum Press, New York, 1990)
20. O. Hemmers, et al., J. Phys. B 30, L727 (1997)
3. I. M. Band, Yu. I. Kharitonov, and M. B. Trzhaskovskaya, ATOMIC DATA AND NUCLEAR DATA TABLES 23, 443 (1979)
21. P. S. Shaw, U. Arp, and S. H. Southworth, Phys. Rev. A 54, 1463 (1996)
4. K.-N. Huang, W. R. Johnson, and K. T. Cheng, ATOMIC DATA AND NUCLEAR DATA TABLES 26, 33 (1981)
22. M. Ya. Amusia, A. S. Baltenkov, Z. Felfli, and A. Z. Msezane, Phys. Rev. A 59, R2544 (1999)
5. J. J. Yeh and I. Lindau, ATOMIC DATA AND NUCLEAR DATA TABLES 32, 1 (1985)
23. W. R. Johnson, A. Derevianko, K. T. Cheng, V. K. Dolmatov, and S. T. Manson, Phys. Rev. A 59, 3609 (1999)
6. M. Ya. Amusia and N. A. Cherepkov, Case Studies in Atomic Physics (North-Holland, Amsterdam, 1975), Vol. 5, p. 155
24. A. Derevianko, W. R. Johnson, and K. T. Cheng, ATOMIC DATA AND NUCLEAR DATA TABLES 73, 153 (1999)
7. J. W. Cooper, Phys. Rev. A 42, 6942 (1990) 25. V. I. Nefedov, V. G. Yarzhemsky, I. S. Nefedova, M. B. Trzhaskovskaya, and I. M. Band, J. Electr. Spectrosc. 107, 123 (2000)
8. J. W. Cooper, Phys. Rev. A 45, 3362 (1992) 9. J. W. Cooper, Phys. Rev. A 47, 1841 (1993)
26. R. Racavy and A. Ron, Spectroscopic and Group Theoretical Methods in Physics (North-Holland, Amsterdam, 1968), p. 175
10. A. Bechler and R. H. Pratt, Phys. Rev. A 39, 1774 (1989) 11. A. Bechler and R. H. Pratt, Phys. Rev. A 42, 6400 (1990)
27. J. Bearden and A. Burr, Rev. Mod. Phys. 39, 125 (1967) 12. Y. S. Kim, R. H. Pratt, A. Ron, and H. K. Tseng, Phys. Rev. A 22, 567 (1980)
28. W. Lotz, J. Opt. Soc. Am. 60, 206 (1970)
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29. K. Siegbahn et al., ESCA: Atomic Molecular and Solid State Structure Studied by Means of Electron Spectroscopy (Almqvist & Wiksells, Uppsala, 1967)
14. M. B. Trzhaskovskaya and Yu. I. Kharitonov, Study of Photoelectron Angular-Distribution Parameters in Relativistic Quadrupole Approximation, Petersburg Nuclear Physics Institute Publication No. 2257 (1998)
30. J. C. Slater, Quantum Theory of Atomic Structure (McGraw–Hill, New York, 1960) 104
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31. I. M. Band, M. A. Listengarten, M. B. Trzhaskovskaya, and V. I. Fomichev, Complex of Programs RAINE, Part I, Leningrad Nuclear Physics Institute Publication No. 289 (1976)
Photoelectron Angular Distribution
Band and M. B. Trzhaskovskaya, Poverkhnost 6, 16 (2000) [in Russian]
32. T. E. H. Walker and J. T. Waber, J. Phys. B 7, 674 (1974)
34. C. J. Fisher, R. Ithin, R. G. Jones, G. J. Jackson, D. P. Woodruff, and B. C. C. Cowie, J. Phys.: Condens. Matter. 10, L623 (1998)
33. V. I. Nefedov, V. G. Yarzhemsky, I. S. Nefedova, I. M.
35. D. P. Woodruff, private communication (1998)
105
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EXPLANATION OF TABLE TABLE .
Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 The Table contains the values of the subshell photoionization cross sections σi , Eq. (6), and of the photoelectron angular distribution parameters β, γ , and δ, Eqs. (7–11), at nine photoelectron energies in the range 100 eV ≤ E ≤ 5000 eV. The photoionization cross sections σi are given in kb (=10−21 cm2 ) for completely filled subshells. To obtain σi for a partially filled atomic subshell i, the value from the Table should be divided by 2 ji + 1 and multiplied by the actual occupation number of the ith subshell. Z Atomic number Shell Atomic subshell in which the photoionization occurs Experiment subshell binding energy in eV from [27–29] Eb E Photoelectron energy in eV σ Subshell photoionization cross section in kb (=10−21 cm2 ) β Dipole parameter of the angular distribution γ Nondipolar parameter γ of the angular distribution δ Nondipolar parameter δ of the angular distribution Example In the Table, the first data block gives the parameters for the 1s shell of hydrogen, Z = 1. The binding energy of this shell, rounded off to two digits, is equal to 14 eV. At the photoelectron energy E = 100 eV the subshell photoionization cross section σ = 0.2607 × 102 kb = 0.2607 × 10−19 cm2 , the dipole angular distribution parameter β = 1.999, and the nondipolar parameters γ = 0.237 and δ = −0.164 × 10−8 .
106
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TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables H, Z = 1 Shell 1s1/2 Eb = 14 eV
100 .2607+2 1.999 .237+0 –.164–8
200 .3564+1 1.998 .335+0 –.210–8
500 .2076+0 1.995 .530+0 –.169–8
1000 .2183–1 1.989 .748+0 .309–8
E (eV) 1500 .5691–2 1.984 .915+0 .144–7
2000 .2173–2 1.979 .105+1 .263–7
3000 .5535–3 1.968 .129+1 .913–7
4000 .2085–3 1.958 .148+1 .129–6
5000 .9749–4 1.947 .165+1 .483–6
100 .1411+3 1.999 .187+0 .525–7
200 .3134+2 1.998 .279+0 .597–7
500 .2831+1 1.995 .499+0 .122–7
1000 .3453+0 1.990 .733+0 .172–6
E (eV) 1500 .9821–1 1.985 .881+0 .181–6
2000 .3996–1 1.980 .103+1 –.717–8
3000 .1060–1 1.967 .130+1 .115–6
4000 .4069–2 1.958 .147+1 .680–6
5000 .1963–2 1.949 .162+1 .758–6
100 .3658+3 1.999 .177+0 –.121–6 .2905+2 2.000 .141+0 –.534–7
200 .1044+3 1.998 .276+0 .180–8 .6171+1 1.999 .238+0 .228–7
500 .1276+2 1.996 .471+0 .195–6 .5399+0 1.996 .468+0 –.469–8
1000 .1996+1 1.990 .699+0 .262–6 .7194–1 1.991 .683+0 .166–7
E (eV) 1500 .6168+0 1.985 .872+0 .302–6 .2094–1 1.985 .879+0 .524–7
2000 .2601+0 1.980 .102+1 .328–6 .8490–2 1.980 .101+1 .127–6
3000 .7406–1 1.969 .126+1 .494–6 .2347–2 1.969 .127+1 .201–6
4000 .2976–1 1.959 .146+1 .700–6 .9237–3 1.959 .145+1 .603–6
5000 .1451–1 1.948 .163+1 .106–5 .4462–3 1.947 .164+1 .583–6
σ β γ δ σ β γ δ
100 .4680+3 1.999 .160+0 –.405–6 .8391+2 2.000 .112+0 –.782–7
200 .1773+3 1.998 .262+0 –.264–6 .1884+2 1.999 .213+0 –.760–7
500 .2972+2 1.995 .463+0 .702–7 .2054+1 1.996 .427+0 –.693–8
1000 .5539+1 1.991 .684+0 .351–6 .3027+0 1.991 .672+0 .225–7
E (eV) 1500 .1870+1 1.985 .855+0 .485–6 .9275–1 1.986 .846+0 .687–7
2000 .8315+0 1.980 .100+1 .594–6 .3915–1 1.981 .985+0 .159–6
3000 .2525+0 1.970 .124+1 .848–6 .1127–1 1.970 .123+1 .346–6
4000 .1053+0 1.959 .144+1 .117–5 .4559–2 1.960 .144+1 .620–6
5000 .5267–1 1.949 .162+1 .160–5 .2239–2 1.949 .162+1 .961–6
σ β γ δ
100 .4687+3 1.999 .145+0 –.769–6
200 .2237+3 1.998 .244+0 –.647–6
500 .5013+2 1.995 .448+0 –.271–6
1000 .1110+2 1.991 .675+0 .207–6
E (eV) 1500 .4051+1 1.986 .846+0 .523–6
2000 .1892+1 1.980 .989+0 .755–6
3000 .6116+0 1.970 .123+1 .116–5
4000 .2647+0 1.960 .143+1 .164–5
5000 .1358+0 1.949 .160+1 .222–5
σ β γ δ
He, Z = 2 Shell 1s1/2 Eb = 25 eV
σ β γ δ
Li, Z = 3 Shell 1s1/2 Eb = 58 eV 2s1/2 Eb = 5 eV
σ β γ δ σ β γ δ
Be, Z = 4 Shell 1s1/2 Eb = 115 eV 2s1/2 Eb = 9 eV
B, Z = 5 Shell 1s1/2 Eb = 192 eV
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TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables B, Z = 5 (continued) Shell 2s1/2 Eb = 12 eV 2 p1/2 Eb = 8 eV
σ β γ δ σ β γ δ
100 .1694+3 2.000 .742–1 –.136–6 .3876+2 1.241 .153+0 .125–1
200 .4261+2 1.999 .177+0 –.134–6 .5378+1 0.920 .182+0 .259–1
500 .5253+1 1.997 .389+0 –.563–7 .2925+0 0.548 .262+0 .586–1
1000 .8689+0 1.992 .633+0 .248–7 .2420–1 0.305 .348+0 .989–1
E (eV) 1500 .2789+0 1.987 .814+0 .889–7 .5145–2 0.181 .397+0 .129+0
2000 .1205+0 1.981 .966+0 .159–6 .1667–2 0.127 .384+0 .154+0
3000 .3594–1 1.971 .121+1 .407–6 .3384–3 0.088 .446+0 .195+0
4000 .1492–1 1.961 .142+1 .735–6 .1067–3 0.061 .511+0 .229+0
5000 .7462–2 1.950 .160+1 .118–5 .4297–4 0.033 .582+0 .259+0
σ β γ δ σ β γ δ σ β γ δ
100 .4240+3 1.999 .128+0 –.120–5 .2500+3 2.000 .391–1 –.226–6 .9818+2 1.380 .149+0 .107–1
200 .2399+3 1.998 .227+0 –.112–5 .7188+2 1.999 .136+0 –.228–6 .1495+2 1.099 .204+0 .214–1
500 .6913+2 1.996 .431+0 –.747–6 .9932+1 1.997 .349+0 –.870–7 .9207+0 0.685 .286+0 .507–1
1000 .1809+2 1.991 .661+0 –.176–6 .1778+1 1.993 .589+0 .140–7 .8638–1 0.438 .371+0 .890–1
E (eV) 1500 .7150+1 1.986 .835+0 .294–6 .5983+0 1.988 .777+0 .796–7 .1939–1 0.313 .417+0 .120+0
2000 .3502+1 1.980 .979+0 .687–6 .2674+0 1.982 .937+0 .179–6 .6439–2 0.216 .460+0 .147+0
3000 .1198+1 1.970 .122+1 .137–5 .8230–1 1.972 .119+1 .458–6 .1321–2 0.119 .504+0 .190+0
4000 .5375+0 1.960 .142+1 .204–5 .3483–1 1.962 .139+1 .869–6 .4244–3 0.078 .549+0 .224+0
5000 .2828+0 1.950 .159+1 .276–5 .1767–1 1.951 .157+1 .141–5 .1741–3 0.057 .582+0 .253+0
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3688+3 1.999 .106+0 –.169–5 .3172+3 2.000 .104–1 –.379–6 .1901+3 1.454 .133+0 .988–2 .3788+3 1.455 .133+0 .101–1
200 .2356+3 1.998 .209+0 –.166–5 .1030+3 2.000 .951–1 –.363–6 .3229+2 1.239 .210+0 .182–1 .6429+2 1.241 .210+0 .186–1
500 .8359+2 1.996 .413+0 –.133–5 .1602+2 1.998 .304+0 –.116–6 .2199+1 0.825 .308+0 .437–1 .4371+1 0.827 .308+0 .440–1
1000 .2554+2 1.991 .643+0 –.713–6 .3061+1 1.993 .551+0 –.428–7 .2219+0 0.544 .379+0 .812–1 .4402+0 0.546 .379+0 .814–1
E (eV) 1500 .1092+2 1.986 .819+0 –.155–6 .1074+1 1.988 .742+0 .454–7 .5255–1 0.405 .436+0 .113+0 .1041+0 0.408 .435+0 .113+0
2000 .5614+1 1.981 .967+0 .352–6 .4936+0 1.983 .895+0 .188–6 .1829–1 0.318 .492+0 .137+0 .3620–1 0.323 .491+0 .137+0
3000 .2034+1 1.970 .121+1 .131–5 .1573+0 1.973 .115+1 .498–6 .3879–2 0.202 .548+0 .180+0 .7663–2 0.209 .545+0 .180+0
4000 .9444+0 1.960 .141+1 .226–5 .6793–1 1.962 .137+1 .945–6 .1254–2 0.127 .578+0 .217+0 .2473–2 0.137 .574+0 .217+0
5000 .5088+0 1.950 .158+1 .322–5 .3493–1 1.952 .155+1 .158–5 .5194–3 0.083 .625+0 .247+0 .1022–2 0.096 .620+0 .247+0
C, Z = 6 Shell 1s1/2 Eb = 288 eV 2s1/2 Eb = 16 eV 2 p1/2 Eb = 11 eV
N, Z = 7 Shell 1s1/2 Eb = 403 eV 2s1/2 Eb = 20 eV 2 p1/2 Eb = 14 eV 2 p3/2 Eb = 14 eV
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TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables O, Z = 8 Shell 1s1/2 Eb = 538 eV 2s1/2 Eb = 28 eV 2 p1/2 Eb = 14 eV 2 p3/2 Eb = 14 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3160+3 1.999 .795–1 –.226–5 .3572+3 2.000 –.975–2 –.621–6 .3183+3 1.486 .111+0 .941–2 .6340+3 1.487 .111+0 .963–2
200 .2206+3 1.998 .187+0 –.229–5 .1306+3 2.000 .577–1 –.560–6 .5985+2 1.337 .199+0 .159–1 .1191+3 1.339 .199+0 .163–1
500 .9256+2 1.996 .395+0 –.202–5 .2302+2 1.998 .260+0 –.199–6 .4449+1 0.957 .320+0 .380–1 .8832+1 0.959 .320+0 .382–1
1000 .3253+2 1.991 .626+0 –.138–5 .4727+1 1.994 .513+0 –.140–6 .4744+0 0.645 .399+0 .740–1 .9398+0 0.648 .399+0 .743–1
E (eV) 1500 .1500+2 1.986 .802+0 –.768–6 .1719+1 1.989 .702+0 .104–7 .1177+0 0.491 .463+0 .104+0 .2329+0 0.494 .462+0 .104+0
2000 .8087+1 1.981 .951+0 –.185–6 .8077+0 1.984 .861+0 .131–6 .4199–1 0.397 .500+0 .129+0 .8297–1 0.401 .499+0 .130+0
3000 .3107+1 1.970 .120+1 .974–6 .2664+0 1.974 .112+1 .495–6 .9294–2 0.273 .575+0 .173+0 .1833–1 0.280 .573+0 .173+0
4000 .1493+1 1.960 .140+1 .217–5 .1175+0 1.964 .134+1 .104–5 .3085–2 0.191 .635+0 .208+0 .6070–2 0.201 .631+0 .208+0
5000 .8238+0 1.950 .157+1 .340–5 .6126–1 1.953 .152+1 .169–5 .1289–2 0.136 .661+0 .239+0 .2531–2 0.148 .656+0 .239+0
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2699+3 1.999 .497–1 –.290–5 .3764+3 2.000 –.206–1 –.960–6 .4608+3 1.491 .931–1 .947–2 .9173+3 1.492 .933–1 .963–2
200 .2012+3 1.998 .162+0 –.301–5 .1531+3 2.000 .250–1 –.839–6 .9682+2 1.400 .183+0 .147–1 .1924+3 1.402 .183+0 .151–1
500 .9660+2 1.995 .375+0 –.281–5 .3050+2 1.999 .216+0 –.367–6 .7933+1 1.071 .324+0 .339–1 .1573+2 1.074 .325+0 .340–1
1000 .3843+2 1.991 .609+0 –.220–5 .6754+1 1.995 .472+0 –.245–6 .8987+0 0.750 .426+0 .672–1 .1778+1 0.752 .426+0 .675–1
E (eV) 1500 .1900+2 1.986 .785+0 –.154–5 .2537+1 1.990 .662+0 –.503–7 .2307+0 0.581 .486+0 .957–1 .4556+0 0.584 .486+0 .958–1
2000 .1073+2 1.981 .935+0 –.898–6 .1219+1 1.985 .826+0 .602–7 .8403–1 0.469 .526+0 .122+0 .1657+0 0.473 .525+0 .122+0
3000 .4370+1 1.971 .118+1 .410–6 .4140+0 1.975 .109+1 .502–6 .1934–1 0.339 .606+0 .164+0 .3805–1 0.345 .604+0 .164+0
4000 .2177+1 1.960 .138+1 .180–5 .1861+0 1.965 .130+1 .104–5 .6568–2 0.255 .656+0 .200+0 .1289–1 0.264 .652+0 .200+0
5000 .1230+1 1.950 .156+1 .328–5 .9848–1 1.955 .149+1 .178–5 .2786–2 0.190 .702+0 .232+0 .5459–2 0.201 .697+0 .231+0
100 .2313+3 1.999 .184–1 –.361–5
200 .1813+3 1.998 .134+0 –.381–5
500 .9695+2 1.995 .353+0 –.371–5
1000 .4296+2 1.991 .591+0 –.314–5
E (eV) 1500 .2267+2 1.986 .769+0 –.246–5
2000 .1338+2 1.981 .918+0 –.177–5
3000 .5764+1 1.971 .117+1 –.347–6
4000 .2974+1 1.961 .137+1 .120–5
5000 .1722+1 1.950 .155+1 .286–5
F, Z = 9 Shell 1s1/2 Eb = 694 eV 2s1/2 Eb = 38 eV 2 p1/2 Eb = 17 eV 2 p3/2 Eb = 17 eV
Ne, Z = 10 Shell 1s1/2 Eb = 870 eV
σ β γ δ
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Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Ne, Z = 10 (continued) Shell 2s1/2 Eb = 48 eV 2 p1/2 Eb = 22 eV 2 p3/2 Eb = 22 eV
σ β γ δ σ β γ δ σ β γ δ
100 .3839+3 2.000 –.203–1 –.138–5 .6004+3 1.477 .791–1 .982–2 .1194+4 1.479 .793–1 .993–2
200 .1711+3 2.000 –.160–2 –.120–5 .1415+3 1.440 .166+0 .142–1 .2810+3 1.442 .166+0 .145–1
500 .3815+2 1.999 .172+0 –.630–6 .1288+2 1.167 .323+0 .307–1 .2549+2 1.170 .324+0 .310–1
1000 .9095+1 1.995 .425+0 –.355–6 .1557+1 0.851 .449+0 .609–1 .3075+1 0.854 .449+0 .611–1
E (eV) 1500 .3527+1 1.991 .620+0 –.175–6 .4103+0 0.671 .509+0 .885–1 .8086+0 0.674 .509+0 .885–1
2000 .1732+1 1.986 .784+0 –.854–8 .1529+0 0.546 .557+0 .114+0 .3008+0 0.551 .557+0 .114+0
3000 .6034+0 1.977 .105+1 .432–6 .3620–1 0.403 .626+0 .156+0 .7104–1 0.409 .625+0 .156+0
4000 .2763+0 1.966 .127+1 .102–5 .1254–1 0.310 .679+0 .192+0 .2455–1 0.318 .675+0 .192+0
5000 .1482+0 1.956 .146+1 .187–5 .5420–2 0.245 .734+0 .223+0 .1059–1 0.256 .729+0 .223+0
100 .1937+3 1.999 –.531–3 –.445–5 .3890+3 2.000 –.135–1 –.204–5 .7121+3 1.471 .721–1 .101–1 .1417+4 1.473 .724–1 .101–1 .2683+2 2.000 –.690–2 .507–6
200 .1582+3 1.998 .115+0 –.472–5 .1861+3 2.000 –.139–1 –.176–5 .1911+3 1.459 .155+0 .140–1 .3794+3 1.461 .155+0 .143–1 .1019+2 2.000 –.264–1 .385–6
500 .9272+2 1.995 .336+0 –.468–5 .4678+2 1.999 .136+0 –.957–6 .2049+2 1.236 .321+0 .283–1 .4056+2 1.239 .322+0 .286–1 .1905+1 1.999 .120+0 –.130–6
1000 .4529+2 1.991 .573+0 –.415–5 .1206+2 1.996 .380+0 –.520–6 .2712+1 0.942 .460+0 .555–1 .5353+1 0.945 .461+0 .557–1 .4362+0 1.996 .370+0 –.307–6
E (eV) 1500 .2543+2 1.986 .753+0 –.348–5 .4867+1 1.992 .578+0 –.333–6 .7427+0 0.750 .532+0 .819–1 .1462+1 0.754 .532+0 .820–1 .1683+0 1.992 .567+0 .110–7
2000 .1567+2 1.981 .902+0 –.274–5 .2447+1 1.987 .742+0 –.142–6 .2840+0 0.625 .581+0 .106+0 .5583+0 0.630 .581+0 .106+0 .8216–1 1.987 .736+0 –.566–7
3000 .7148+1 1.971 .115+1 –.121–5 .8781+0 1.978 .101+1 .338–6 .6938–1 0.464 .652+0 .148+0 .1360+0 0.471 .651+0 .148+0 .2868–1 1.978 .101+1 .318–6
4000 .3824+1 1.961 .136+1 .474–6 .4098+0 1.968 .123+1 .101–5 .2462–1 0.364 .706+0 .184+0 .4814–1 0.372 .704+0 .184+0 .1319–1 1.968 .123+1 .973–6
5000 .2272+1 1.950 .153+1 .228–5 .2227+0 1.958 .143+1 .188–5 .1081–1 0.293 .756+0 .215+0 .2109–1 0.303 .751+0 .215+0 .7102–2 1.958 .142+1 .171–5
100 .1632+3 1.999 –.203–1 –.545–5
200 .1374+3 1.998 .949–1 –.577–5
500 .8683+2 1.995 .320+0 –.581–5
1000 .4615+2 1.990 .560+0 –.534–5
E (eV) 1500 .2742+2 1.986 .741+0 –.467–5
2000 .1760+2 1.981 .890+0 –.392–5
3000 .8476+1 1.971 .114+1 –.228–5
4000 .4700+1 1.961 .134+1 –.450–6
5000 .2864+1 1.950 .152+1 .154–5
Na, Z = 11 Shell 1s1/2 Eb = 1075 eV 2s1/2 Eb = 66 eV 2 p1/2 Eb = 34 eV 2 p3/2 Eb = 34 eV 3s1/2 Eb = 5 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
Mg, Z = 12 Shell 1s1/2 Eb = 1308 eV
σ β γ δ
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Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Mg, Z = 12 (continued) Shell 2s1/2 Eb = 92 eV 2 p1/2 Eb = 54 eV 2 p3/2 Eb = 54 eV 3s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3760+3 1.999 –.291–2 –.263–5 .7617+3 1.460 .633–1 .102–1 .1516+4 1.462 .635–1 .102–1 .5502+2 2.000 .473–2 –.882–6
200 .1951+3 2.000 –.233–1 –.238–5 .2346+3 1.474 .148+0 .140–1 .4659+3 1.477 .148+0 .143–1 .1971+2 2.000 –.285–1 –.104–6
500 .5454+2 1.999 .106+0 –.144–5 .2924+2 1.290 .317+0 .267–1 .5783+2 1.294 .318+0 .270–1 .3969+1 2.000 .883–1 –.138–6
1000 .1520+2 1.997 .340+0 –.816–6 .4253+1 1.017 .469+0 .513–1 .8383+1 1.021 .470+0 .515–1 .9434+0 1.997 .322+0 –.200–6
E (eV) 1500 .6387+1 1.993 .537+0 –.541–6 .1217+1 0.828 .552+0 .760–1 .2393+1 0.833 .554+0 .761–1 .3730+0 1.993 .522+0 –.148–6
2000 .3291+1 1.988 .704+0 –.324–6 .4777+0 0.696 .607+0 .992–1 .9376+0 0.701 .607+0 .993–1 .1858+0 1.989 .691+0 –.101–6
3000 .1217+1 1.979 .977+0 .195–6 .1205+0 0.524 .680+0 .140+0 .2358+0 0.531 .679+0 .141+0 .6631–1 1.979 .966+0 .318–6
4000 .5787+0 1.969 .120+1 .916–6 .4368–1 0.417 .735+0 .176+0 .8523–1 0.426 .733+0 .176+0 .3093–1 1.969 .119+1 .916–6
5000 .3188+0 1.959 .139+1 .186–5 .1948–1 0.341 .782+0 .208+0 .3792–1 0.351 .777+0 .208+0 .1684–1 1.959 .139+1 .171–5
100 .1391+3 1.998 –.400–1 –.660–5 .3581+3 1.999 .111–1 –.325–5 .7773+3 1.444 .527–1 .102–1 .1548+4 1.447 .529–1 .102–1 .9121+2 1.999 .168–1 –.118–5 .7676+2 1.568 .296–1 .602–2
200 .1197+3 1.998 .748–1 –.694–5 .1995+3 2.000 –.279–1 –.308–5 .2703+3 1.482 .138+0 .138–1 .5366+3 1.485 .139+0 .141–1 .3316+2 2.000 –.288–1 –.495–6 .2074+2 1.574 .106+0 .921–2
500 .8043+2 1.995 .303+0 –.709–5 .6154+2 2.000 .785–1 –.206–5 .3896+2 1.333 .313+0 .254–1 .7701+2 1.338 .314+0 .257–1 .6984+1 2.000 .565–1 –.755–7 .2279+1 1.372 .292+0 .206–1
1000 .4595+2 1.990 .546+0 –.668–5 .1840+2 1.997 .303+0 –.122–5 .6204+1 1.081 .474+0 .477–1 .1222+2 1.086 .476+0 .479–1 .1716+1 1.997 .284+0 –.429–6 .3087+0 1.094 .463+0 .443–1
E (eV) 1500 .2871+2 1.985 .725+0 –.600–5 .8039+1 1.993 .495+0 –.840–6 .1857+1 0.904 .568+0 .710–1 .3647+1 0.909 .570+0 .711–1 .6949+0 1.994 .479+0 –.322–6 .8689–1 0.904 .561+0 .679–1
2000 .1912+2 1.981 .877+0 –.525–5 .4246+1 1.989 .663+0 –.571–6 .7487+0 0.767 .629+0 .930–1 .1467+1 0.773 .630+0 .930–1 .3524+0 1.990 .646+0 –.156–6 .3384–1 0.767 .626+0 .901–1
3000 .9701+1 1.971 .112+1 –.351–5 .1619+1 1.980 .937+0 –.165–8 .1951+0 0.587 .709+0 .133+0 .3811+0 0.594 .709+0 .133+0 .1285+0 1.980 .928+0 .153–6 .8474–2 0.585 .703+0 .131+0
4000 .5569+1 1.961 .133+1 –.161–5 .7840+0 1.970 .117+1 .769–6 .7218–1 0.470 .765+0 .168+0 .1406+0 0.479 .763+0 .168+0 .6082–1 1.971 .115+1 .809–6 .3070–2 0.470 .760+0 .167+0
5000 .3479+1 1.950 .151+1 .516–6 .4375+0 1.960 .136+1 .177–5 .3267–1 0.388 .811+0 .199+0 .6347–1 0.398 .808+0 .199+0 .3345–1 1.961 .135+1 .170–5 .1371–2 0.387 .807+0 .198+0
Al, Z = 13 Shell 1s1/2 Eb = 1564 eV 2s1/2 Eb = 121 eV 2 p1/2 Eb = 77 eV 2 p3/2 Eb = 77 eV 3s1/2 Eb = 10 eV 3 p1/2 Eb = 6 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
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TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Si, Z = 14 Shell 1s1/2 Eb = 1844 eV 2s1/2 Eb = 154 eV 2 p1/2 Eb = 104 eV 2 p3/2 Eb = 104 eV 3s1/2 Eb = 13 eV 3 p1/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1196+3 1.998 –.621–1 –.790–5 .3362+3 1.999 .296–1 –.392–5 .7692+3 1.424 .411–1 .102–1 .1532+4 1.427 .413–1 .101–1 .1242+3 1.999 .315–1 –.130–5 .1271+3 1.566 .149–1 .493–2
200 .1049+3 1.997 .545–1 –.833–5 .1999+3 2.000 –.286–1 –.389–5 .2982+3 1.482 .127+0 .137–1 .5922+3 1.487 .128+0 .140–1 .4560+2 2.000 –.254–1 –.822–6 .3615+2 1.593 .899–1 .827–2
500 .7405+2 1.995 .285+0 –.855–5 .6760+2 2.000 .530–1 –.283–5 .4935+2 1.369 .308+0 .243–1 .9750+2 1.374 .309+0 .247–1 .9892+1 2.000 .313–1 –.351–6 .4368+1 1.415 .275+0 .185–1
1000 .4500+2 1.990 .530+0 –.820–5 .2158+2 1.998 .267+0 –.177–5 .8553+1 1.139 .477+0 .447–1 .1682+2 1.145 .479+0 .450–1 .2525+1 1.998 .244+0 –.443–6 .6291+0 1.157 .462+0 .401–1
E (eV) 1500 .2941+2 1.985 .711+0 –.752–5 .9777+1 1.994 .455+0 –.125–5 .2675+1 0.968 .580+0 .665–1 .5247+1 0.975 .582+0 .665–1 .1042+1 1.995 .435+0 –.532–6 .1822+0 0.971 .565+0 .622–1
2000 .2026+2 1.980 .863+0 –.676–5 .5290+1 1.990 .621+0 –.912–6 .1109+1 0.834 .648+0 .874–1 .2170+1 0.841 .650+0 .874–1 .5367+0 1.991 .601+0 –.416–6 .7246–1 0.835 .635+0 .836–1
3000 .1079+2 1.970 .111+1 –.497–5 .2078+1 1.981 .897+0 –.276–6 .2986+0 0.650 .737+0 .127+0 .5821+0 0.657 .737+0 .126+0 .2001+0 1.982 .882+0 .406–7 .1863–1 0.646 .730+0 .123+0
4000 .6402+1 1.960 .132+1 –.294–5 .1025+1 1.971 .113+1 .545–6 .1127+0 0.525 .795+0 .161+0 .2190+0 0.534 .794+0 .161+0 .9598–1 1.972 .111+1 .687–6 .6854–2 0.522 .789+0 .159+0
5000 .4097+1 1.950 .150+1 –.659–6 .5795+0 1.962 .132+1 .161–5 .5173–1 0.437 .841+0 .192+0 .1003+0 0.447 .838+0 .192+0 .5332–1 1.962 .131+1 .162–5 .3098–2 0.432 .835+0 .190+0
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1036+3 1.998 –.865–1 –.937–5 .3122+3 1.999 .526–1 –.465–5 .7396+3 1.401 .289–1 .103–1 .1480+4 1.404 .289–1 .101–1
200 .9251+2 1.997 .333–1 –.993–5 .1969+3 1.999 –.254–1 –.480–5 .3173+3 1.478 .115+0 .137–1 .6319+3 1.483 .116+0 .139–1
500 .6793+2 1.994 .266+0 –.102–4 .7257+2 2.000 .298–1 –.376–5 .5983+2 1.397 .302+0 .234–1 .1183+3 1.403 .303+0 .238–1
1000 .4354+2 1.990 .514+0 –.992–5 .2465+2 1.998 .232+0 –.249–5 .1126+2 1.190 .480+0 .423–1 .2214+2 1.197 .482+0 .425–1
E (eV) 1500 .2960+2 1.985 .697+0 –.926–5 .1155+2 1.995 .417+0 –.180–5 .3673+1 1.027 .589+0 .626–1 .7198+1 1.034 .592+0 .626–1
2000 .2104+2 1.980 .850+0 –.850–5 .6396+1 1.991 .581+0 –.137–5 .1565+1 0.895 .664+0 .823–1 .3058+1 0.903 .666+0 .822–1
3000 .1172+2 1.970 .110+1 –.665–5 .2588+1 1.982 .857+0 –.646–6 .4356+0 0.710 .762+0 .120+0 .8479+0 0.718 .764+0 .120+0
4000 .7175+1 1.960 .130+1 –.453–5 .1301+1 1.973 .109+1 .230–6 .1677+0 0.581 .825+0 .154+0 .3253+0 0.590 .825+0 .154+0
5000 .4701+1 1.950 .149+1 –.216–5 .7447+0 1.963 .129+1 .136–5 .7810–1 0.486 .873+0 .184+0 .1511+0 0.497 .871+0 .184+0
P, Z = 15 Shell 1s1/2 Eb = 2148 eV 2s1/2 Eb = 191 eV 2 p1/2 Eb = 136 eV 2 p3/2 Eb = 135 eV
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Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables P, Z = 15 (continued) Shell 3s1/2 Eb = 16 eV 3 p1/2 Eb = 10 eV 3 p3/2 Eb = 10 eV
σ β γ δ σ β γ δ σ β γ δ
100 .1547+3 1.999 .481–1 –.149–5 .1768+3 1.555 .147–2 .379–2 .3525+3 1.555 .169–2 .377–2
200 .5819+2 1.999 –.194–1 –.107–5 .5329+2 1.606 .724–1 .732–2 .1057+3 1.609 .728–1 .740–2
500 .1289+2 2.000 .112–1 –.787–6 .6948+1 1.452 .257+0 .168–1 .1370+2 1.458 .259+0 .168–1
1000 .3410+1 1.998 .204+0 –.559–6 .1067+1 1.211 .454+0 .359–1 .2093+1 1.218 .456+0 .357–1
E (eV) 1500 .1433+1 1.995 .393+0 –.709–6 .3167+0 1.032 .567+0 .572–1 .6192+0 1.038 .569+0 .568–1
2000 .7473+0 1.992 .559+0 –.717–6 .1282+0 0.897 .643+0 .780–1 .2501+0 0.904 .645+0 .776–1
3000 .2843+0 1.983 .836+0 –.227–6 .3389–1 0.707 .748+0 .116+0 .6584–1 0.715 .749+0 .115+0
4000 .1382+0 1.974 .107+1 .463–6 .1266–1 0.576 .815+0 .150+0 .2452–1 0.585 .815+0 .150+0
5000 .7751–1 1.964 .127+1 .141–5 .5787–2 0.482 .863+0 .181+0 .1117–1 0.493 .861+0 .181+0
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .9033+2 1.998 –.113+0 –.110–4 .2880+3 1.998 .797–1 –.542–5 .7044+3 1.377 .157–1 .102–1 .1414+4 1.380 .157–1 .992–2 .1807+3 1.999 .662–1 –.175–5 .2268+3 1.536 –.895–2 .253–2 .4528+3 1.536 –.878–2 .249–2
200 .8194+2 1.997 .106–1 –.117–4 .1914+3 1.999 –.178–1 –.580–5 .3306+3 1.470 .101+0 .136–1 .6600+3 1.475 .101+0 .137–1 .7056+2 1.999 –.108–1 –.141–5 .7261+2 1.615 .538–1 .632–2 .1441+3 1.618 .543–1 .642–2
500 .6225+2 1.994 .246+0 –.121–4 .7643+2 2.000 .940–2 –.483–5 .7020+2 1.419 .293+0 .227–1 .1390+3 1.426 .294+0 .231–1 .1601+2 2.000 –.507–2 –.128–5 .1006+2 1.486 .239+0 .152–1 .1982+2 1.492 .240+0 .153–1
1000 .4176+2 1.989 .497+0 –.119–4 .2756+2 1.998 .198+0 –.339–5 .1431+2 1.235 .481+0 .401–1 .2813+2 1.242 .483+0 .403–1 .4362+1 1.999 .167+0 –.912–6 .1636+1 1.261 .442+0 .328–1 .3204+1 1.268 .445+0 .326–1
E (eV) 1500 .2940+2 1.984 .682+0 –.112–4 .1333+2 1.995 .379+0 –.253–5 .4853+1 1.079 .596+0 .591–1 .9505+1 1.087 .599+0 .591–1 .1870+1 1.996 .352+0 –.954–6 .4987+0 1.088 .569+0 .524–1 .9736+0 1.095 .572+0 .521–1
2000 .2149+2 1.980 .836+0 –.105–4 .7543+1 1.992 .541+0 –.197–5 .2122+1 0.951 .676+0 .777–1 .4144+1 0.960 .679+0 .776–1 .9869+0 1.992 .516+0 –.920–6 .2053+0 0.955 .654+0 .720–1 .3997+0 0.962 .657+0 .716–1
3000 .1248+2 1.970 .108+1 –.859–5 .3142+1 1.983 .816+0 –.113–5 .6110+0 0.766 .784+0 .114+0 .1187+1 0.775 .786+0 .113+0 .3818+0 1.984 .793+0 –.593–6 .5551–1 0.764 .763+0 .109+0 .1076+0 0.773 .765+0 .109+0
4000 .7871+1 1.960 .129+1 –.639–5 .1608+1 1.974 .105+1 –.194–6 .2400+0 0.635 .854+0 .147+0 .4647+0 0.644 .854+0 .147+0 .1881+0 1.975 .103+1 .142–6 .2108–1 0.630 .838+0 .143+0 .4073–1 0.640 .838+0 .142+0
5000 .5274+1 1.950 .147+1 –.390–5 .9324+0 1.964 .125+1 .993–6 .1133+0 0.535 .904+0 .177+0 .2187+0 0.546 .902+0 .176+0 .1065+0 1.965 .123+1 .120–5 .9739–2 0.531 .891+0 .173+0 .1875–1 0.542 .890+0 .173+0
S, Z = 16 Shell 1s1/2 Eb = 2476 eV 2s1/2 Eb = 232 eV 2 p1/2 Eb = 170 eV 2 p3/2 Eb = 168 eV 3s1/2 Eb = 20 eV 3 p1/2 Eb = 10 eV 3 p3/2 Eb = 10 eV
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TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Cl, Z = 17 Shell 1s1/2 Eb = 2829 eV 2s1/2 Eb = 277 eV 2 p1/2 Eb = 208 eV 2 p3/2 Eb = 206 eV 3s1/2 Eb = 24 eV 3 p1/2 Eb = 13 eV 3 p3/2 Eb = 13 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .7925+2 1.997 –.141+0 –.129–4 .2647+3 1.998 .111+0 –.624–5 .6620+3 1.351 .179–2 .100–1 .1328+4 1.354 .173–2 .971–2 .2028+3 1.999 .847–1 –.204–5 .2653+3 1.510 –.154–1 .131–2 .5302+3 1.509 –.154–1 .126–2
200 .7286+2 1.996 –.138–1 –.138–4 .1840+3 1.999 –.603–2 –.689–5 .3367+3 1.459 .861–1 .135–1 .6721+3 1.465 .864–1 .136–1 .8262+2 1.999 .692–3 –.185–5 .9195+2 1.617 .365–1 .542–2 .1825+3 1.620 .369–1 .553–2
500 .5704+2 1.994 .224+0 –.143–4 .7919+2 2.000 –.782–2 –.604–5 .7995+2 1.436 .282+0 .222–1 .1582+3 1.444 .284+0 .225–1 .1932+2 2.000 –.186–1 –.178–5 .1365+2 1.515 .222+0 .137–1 .2688+2 1.522 .223+0 .138–1
1000 .3978+2 1.989 .481+0 –.141–4 .3024+2 1.999 .166+0 –.450–5 .1761+2 1.272 .480+0 .383–1 .3460+2 1.281 .482+0 .385–1 .5381+1 1.999 .134+0 –.143–5 .2338+1 1.304 .431+0 .300–1 .4573+1 1.313 .434+0 .298–1
E (eV) 1500 .2889+2 1.984 .667+0 –.135–4 .1509+2 1.996 .343+0 –.346–5 .6208+1 1.126 .602+0 .560–1 .1214+2 1.135 .605+0 .560–1 .2350+1 1.997 .309+0 –.124–5 .7346+0 1.139 .569+0 .478–1 .1432+1 1.148 .572+0 .475–1
2000 .2165+2 1.979 .821+0 –.127–4 .8712+1 1.992 .503+0 –.277–5 .2783+1 1.003 .687+0 .736–1 .5424+1 1.012 .690+0 .734–1 .1255+1 1.993 .472+0 –.121–5 .3073+0 1.009 .659+0 .664–1 .5970+0 1.017 .662+0 .659–1
3000 .1307+2 1.969 .107+1 –.108–4 .3730+1 1.984 .776+0 –.176–5 .8278+0 0.820 .803+0 .108+0 .1606+1 0.830 .806+0 .108+0 .4932+0 1.985 .749+0 –.955–6 .8480–1 0.819 .779+0 .102+0 .1640+0 0.828 .782+0 .102+0
4000 .8477+1 1.960 .128+1 –.854–5 .1943+1 1.975 .101+1 –.753–6 .3319+0 0.685 .879+0 .140+0 .6412+0 0.696 .881+0 .140+0 .2457+0 1.976 .983+0 –.242–6 .3272–1 0.683 .859+0 .135+0 .6304–1 0.693 .860+0 .134+0
5000 .5804+1 1.950 .146+1 –.594–5 .1141+1 1.966 .121+1 .500–6 .1589+0 0.583 .933+0 .170+0 .3060+0 0.595 .933+0 .169+0 .1404+0 1.967 .119+1 .811–6 .1528–1 0.580 .917+0 .165+0 .2935–1 0.591 .916+0 .164+0
100 .6998+2 1.997 –.171+0 –.151–4 .2430+3 1.997 .145+0 –.711–5 .6149+3 1.325 –.129–1 .975–2
200 .6506+2 1.996 –.398–1 –.162–4 .1755+3 1.998 .991–2 –.810–5 .3361+3 1.446 .707–1 .135–1
500 .5231+2 1.993 .203+0 –.168–4 .8094+2 2.000 –.217–1 –.743–5 .8871+2 1.447 .270+0 .217–1
1000 .3771+2 1.988 .462+0 –.167–4 .3264+2 1.999 .134+0 –.581–5 .2108+2 1.305 .477+0 .367–1
E (eV) 1500 .2816+2 1.984 .650+0 –.161–4 .1679+2 1.996 .306+0 –.464–5 .7718+1 1.167 .606+0 .531–1
2000 .2159+2 1.979 .806+0 –.153–4 .9885+1 1.993 .464+0 –.379–5 .3544+1 1.050 .696+0 .699–1
3000 .1350+2 1.969 .106+1 –.133–4 .4343+1 1.985 .736+0 –.257–5 .1088+1 0.871 .820+0 .103+0
4000 .8991+1 1.959 .127+1 –.110–4 .2303+1 1.977 .968+0 –.146–5 .4453+0 0.736 .902+0 .134+0
5000 .6283+1 1.949 .145+1 –.831–5 .1370+1 1.967 .117+1 –.143–6 .2163+0 0.631 .961+0 .163+0
Ar, Z = 18 Shell 1s1/2 Eb = 3206 eV 2s1/2 Eb = 326 eV 2 p1/2 Eb = 251 eV
σ β γ δ σ β γ δ σ β γ δ
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Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Ar, Z = 18 (continued) Shell 2 p3/2 Eb = 248 eV 3s1/2 Eb = 29 eV 3 p1/2 Eb = 16 eV 3 p3/2 Eb = 16 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1237+4 1.328 –.130–1 .936–2 .2191+3 1.999 .104+0 –.236–5 .2958+3 1.479 –.170–1 .111–3 .5921+3 1.478 –.171–1 .290–4
200 .6721+3 1.452 .708–1 .135–1 .9369+2 1.999 .148–1 –.240–5 .1114+3 1.615 .201–1 .449–2 .2212+3 1.617 .206–1 .461–2
500 .1757+3 1.456 .271+0 .221–1 .2275+2 2.000 –.296–1 –.220–5 .1777+2 1.541 .202+0 .122–1 .3497+2 1.548 .204+0 .123–1
1000 .4140+2 1.315 .480+0 .370–1 .6457+1 1.999 .103+0 –.194–5 .3184+1 1.344 .417+0 .272–1 .6220+1 1.353 .420+0 .271–1
E (eV) 1500 .1508+2 1.178 .610+0 .531–1 .2866+1 1.997 .268+0 –.169–5 .1029+1 1.187 .561+0 .437–1 .2002+1 1.196 .564+0 .433–1
2000 .6900+1 1.060 .700+0 .697–1 .1549+1 1.994 .429+0 –.169–5 .4374+0 1.059 .660+0 .615–1 .8481+0 1.069 .664+0 .610–1
3000 .2107+1 0.881 .824+0 .103+0 .6181+0 1.986 .706+0 –.145–5 .1231+0 0.870 .790+0 .961–1 .2376+0 0.881 .794+0 .954–1
4000 .8585+0 0.747 .905+0 .133+0 .3112+0 1.978 .940+0 –.788–6 .4818–1 0.733 .875+0 .128+0 .9258–1 0.744 .877+0 .127+0
5000 .4155+0 0.643 .962+0 .162+0 .1794+0 1.969 .115+1 .352–6 .2277–1 0.629 .939+0 .157+0 .4360–1 0.640 .940+0 .157+0
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .6192+2 1.996 –.193+0 –.178–4 .2204+3 1.997 .164+0 –.813–5 .5511+3 1.312 –.235–1 .942–2 .1107+4 1.316 –.238–1 .905–2 .2371+3 1.999 .112+0 –.286–5 .3549+3 1.467 –.136–1 –.280–3
200 .5806+2 1.995 –.597–1 –.190–4 .1645+3 1.998 .235–1 –.934–5 .3217+3 1.435 .587–1 .134–1 .6428+3 1.442 .589–1 .134–1 .1065+3 1.999 .255–1 –.283–5 .1413+3 1.614 .895–2 .365–2
500 .4781+2 1.993 .186+0 –.197–4 .8098+2 2.000 –.307–1 –.893–5 .9455+2 1.454 .258+0 .214–1 .1871+3 1.464 .260+0 .217–1 .2709+2 2.000 –.360–1 –.262–5 .2426+2 1.560 .181+0 .108–1
1000 .3551+2 1.988 .446+0 –.195–4 .3449+2 1.999 .107+0 –.728–5 .2431+2 1.331 .472+0 .356–1 .4769+2 1.342 .476+0 .358–1 .7881+1 2.000 .767–1 –.253–5 .4560+1 1.378 .401+0 .249–1
E (eV) 1500 .2717+2 1.983 .637+0 –.189–4 .1829+2 1.997 .273+0 –.600–5 .9274+1 1.202 .607+0 .508–1 .1810+2 1.214 .612+0 .508–1 .3556+1 1.998 .233+0 –.236–5 .1518+1 1.226 .549+0 .402–1
2000 .2127+2 1.978 .790+0 –.182–4 .1099+2 1.994 .427+0 –.504–5 .4368+1 1.093 .704+0 .667–1 .8492+1 1.105 .709+0 .664–1 .1948+1 1.995 .386+0 –.227–5 .6585+0 1.106 .658+0 .568–1
3000 .1374+2 1.969 .104+1 –.162–4 .4958+1 1.986 .697+0 –.358–5 .1386+1 0.917 .834+0 .984–1 .2678+1 0.929 .839+0 .979–1 .7904+0 1.988 .663+0 –.199–5 .1896+0 0.918 .801+0 .900–1
4000 .9386+1 1.959 .125+1 –.138–4 .2676+1 1.978 .929+0 –.231–5 .5794+0 0.783 .922+0 .128+0 .1114+1 0.795 .926+0 .128+0 .4022+0 1.979 .898+0 –.135–5 .7522–1 0.780 .891+0 .121+0
5000 .6689+1 1.949 .143+1 –.110–4 .1612+1 1.969 .113+1 –.941–6 .2857+0 0.677 .986+0 .156+0 .5475+0 0.690 .988+0 .156+0 .2337+0 1.970 .110+1 –.307–6 .3594–1 0.673 .957+0 .150+0
K, Z = 19 Shell 1s1/2 Eb = 3611 eV 2s1/2 Eb = 381 eV 2 p1/2 Eb = 299 eV 2 p3/2 Eb = 296 eV 3s1/2 Eb = 37 eV 3 p1/2 Eb = 19 eV
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Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables K, Z = 19 (continued) Shell 3 p3/2 Eb = 19 eV 4s1/2 Eb = 4 eV
σ β γ δ σ β γ δ
100 .7126+3 1.466 –.138–1 –.407–3 .2033+2 1.999 .120+0 .105–5
200 .2813+3 1.616 .932–2 .378–2 .7321+1 1.999 .345–1 –.190–5
500 .4781+2 1.567 .183+0 .110–1 .1561+1 2.000 –.382–1 –.206–5
1000 .8918+1 1.388 .404+0 .248–1 .4201+0 2.000 .731–1 –.202–5
E (eV) 1500 .2954+1 1.237 .553+0 .399–1 .1845+0 1.998 .228+0 –.229–5
2000 .1277+1 1.116 .663+0 .562–1 .9966–1 1.995 .381+0 –.185–5
3000 .3658+0 0.930 .805+0 .892–1 .3982–1 1.988 .661+0 –.179–5
4000 .1445+0 0.792 .894+0 .120+0 .2010–1 1.979 .896+0 –.120–5
5000 .6877–1 0.686 .959+0 .149+0 .1162–1 1.970 .110+1 –.276–6
100 .5510+2 1.996 –.214+0 –.207–4 .1999+3 1.996 .181+0 –.919–5 .4914+3 1.303 –.350–1 .892–2 .9887+3 1.307 –.353–1 .855–2 .2537+3 1.998 .121+0 –.337–5 .3906+3 1.459 –.956–2 –.495–3 .7859+3 1.458 –.997–2 –.661–3 .3611+2 1.999 .121+0 –.720–6
200 .5205+2 1.995 –.800–1 –.221–4 .1537+3 1.998 .379–1 –.107–4 .3039+3 1.425 .464–1 .132–1 .6080+3 1.433 .464–1 .132–1 .1185+3 1.998 .363–1 –.359–5 .1646+3 1.610 .559–3 .307–2 .3282+3 1.613 .857–3 .320–2 .1376+2 1.998 .462–1 –.709–6
500 .4374+2 1.992 .169+0 –.230–4 .8020+2 2.000 –.370–1 –.106–4 .9874+2 1.458 .246+0 .211–1 .1955+3 1.469 .248+0 .214–1 .3156+2 1.999 –.398–1 –.330–5 .3074+2 1.576 .163+0 .970–2 .6062+2 1.584 .165+0 .988–2 .2940+1 1.999 –.414–1 –.234–5
1000 .3335+2 1.987 .430+0 –.228–4 .3599+2 1.999 .819–1 –.901–5 .2739+2 1.352 .466+0 .343–1 .5373+2 1.364 .469+0 .346–1 .9413+1 2.000 .540–1 –.329–5 .6080+1 1.407 .386+0 .227–1 .1189+2 1.418 .390+0 .226–1 .8008+0 2.000 .480–1 –.222–5
E (eV) 1500 .2609+2 1.983 .622+0 –.222–4 .1966+2 1.997 .239+0 –.762–5 .1089+2 1.235 .608+0 .488–1 .2124+2 1.247 .613+0 .488–1 .4308+1 1.998 .199+0 –.315–5 .2084+1 1.264 .539+0 .374–1 .4054+1 1.276 .544+0 .371–1 .3544+0 1.998 .193+0 –.267–5
2000 .2081+2 1.978 .777+0 –.215–4 .1205+2 1.994 .391+0 –.656–5 .5264+1 1.129 .709+0 .636–1 .1022+2 1.142 .715+0 .634–1 .2388+1 1.996 .347+0 –.301–5 .9227+0 1.145 .653+0 .526–1 .1788+1 1.157 .659+0 .520–1 .1930+0 1.996 .341+0 –.276–5
3000 .1386+2 1.968 .103+1 –.194–4 .5579+1 1.987 .659+0 –.486–5 .1724+1 0.960 .848+0 .942–1 .3326+1 0.973 .854+0 .935–1 .9854+0 1.989 .619+0 –.268–5 .2722+0 0.963 .808+0 .843–1 .5245+0 0.975 .814+0 .834–1 .7820–1 1.989 .615+0 –.242–5
4000 .9687+1 1.958 .124+1 –.169–4 .3062+1 1.979 .889+0 –.343–5 .7361+0 0.827 .940+0 .123+0 .1413+1 0.841 .945+0 .122+0 .5067+0 1.981 .854+0 –.207–5 .1095+0 0.825 .906+0 .115+0 .2101+0 0.838 .910+0 .114+0 .3983–1 1.981 .852+0 –.186–5
5000 .7033+1 1.948 .142+1 –.140–4 .1868+1 1.970 .109+1 –.189–5 .3686+0 0.719 .101+1 .150+0 .7047+0 0.734 .101+1 .149+0 .2966+0 1.972 .106+1 –.100–5 .5287–1 0.716 .975+0 .143+0 .1010+0 0.729 .978+0 .142+0 .2318–1 1.972 .106+1 –.802–6
Ca, Z = 20 Shell 1s1/2 Eb = 4041 eV 2s1/2 Eb = 441 eV 2 p1/2 Eb = 353 eV 2 p3/2 Eb = 349 eV 3s1/2 Eb = 46 eV 3 p1/2 Eb = 28 eV 3 p3/2 Eb = 28 eV 4s1/2 Eb = 6 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
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M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Sc, Z = 21 Shell 1s1/2 Eb = 4494 eV 2s1/2 Eb = 503 eV 2 p1/2 Eb = 408 eV 2 p3/2 Eb = 403 eV 3s1/2 Eb = 55 eV 3 p1/2 Eb = 33 eV 3 p3/2 Eb = 33 eV 3d3/2 Eb = 8 eV 4s1/2 Eb = 6 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .4945+2 1.995 –.245+0 –.242–4 .1838+3 1.996 .214+0 –.104–4 .4514+3 1.282 –.498–1 .819–2 .9095+3 1.287 –.503–1 .780–2 .2580+3 1.998 .138+0 –.387–5 .4065+3 1.429 –.732–3 –.859–3 .8196+3 1.428 –.143–2 –.109–2 .8991+3 1.178 .556–1 .181–1 .4017+2 1.999 .131+0 –.101–5
200 .4699+2 1.994 –.108+0 –.258–4 .1448+3 1.997 .594–1 –.123–4 .2924+3 1.411 .302–1 .129–1 .5858+3 1.419 .301–1 .129–1 .1262+3 1.998 .525–1 –.439–5 .1823+3 1.600 –.837–2 .229–2 .3639+3 1.603 –.821–2 .241–2 .1578+3 1.275 .143+0 .274–1 .1544+2 1.998 .616–1 –.655–6
500 .4018+2 1.992 .148+0 –.268–4 .7949+2 1.999 –.416–1 –.126–4 .1035+3 1.460 .231+0 .207–1 .2051+3 1.472 .232+0 .210–1 .3521+2 1.999 –.420–1 –.411–5 .3664+2 1.589 .142+0 .858–2 .7226+2 1.598 .143+0 .881–2 .1026+2 1.090 .314+0 .514–1 .3391+1 1.999 –.429–1 –.270–5
1000 .3137+2 1.987 .411+0 –.267–4 .3740+2 2.000 .574–1 –.110–4 .3072+2 1.371 .456+0 .333–1 .6026+2 1.385 .460+0 .335–1 .1076+2 2.000 .314–1 –.415–5 .7560+1 1.435 .368+0 .205–1 .1477+2 1.447 .372+0 .205–1 .9582+0 0.821 .457+0 .935–1 .9326+0 2.000 .264–1 –.320–5
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E (eV) 1500 .2501+2 1.982 .605+0 –.260–4 .2100+2 1.998 .206+0 –.955–5 .1268+2 1.263 .605+0 .469–1 .2470+2 1.278 .611+0 .469–1 .4983+1 1.999 .167+0 –.408–5 .2651+1 1.299 .527+0 .344–1 .5151+1 1.312 .532+0 .341–1 .2126+0 0.666 .547+0 .134+0 .4155+0 1.999 .161+0 –.323–5
2000 .2029+2 1.977 .761+0 –.252–4 .1312+2 1.995 .354+0 –.838–5 .6277+1 1.164 .712+0 .609–1 .1218+2 1.178 .719+0 .606–1 .2789+1 1.996 .308+0 –.395–5 .1194+1 1.185 .645+0 .487–1 .2310+1 1.198 .651+0 .482–1 .6890–1 0.562 .611+0 .171+0 .2279+0 1.996 .302+0 –.354–5
3000 .1389+2 1.968 .102+1 –.231–4 .6223+1 1.988 .620+0 –.647–5 .2118+1 1.000 .860+0 .901–1 .4080+1 1.015 .867+0 .894–1 .1168+1 1.990 .575+0 –.357–5 .3602+0 1.007 .812+0 .790–1 .6926+0 1.021 .819+0 .781–1 .1308–1 0.418 .671+0 .237+0 .9350–1 1.990 .571+0 –.324–5
4000 .9918+1 1.958 .123+1 –.205–4 .3470+1 1.980 .850+0 –.485–5 .9218+0 0.869 .958+0 .118+0 .1766+1 0.884 .964+0 .117+0 .6068+0 1.982 .810+0 –.295–5 .1468+0 0.870 .919+0 .108+0 .2809+0 0.883 .925+0 .107+0 .3893–2 0.336 .686+0 .294+0 .4803–1 1.982 .808+0 –.272–5
5000 .7328+1 1.948 .141+1 –.176–4 .2142+1 1.971 .105+1 –.316–5 .4681+0 0.762 .103+1 .144+0 .8928+0 0.777 .103+1 .143+0 .3578+0 1.973 .102+1 –.189–5 .7152–1 0.759 .993+0 .136+0 .1363+0 0.773 .997+0 .134+0 .1504–2 0.286 .697+0 .344+0 .2813–1 1.973 .101+1 –.177–5
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Ti, Z = 22 Shell 1s1/2 Eb = 4970 eV 2s1/2 Eb = 567 eV 2 p1/2 Eb = 465 eV 2 p3/2 Eb = 459 eV 3s1/2 Eb = 64 eV 3 p1/2 Eb = 39 eV 3 p3/2 Eb = 38 eV 3d3/2 Eb = 8 eV 4s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .4464+2 1.995 –.277+0 –.282–4 .1699+3 1.995 .248+0 –.116–4 .4171+3 1.260 –.645–1 .733–2 .8412+3 1.265 –.651–1 .692–2 .2592+3 1.998 .155+0 –.434–5 .4115+3 1.396 .119–1 –.881–3 .8377+3 1.394 .108–1 –.118–2 .1193+4 1.131 .448–1 .171–1 .4275+2 1.998 .142+0 –.122–5
200 .4263+2 1.994 –.137+0 –.300–4 .1366+3 1.997 .836–1 –.140–4 .2811+3 1.395 .131–1 .125–1 .5637+3 1.404 .128–1 .125–1 .1323+3 1.998 .701–1 –.525–5 .1963+3 1.587 –.144–1 .155–2 .3941+3 1.590 –.143–1 .165–2 .2235+3 1.264 .128+0 .265–1 .1656+2 1.998 .774–1 –.594–6
500 .3700+2 1.991 .124+0 –.312–4 .7846+2 1.999 –.430–1 –.148–4 .1075+3 1.460 .214+0 .204–1 .2131+3 1.473 .216+0 .207–1 .3866+2 1.999 –.413–1 –.507–5 .4256+2 1.600 .120+0 .758–2 .8409+2 1.609 .121+0 .785–2 .1538+2 1.124 .308+0 .493–1 .3752+1 1.999 –.411–1 –.304–5
1000 .2950+2 1.986 .391+0 –.311–4 .3857+2 2.000 .349–1 –.133–4 .3400+2 1.387 .445+0 .323–1 .6667+2 1.402 .449+0 .325–1 .1211+2 2.000 .109–1 –.514–5 .9165+1 1.461 .349+0 .186–1 .1791+2 1.474 .352+0 .186–1 .1490+1 0.863 .460+0 .892–1 .1047+1 2.000 .603–2 –.407–5
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E (eV) 1500 .2393+2 1.981 .586+0 –.304–4 .2223+2 1.998 .174+0 –.118–4 .1453+2 1.289 .600+0 .452–1 .2830+2 1.304 .606+0 .451–1 .5673+1 1.999 .135+0 –.516–5 .3285+1 1.331 .512+0 .316–1 .6378+1 1.345 .518+0 .313–1 .3383+0 0.705 .552+0 .128+0 .4694+0 1.999 .130+0 –.432–5
2000 .1970+2 1.977 .744+0 –.295–4 .1414+2 1.996 .317+0 –.105–4 .7366+1 1.196 .712+0 .584–1 .1427+2 1.212 .720+0 .581–1 .3203+1 1.997 .271+0 –.507–5 .1503+1 1.222 .636+0 .452–1 .2904+1 1.236 .642+0 .446–1 .1118+0 0.600 .620+0 .165+0 .2590+0 1.997 .265+0 –.434–5
3000 .1383+2 1.967 .100+1 –.273–4 .6868+1 1.989 .580+0 –.841–5 .2560+1 1.038 .869+0 .863–1 .4923+1 1.054 .877+0 .855–1 .1360+1 1.991 .531+0 –.468–5 .4633+0 1.048 .812+0 .740–1 .8892+0 1.063 .820+0 .730–1 .2171–1 0.452 .695+0 .230+0 .1074+0 1.991 .525+0 –.439–5
4000 .1008+2 1.957 .121+1 –.247–4 .3889+1 1.981 .810+0 –.660–5 .1135+1 0.909 .973+0 .113+0 .2170+1 0.926 .981+0 .112+0 .7134+0 1.983 .765+0 –.404–5 .1914+0 0.912 .928+0 .102+0 .3654+0 0.927 .935+0 .101+0 .6512–2 0.359 .720+0 .287+0 .5567–1 1.983 .762+0 –.371–5
5000 .7566+1 1.947 .140+1 –.216–4 .2427+1 1.973 .102+1 –.475–5 .5840+0 0.802 .105+1 .139+0 .1111+1 0.818 .106+1 .137+0 .4236+0 1.975 .975+0 –.297–5 .9409–1 0.800 .101+1 .129+0 .1788+0 0.816 .101+1 .127+0 .2524–2 0.301 .729+0 .336+0 .3280–1 1.975 .969+0 –.267–5
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables V, Z = 23 Shell 1s1/2 Eb = 5470 eV 2s1/2 Eb = 633 eV 2 p1/2 Eb = 525 eV 2 p3/2 Eb = 518 eV 3s1/2 Eb = 72 eV 3 p1/2 Eb = 44 eV 3 p3/2 Eb = 43 eV 3d3/2 Eb = 8 eV 4s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .4049+2 1.994 –.310+0 –.328–4 .1578+3 1.994 .283+0 –.129–4 .3863+3 1.238 –.786–1 .639–2 .7800+3 1.243 –.794–1 .597–2 .2598+3 1.998 .172+0 –.470–5 .4136+3 1.361 .278–1 –.451–3 .8439+3 1.358 .262–1 –.838–3 .1499+4 1.083 .361–1 .162–1 .4499+2 1.998 .151+0 –.120–5
200 .3883+2 1.993 –.167+0 –.348–4 .1291+3 1.996 .110+0 –.158–4 .2695+3 1.380 –.456–2 .119–1 .5410+3 1.389 –.502–2 .119–1 .1375+3 1.998 .882–1 –.612–5 .2086+3 1.572 –.168–1 .886–3 .4193+3 1.574 –.171–1 .959–3 .3002+3 1.247 .112+0 .256–1 .1747+2 1.998 .927–1 –.682–6
500 .3413+2 1.990 .993–1 –.362–4 .7718+2 1.999 –.414–1 –.173–4 .1105+3 1.459 .196+0 .201–1 .2193+3 1.472 .198+0 .204–1 .4198+2 1.999 –.378–1 –.618–5 .4857+2 1.608 .981–1 .666–2 .9597+2 1.617 .996–1 .698–2 .2191+2 1.153 .298+0 .474–1 .4063+1 1.999 –.359–1 –.346–5
1000 .2773+2 1.986 .371+0 –.361–4 .3950+2 2.000 .147–1 –.159–4 .3714+2 1.400 .431+0 .314–1 .7282+2 1.416 .436+0 .316–1 .1348+2 2.000 –.726–2 –.630–5 .1091+2 1.484 .327+0 .167–1 .2130+2 1.497 .331+0 .168–1 .2195+1 0.903 .462+0 .853–1 .1152+1 2.000 –.128–1 –.485–5
119
E (eV) 1500 .2285+2 1.981 .568+0 –.353–4 .2334+2 1.999 .144+0 –.144–4 .1642+2 1.311 .592+0 .436–1 .3196+2 1.328 .599+0 .436–1 .6384+1 1.999 .106+0 –.642–5 .3991+1 1.361 .496+0 .290–1 .7739+1 1.376 .502+0 .287–1 .5086+0 0.742 .558+0 .123+0 .5199+0 1.999 .992–1 –.531–5
2000 .1907+2 1.976 .726+0 –.344–4 .1510+2 1.996 .281+0 –.130–4 .8516+1 1.225 .710+0 .562–1 .1649+2 1.242 .719+0 .559–1 .3632+1 1.997 .235+0 –.639–5 .1853+1 1.256 .624+0 .419–1 .3574+1 1.272 .631+0 .414–1 .1709+0 0.636 .627+0 .158+0 .2883+0 1.997 .227+0 –.552–5
3000 .1369+2 1.966 .986+0 –.321–4 .7508+1 1.990 .540+0 –.107–4 .3047+1 1.073 .876+0 .828–1 .5850+1 1.090 .886+0 .819–1 .1562+1 1.992 .488+0 –.602–5 .5830+0 1.087 .809+0 .693–1 .1116+1 1.103 .818+0 .683–1 .3401–1 0.485 .714+0 .222+0 .1207+0 1.992 .482+0 –.547–5
4000 .1016+2 1.957 .120+1 –.294–4 .4316+1 1.982 .769+0 –.873–5 .1375+1 0.947 .987+0 .109+0 .2624+1 0.965 .996+0 .108+0 .8268+0 1.985 .720+0 –.538–5 .2441+0 0.952 .934+0 .964–1 .4648+0 0.968 .943+0 .950–1 .1031–1 0.387 .751+0 .279+0 .6304–1 1.985 .715+0 –.506–5
5000 .7751+1 1.947 .138+1 –.262–4 .2723+1 1.974 .975+0 –.671–5 .7170+0 0.840 .107+1 .133+0 .1361+1 0.858 .108+1 .132+0 .4943+0 1.976 .930+0 –.430–5 .1211+0 0.841 .102+1 .122+0 .2295+0 0.857 .103+1 .121+0 .4012–2 0.319 .762+0 .328+0 .3738–1 1.977 .923+0 –.403–5
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Cr, Z = 24 Shell 1s1/2 Eb = 5995 eV 2s1/2 Eb = 702 eV 2 p1/2 Eb = 589 eV 2 p3/2 Eb = 580 eV 3s1/2 Eb = 80 eV 3 p1/2 Eb = 49 eV 3 p3/2 Eb = 48 eV 3d3/2 Eb = 8 eV 3d5/2 Eb = 8 eV 4s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3691+2 1.994 –.350+0 –.379–4 .1474+3 1.993 .333+0 –.141–4 .3624+3 1.207 –.932–1 .530–2 .7336+3 1.212 –.941–1 .483–2 .2537+3 1.997 .195+0 –.483–5 .3943+3 1.306 .524–1 .518–3 .8070+3 1.302 .499–1 –.166–4 .1640+4 1.015 .315–1 .162–1 .2438+4 1.021 .320–1 .161–1 .3464+2 1.998 .162+0 .612–6
200 .3554+2 1.993 –.204+0 –.405–4 .1226+3 1.995 .146+0 –.179–4 .2607+3 1.359 –.253–1 .112–1 .5244+3 1.368 –.260–1 .112–1 .1398+3 1.997 .112+0 –.704–5 .2140+3 1.549 –.155–1 .146–3 .4308+3 1.550 –.161–1 .177–3 .3537+3 1.216 .971–1 .251–1 .5244+3 1.217 .978–1 .251–1 .1347+2 1.998 .113+0 –.211–5
500 .3160+2 1.990 .697–1 –.420–4 .7594+2 1.998 –.362–1 –.201–4 .1137+3 1.455 .176+0 .198–1 .2260+3 1.470 .177+0 .201–1 .4468+2 1.998 –.311–1 –.746–5 .5384+2 1.614 .752–1 .574–2 .1063+3 1.623 .766–1 .611–2 .2701+2 1.176 .286+0 .460–1 .3987+2 1.170 .286+0 .463–1 .3240+1 1.998 –.268–1 –.504–5
1000 .2611+2 1.985 .345+0 –.417–4 .4033+2 2.000 –.434–2 –.189–4 .4038+2 1.412 .415+0 .307–1 .7923+2 1.430 .420+0 .309–1 .1469+2 2.000 –.240–1 –.763–5 .1260+2 1.506 .302+0 .151–1 .2456+2 1.520 .307+0 .152–1 .2759+1 0.944 .465+0 .821–1 .4056+1 0.938 .464+0 .829–1 .9352+0 2.000 –.280–1 –.628–5
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E (eV) 1500 .2181+2 1.980 .544+0 –.410–4 .2439+2 1.999 .113+0 –.173–4 .1843+2 1.333 .582+0 .422–1 .3587+2 1.352 .590+0 .421–1 .7032+1 1.999 .766–1 –.788–5 .4694+1 1.391 .477+0 .264–1 .9083+1 1.407 .484+0 .262–1 .6476+0 0.780 .564+0 .118+0 .9494+0 0.776 .563+0 .119+0 .4259+0 1.999 .704–1 –.667–5
2000 .1842+2 1.975 .706+0 –.400–4 .1604+2 1.997 .245+0 –.159–4 .9763+1 1.252 .707+0 .544–1 .1889+2 1.271 .716+0 .540–1 .4028+1 1.998 .199+0 –.792–5 .2206+1 1.290 .611+0 .389–1 .4246+1 1.307 .619+0 .384–1 .2201+0 0.672 .636+0 .153+0 .3221+0 0.672 .635+0 .153+0 .2374+0 1.998 .190+0 –.656–5
3000 .1351+2 1.966 .969+0 –.377–4 .8153+1 1.991 .499+0 –.135–4 .3591+1 1.106 .882+0 .794–1 .6886+1 1.125 .892+0 .785–1 .1750+1 1.993 .445+0 –.765–5 .7069+0 1.123 .804+0 .648–1 .1350+1 1.141 .814+0 .637–1 .4468–1 0.520 .731+0 .215+0 .6512–1 0.527 .733+0 .216+0 .1002+0 1.993 .439+0 –.697–5
4000 .1020+2 1.956 .118+1 –.349–4 .4755+1 1.984 .728+0 –.113–4 .1649+1 0.983 .999+0 .104+0 .3142+1 1.002 .101+1 .103+0 .9345+0 1.986 .674+0 –.700–5 .2997+0 0.991 .938+0 .909–1 .5687+0 1.009 .947+0 .894–1 .1370–1 0.417 .778+0 .271+0 .1990–1 0.431 .784+0 .272+0 .5274–1 1.986 .669+0 –.650–5
5000 .7893+1 1.946 .137+1 –.316–4 .3032+1 1.975 .933+0 –.913–5 .8705+0 0.878 .108+1 .128+0 .1649+1 0.897 .109+1 .127+0 .5624+0 1.978 .882+0 –.597–5 .1500+0 0.883 .103+1 .116+0 .2831+0 0.901 .104+1 .115+0 .5358–2 0.343 .796+0 .320+0 .7761–2 0.362 .806+0 .320+0 .3145–1 1.978 .876+0 –.547–5
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Mn, Z = 25 Shell 1s1/2 Eb = 6544 eV 2s1/2 Eb = 775 eV 2 p1/2 Eb = 656 eV 2 p3/2 Eb = 645 eV 3s1/2 Eb = 89 eV 3 p1/2 Eb = 55 eV 3 p3/2 Eb = 53 eV 3d3/2 Eb = 9 eV 3d5/2 Eb = 9 eV 4s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3373+2 1.993 –.379+0 –.441–4 .1367+3 1.993 .359+0 –.157–4 .3328+3 1.193 –.104+0 .451–2 .6748+3 1.198 –.105+0 .404–2 .2550+3 1.997 .205+0 –.506–5 .4023+3 1.282 .658–1 .204–2 .8311+3 1.278 .625–1 .141–2 .2091+4 0.986 .241–1 .150–1 .3113+4 0.992 .246–1 .148–1 .4804+2 1.998 .164+0 –.593–6
200 .3256+2 1.992 –.231+0 –.467–4 .1154+3 1.994 .169+0 –.200–4 .2459+3 1.346 –.400–1 .105–1 .4956+3 1.356 –.410–1 .105–1 .1444+3 1.997 .126+0 –.799–5 .2252+3 1.536 –.110–1 –.438–4 .4562+3 1.537 –.119–1 –.557–4 .4812+3 1.201 .852–1 .240–1 .7145+3 1.202 .860–1 .240–1 .1876+2 1.997 .122+0 –.113–5
500 .2923+2 1.989 .457–1 –.484–4 .7385+2 1.998 –.291–1 –.231–4 .1139+3 1.451 .158+0 .194–1 .2266+3 1.467 .159+0 .198–1 .4794+2 1.998 –.231–1 –.890–5 .6021+2 1.617 .576–1 .499–2 .1193+3 1.627 .588–1 .540–2 .3981+2 1.193 .273+0 .443–1 .5885+2 1.186 .273+0 .446–1 .4569+1 1.998 –.183–1 –.504–5
1000 .2452+2 1.984 .326+0 –.483–4 .4065+2 2.000 –.184–1 –.222–4 .4280+2 1.420 .401+0 .301–1 .8402+2 1.439 .405+0 .303–1 .1619+2 1.999 –.358–1 –.923–5 .1475+2 1.522 .280+0 .136–1 .2878+2 1.537 .284+0 .138–1 .4268+1 0.976 .462+0 .786–1 .6281+1 0.968 .460+0 .794–1 .1338+1 1.999 –.404–1 –.693–5
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E (eV) 1500 .2075+2 1.980 .527+0 –.475–4 .2516+2 1.999 .876–1 –.207–4 .2018+2 1.348 .572+0 .410–1 .3928+2 1.368 .579+0 .409–1 .7847+1 1.999 .525–1 –.958–5 .5617+1 1.413 .458+0 .242–1 .1087+2 1.431 .464+0 .241–1 .1025+1 0.815 .568+0 .113+0 .1504+1 0.810 .567+0 .114+0 .6130+0 1.999 .452–1 –.787–5
2000 .1773+2 1.975 .689+0 –.464–4 .1682+2 1.997 .212+0 –.192–4 .1094+2 1.273 .700+0 .524–1 .2115+2 1.294 .710+0 .520–1 .4531+1 1.998 .167+0 –.972–5 .2678+1 1.317 .595+0 .358–1 .5152+1 1.335 .603+0 .354–1 .3540+0 0.704 .643+0 .147+0 .5183+0 0.703 .642+0 .148+0 .3433+0 1.998 .160+0 –.856–5
3000 .1325+2 1.965 .953+0 –.438–4 .8739+1 1.992 .461+0 –.166–4 .4142+1 1.135 .883+0 .766–1 .7933+1 1.155 .895+0 .755–1 .1991+1 1.994 .405+0 –.952–5 .8753+0 1.157 .797+0 .608–1 .1669+1 1.175 .807+0 .597–1 .7357–1 0.550 .742+0 .208+0 .1073+0 0.556 .744+0 .209+0 .1461+0 1.994 .398+0 –.856–5
4000 .1017+2 1.955 .117+1 –.409–4 .5173+1 1.985 .687+0 –.143–4 .1938+1 1.016 .101+1 .101+0 .3685+1 1.037 .102+1 .991–1 .1072+1 1.987 .630+0 –.892–5 .3761+0 1.027 .937+0 .857–1 .7126+0 1.046 .948+0 .842–1 .2291–1 0.446 .799+0 .263+0 .3330–1 0.459 .804+0 .264+0 .7742–1 1.987 .624+0 –.830–5
5000 .7974+1 1.945 .135+1 –.375–4 .3334+1 1.977 .890+0 –.120–4 .1036+1 0.915 .110+1 .124+0 .1960+1 0.936 .111+1 .122+0 .6497+0 1.979 .836+0 –.788–5 .1901+0 0.920 .104+1 .110+0 .3582+0 0.939 .105+1 .108+0 .9038–2 0.367 .825+0 .312+0 .1310–1 0.385 .834+0 .312+0 .4644–1 1.980 .829+0 –.740–5
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Fe, Z = 26 Shell 1s1/2 Eb = 7117 eV 2s1/2 Eb = 851 eV 2 p1/2 Eb = 727 eV 2 p3/2 Eb = 714 eV 3s1/2 Eb = 99 eV 3 p1/2 Eb = 61 eV 3 p3/2 Eb = 59 eV 3d3/2 Eb = 9 eV 3d5/2 Eb = 9 eV 4s1/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3095+2 1.992 –.415+0 –.510–4 .1276+3 1.992 .398+0 –.172–4 .3096+3 1.171 –.114+0 .369–2 .6287+3 1.175 –.116+0 .320–2 .2492+3 1.997 .222+0 –.497–5 .3911+3 1.239 .857–1 .419–2 .8104+3 1.235 .817–1 .341–2 .2368+4 0.937 .198–1 .145–1 .3526+4 0.944 .203–1 .142–1 .4856+2 1.998 .170+0 –.410–8
200 .2997+2 1.991 –.264+0 –.540–4 .1091+3 1.994 .202+0 –.224–4 .2343+3 1.329 –.574–1 .960–2 .4730+3 1.339 –.587–1 .963–2 .1458+3 1.997 .146+0 –.894–5 .2300+3 1.515 –.267–2 –.220–3 .4668+3 1.515 –.405–2 –.294–3 .5844+3 1.173 .738–1 .233–1 .8673+3 1.175 .747–1 .233–1 .1915+2 1.997 .136+0 –.145–5
500 .2714+2 1.988 .174–1 –.559–4 .7193+2 1.997 –.187–1 –.265–4 .1144+3 1.446 .138+0 .191–1 .2279+3 1.463 .139+0 .195–1 .5049+2 1.997 –.124–1 –.106–4 .6570+2 1.618 .397–1 .423–2 .1302+3 1.628 .408–1 .469–2 .5152+2 1.206 .257+0 .430–1 .7609+2 1.199 .257+0 .433–1 .4772+1 1.997 –.669–2 –.616–5
1000 .2306+2 1.984 .303+0 –.558–4 .4090+2 1.999 –.312–1 –.260–4 .4527+2 1.427 .384+0 .295–1 .8890+2 1.447 .388+0 .297–1 .1750+2 1.999 –.461–1 –.111–4 .1680+2 1.538 .255+0 .122–1 .3277+2 1.554 .259+0 .125–1 .5713+1 1.009 .457+0 .756–1 .8398+1 1.000 .456+0 .764–1 .1420+1 1.999 –.491–1 –.845–5
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E (eV) 1500 .1975+2 1.979 .506+0 –.549–4 .2587+2 1.999 .626–1 –.245–4 .2201+2 1.363 .559+0 .398–1 .4283+2 1.384 .567+0 .397–1 .8588+1 1.999 .289–1 –.116–4 .6532+1 1.436 .436+0 .220–1 .1263+2 1.455 .443+0 .220–1 .1394+1 0.852 .572+0 .109+0 .2043+1 0.846 .571+0 .110+0 .6563+0 1.999 .225–1 –.965–5
2000 .1705+2 1.974 .668+0 –.537–4 .1756+2 1.998 .180+0 –.230–4 .1218+2 1.294 .692+0 .509–1 .2353+2 1.316 .702+0 .504–1 .4996+1 1.999 .135+0 –.118–4 .3155+1 1.345 .578+0 .332–1 .6059+1 1.364 .587+0 .327–1 .4875+0 0.737 .650+0 .141+0 .7126+0 0.735 .648+0 .143+0 .3696+0 1.999 .128+0 –.104–4
3000 .1297+2 1.964 .936+0 –.509–4 .9321+1 1.993 .422+0 –.202–4 .4742+1 1.162 .884+0 .738–1 .9071+1 1.184 .897+0 .727–1 .2218+1 1.994 .366+0 –.117–4 .1049+1 1.188 .787+0 .569–1 .1997+1 1.209 .799+0 .559–1 .1032+0 0.580 .754+0 .201+0 .1503+0 0.585 .755+0 .202+0 .1585+0 1.995 .358+0 –.107–4
4000 .1010+2 1.955 .115+1 –.479–4 .5596+1 1.986 .646+0 –.178–4 .2259+1 1.047 .102+1 .968–1 .4288+1 1.070 .103+1 .952–1 .1204+1 1.988 .586+0 –.112–4 .4566+0 1.062 .935+0 .809–1 .8627+0 1.082 .947+0 .793–1 .3258–1 0.475 .818+0 .256+0 .4728–1 0.486 .822+0 .257+0 .8448–1 1.988 .579+0 –.104–4
5000 .8022+1 1.945 .134+1 –.443–4 .3644+1 1.978 .848+0 –.153–4 .1223+1 0.948 .111+1 .120+0 .2308+1 0.971 .113+1 .118+0 .7339+0 1.981 .790+0 –.102–4 .2328+0 0.956 .104+1 .105+0 .4374+0 0.976 .106+1 .103+0 .1297–1 0.393 .852+0 .304+0 .1876–1 0.410 .860+0 .305+0 .5095–1 1.981 .783+0 –.962–5
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Co, Z = 27 Shell 1s1/2 Eb = 7715 eV 2s1/2 Eb = 931 eV 2 p1/2 Eb = 800 eV 2 p3/2 Eb = 785 eV 3s1/2 Eb = 107 eV 3 p1/2 Eb = 68 eV 3 p3/2 Eb = 66 eV 3d3/2 Eb = 9 eV 3d5/2 Eb = 9 eV 4s1/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2850+2 1.991 –.451+0 –.588–4 .1193+3 1.991 .439+0 –.187–4 .2888+3 1.149 –.123+0 .302–2 .5875+3 1.153 –.125+0 .250–2 .2453+3 1.997 .236+0 –.456–5 .3757+3 1.195 .105+0 .698–2 .7813+3 1.190 .101+0 .603–2 .2615+4 0.890 .165–1 .140–1 .3893+4 0.898 .170–1 .137–1 .4925+2 1.998 .174+0 .814–6
200 .2767+2 1.990 –.299+0 –.623–4 .1032+3 1.993 .236+0 –.250–4 .2234+3 1.312 –.742–1 .867–2 .4517+3 1.322 –.758–1 .871–2 .1475+3 1.996 .165+0 –.978–5 .2320+3 1.492 .909–2 –.141–3 .4720+3 1.492 .709–2 –.295–3 .6929+3 1.143 .638–1 .227–1 .1028+4 1.146 .648–1 .226–1 .1955+2 1.997 .150+0 –.177–5
500 .2524+2 1.988 –.119–1 –.645–4 .6987+2 1.996 –.566–2 –.303–4 .1144+3 1.440 .118+0 .186–1 .2282+3 1.457 .119+0 .191–1 .5299+2 1.997 .167–3 –.124–4 .7077+2 1.618 .238–1 .352–2 .1403+3 1.628 .247–1 .402–2 .6518+2 1.214 .241+0 .419–1 .9618+2 1.207 .241+0 .421–1 .4964+1 1.997 .642–2 –.736–5
1000 .2171+2 1.983 .278+0 –.644–4 .4096+2 1.999 –.415–1 –.304–4 .4751+2 1.432 .365+0 .289–1 .9335+2 1.453 .370+0 .292–1 .1882+2 1.999 –.535–1 –.132–4 .1891+2 1.551 .230+0 .110–1 .3686+2 1.568 .234+0 .114–1 .7480+1 1.039 .450+0 .728–1 .1098+2 1.029 .449+0 .736–1 .1498+1 1.999 –.551–1 –.103–4
123
E (eV) 1500 .1879+2 1.978 .482+0 –.631–4 .2644+2 1.999 .394–1 –.288–4 .2379+2 1.376 .544+0 .389–1 .4629+2 1.400 .553+0 .388–1 .9344+1 1.999 .747–2 –.138–4 .7507+1 1.458 .413+0 .201–1 .1449+2 1.478 .420+0 .202–1 .1856+1 0.885 .574+0 .105+0 .2715+1 0.878 .572+0 .106+0 .6987+0 1.999 .171–2 –.117–4
2000 .1637+2 1.973 .648+0 –.619–4 .1822+2 1.998 .150+0 –.273–4 .1343+2 1.312 .682+0 .493–1 .2594+2 1.336 .693+0 .489–1 .5476+1 1.999 .105+0 –.142–4 .3673+1 1.370 .560+0 .306–1 .7043+1 1.391 .569+0 .302–1 .6558+0 0.770 .656+0 .136+0 .9572+0 0.766 .654+0 .138+0 .3956+0 1.999 .976–1 –.123–4
3000 .1266+2 1.964 .916+0 –.590–4 .9873+1 1.993 .383+0 –.245–4 .5373+1 1.187 .882+0 .713–1 .1027+2 1.212 .896+0 .701–1 .2454+1 1.995 .326+0 –.143–4 .1243+1 1.219 .777+0 .532–1 .2359+1 1.241 .789+0 .522–1 .1412+0 0.611 .765+0 .195+0 .2053+0 0.614 .765+0 .196+0 .1708+0 1.995 .318+0 –.131–4
4000 .9997+1 1.954 .113+1 –.558–4 .6011+1 1.987 .604+0 –.219–4 .2604+1 1.076 .102+1 .934–1 .4936+1 1.100 .104+1 .917–1 .1341+1 1.989 .543+0 –.138–4 .5472+0 1.094 .931+0 .763–1 .1031+1 1.116 .944+0 .747–1 .4516–1 0.503 .835+0 .248+0 .6542–1 0.513 .838+0 .249+0 .9155–1 1.990 .535+0 –.128–4
5000 .8033+1 1.944 .132+1 –.521–4 .3955+1 1.979 .806+0 –.193–4 .1428+1 0.979 .112+1 .115+0 .2689+1 1.004 .114+1 .113+0 .8226+0 1.982 .744+0 –.129–4 .2815+0 0.990 .105+1 .992–1 .5274+0 1.012 .106+1 .972–1 .1814–1 0.419 .875+0 .296+0 .2619–1 0.435 .882+0 .297+0 .5549–1 1.983 .737+0 –.121–4
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Ni, Z = 28 Shell 1s1/2 Eb = 8338 eV 2s1/2 Eb = 1015 eV 2 p1/2 Eb = 877 eV 2 p3/2 Eb = 860 eV 3s1/2 Eb = 117 eV 3 p1/2 Eb = 75 eV 3 p3/2 Eb = 73 eV 3d3/2 Eb = 10 eV 3d5/2 Eb = 10 eV 4s1/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2631+2 1.991 –.488+0 –.677–4 .1116+3 1.990 .481+0 –.202–4 .2697+3 1.127 –.131+0 .255–2 .5493+3 1.131 –.132+0 .200–2 .2387+3 1.996 .251+0 –.385–5 .3593+3 1.148 .123+0 .104–1 .7502+3 1.142 .117+0 .922–2 .2797+4 0.842 .140–1 .138–1 .4164+4 0.851 .145–1 .134–1 .4970+2 1.997 .176+0 .191–5
200 .2561+2 1.990 –.334+0 –.719–4 .9755+2 1.992 .272+0 –.278–4 .2128+3 1.294 –.903–1 .771–2 .4307+3 1.304 –.923–1 .777–2 .1476+3 1.996 .184+0 –.106–4 .2324+3 1.468 .239–1 .239–3 .4741+3 1.467 .212–1 –.103–4 .8005+3 1.112 .555–1 .222–1 .1187+4 1.116 .565–1 .221–1 .1990+2 1.997 .163+0 –.198–5
500 .2352+2 1.987 –.422–1 –.743–4 .6772+2 1.996 .998–2 –.345–4 .1138+3 1.432 .972–1 .182–1 .2272+3 1.451 .977–1 .187–1 .5511+2 1.997 .144–1 –.144–4 .7552+2 1.616 .990–2 .285–2 .1499+3 1.626 .106–1 .338–2 .8069+2 1.218 .225+0 .409–1 .1190+3 1.212 .226+0 .411–1 .5137+1 1.997 .208–1 –.866–5
1000 .2045+2 1.982 .253+0 –.741–4 .4085+2 1.999 –.491–1 –.353–4 .4946+2 1.435 .346+0 .284–1 .9724+2 1.458 .351+0 .287–1 .2007+2 1.998 –.583–1 –.156–4 .2106+2 1.563 .205+0 .981–2 .4105+2 1.580 .209+0 .103–1 .9595+1 1.066 .441+0 .704–1 .1407+2 1.056 .440+0 .712–1 .1573+1 1.998 –.585–1 –.125–4
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E (eV) 1500 .1787+2 1.977 .460+0 –.727–4 .2689+2 1.999 .186–1 –.338–4 .2548+2 1.387 .528+0 .380–1 .4958+2 1.412 .537+0 .379–1 .1009+2 1.999 –.114–1 –.164–4 .8540+1 1.477 .389+0 .183–1 .1647+2 1.497 .396+0 .185–1 .2420+1 0.917 .573+0 .101+0 .3536+1 0.909 .571+0 .102+0 .7396+0 1.999 –.171–1 –.140–4
2000 .1570+2 1.972 .627+0 –.714–4 .1880+2 1.998 .121+0 –.323–4 .1467+2 1.328 .670+0 .480–1 .2833+2 1.354 .682+0 .475–1 .5959+1 1.999 .775–1 –.169–4 .4233+1 1.393 .539+0 .282–1 .8104+1 1.415 .549+0 .279–1 .8645+0 0.801 .661+0 .132+0 .1260+1 0.796 .659+0 .133+0 .4209+0 1.999 .687–1 –.145–4
3000 .1233+2 1.963 .897+0 –.682–4 .1039+2 1.994 .346+0 –.293–4 .6027+1 1.210 .878+0 .689–1 .1150+2 1.237 .893+0 .677–1 .2696+1 1.996 .289+0 –.173–4 .1456+1 1.247 .764+0 .498–1 .2759+1 1.270 .777+0 .487–1 .1891+0 0.639 .775+0 .188+0 .2744+0 0.641 .775+0 .190+0 .1830+0 1.996 .280+0 –.157–4
4000 .9859+1 1.953 .112+1 –.650–4 .6413+1 1.988 .563+0 –.267–4 .2973+1 1.103 .102+1 .899–1 .5625+1 1.129 .104+1 .880–1 .1484+1 1.990 .500+0 –.170–4 .6485+0 1.124 .924+0 .717–1 .1219+1 1.148 .939+0 .700–1 .6122–1 0.531 .849+0 .241+0 .8851–1 0.539 .852+0 .242+0 .9859–1 1.991 .493+0 –.155–4
5000 .8011+1 1.943 .131+1 –.609–4 .4263+1 1.981 .764+0 –.238–4 .1651+1 1.008 .113+1 .111+0 .3102+1 1.035 .115+1 .109+0 .9152+0 1.984 .699+0 –.160–4 .3366+0 1.022 .105+1 .941–1 .6287+0 1.046 .106+1 .920–1 .2482–1 0.445 .895+0 .288+0 .3576–1 0.460 .902+0 .289+0 .6003–1 1.984 .691+0 –.149–4
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Cu, Z = 29 Shell 1s1/2 Eb = 8986 eV 2s1/2 Eb = 1103 eV 2 p1/2 Eb = 958 eV 2 p3/2 Eb = 938 eV 3s1/2 Eb = 127 eV 3 p1/2 Eb = 82 eV 3 p3/2 Eb = 80 eV 3d3/2 Eb = 11 eV 3d5/2 Eb = 10 eV 4s1/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2435+2 1.990 –.530+0 –.772–4 .1048+3 1.989 .538+0 –.213–4 .2542+3 1.096 –.135+0 .266–2 .5190+3 1.099 –.137+0 .203–2 .2278+3 1.996 .271+0 –.194–5 .3262+3 1.074 .145+0 .154–1 .6848+3 1.067 .138+0 .140–1 .2714+4 0.781 .143–1 .145–1 .4068+4 0.791 .147–1 .139–1 .3605+2 1.997 .174+0 .554–5
200 .2379+2 1.989 –.375+0 –.825–4 .9257+2 1.991 .320+0 –.306–4 .2044+3 1.271 –.108+0 .658–2 .4147+3 1.281 –.110+0 .663–2 .1456+3 1.995 .211+0 –.111–4 .2266+3 1.435 .469–1 .102–2 .4637+3 1.433 .432–1 .626–3 .8612+3 1.068 .494–1 .223–1 .1279+4 1.073 .502–1 .221–1 .1525+2 1.996 .183+0 –.265–5
500 .2198+2 1.986 –.777–1 –.856–4 .6576+2 1.995 .311–1 –.392–4 .1137+3 1.423 .734–1 .176–1 .2273+3 1.442 .734–1 .181–1 .5669+2 1.996 .329–1 –.166–4 .7932+2 1.611 –.333–2 .211–2 .1575+3 1.621 –.301–2 .266–2 .9315+2 1.217 .208+0 .403–1 .1371+3 1.212 .208+0 .405–1 .3982+1 1.996 .399–1 –.847–5
1000 .1929+2 1.981 .223+0 –.852–4 .4072+2 1.998 –.545–1 –.408–4 .5150+2 1.438 .324+0 .277–1 .1014+3 1.462 .329+0 .281–1 .2117+2 1.998 –.608–1 –.184–4 .2309+2 1.574 .177+0 .864–2 .4495+2 1.592 .182+0 .926–2 .1136+2 1.092 .431+0 .686–1 .1661+2 1.082 .430+0 .693–1 .1240+1 1.998 –.608–1 –.135–4
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E (eV) 1500 .1701+2 1.976 .436+0 –.840–4 .2730+2 1.999 –.131–2 –.397–4 .2724+2 1.396 .512+0 .371–1 .5302+2 1.422 .521+0 .371–1 .1077+2 1.999 –.292–1 –.195–4 .9547+1 1.493 .363+0 .166–1 .1838+2 1.515 .371+0 .169–1 .2898+1 0.947 .571+0 .975–1 .4221+1 0.937 .569+0 .988–1 .5871+0 1.999 –.340–1 –.164–4
2000 .1507+2 1.972 .604+0 –.821–4 .1934+2 1.999 .926–1 –.380–4 .1598+2 1.343 .657+0 .468–1 .3084+2 1.371 .670+0 .463–1 .6404+1 1.999 .503–1 –.201–4 .4789+1 1.415 .517+0 .259–1 .9149+1 1.439 .527+0 .258–1 .1043+1 0.832 .665+0 .127+0 .1515+1 0.825 .662+0 .128+0 .3363+0 1.999 .423–1 –.179–4
3000 .1199+2 1.962 .877+0 –.788–4 .1090+2 1.995 .309+0 –.349–4 .6728+1 1.232 .872+0 .668–1 .1283+2 1.260 .889+0 .655–1 .2924+1 1.996 .251+0 –.207–4 .1673+1 1.274 .749+0 .464–1 .3159+1 1.299 .764+0 .455–1 .2308+0 0.670 .786+0 .183+0 .3335+0 0.670 .785+0 .185+0 .1472+0 1.997 .242+0 –.187–4
4000 .9705+1 1.952 .110+1 –.753–4 .6815+1 1.989 .522+0 –.322–4 .3374+1 1.128 .102+1 .869–1 .6375+1 1.157 .104+1 .849–1 .1619+1 1.991 .457+0 –.206–4 .7526+0 1.155 .916+0 .675–1 .1410+1 1.180 .933+0 .659–1 .7543–1 0.558 .864+0 .234+0 .1086+0 0.565 .865+0 .236+0 .7973–1 1.992 .449+0 –.187–4
5000 .7968+1 1.942 .129+1 –.710–4 .4574+1 1.982 .721+0 –.292–4 .1896+1 1.037 .114+1 .108+0 .3556+1 1.065 .116+1 .105+0 .1003+1 1.985 .654+0 –.196–4 .3937+0 1.054 .104+1 .892–1 .7326+0 1.079 .106+1 .870–1 .3082–1 0.471 .915+0 .281+0 .4422–1 0.484 .920+0 .282+0 .4875–1 1.985 .645+0 –.185–4
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Zn, Z = 30 Shell 1s1/2 Eb = 9663 eV 2s1/2 Eb = 1198 eV 2 p1/2 Eb = 1048 eV 2 p3/2 Eb = 1025 eV 3s1/2 Eb = 141 eV 3 p1/2 Eb = 94 eV 3 p3/2 Eb = 91 eV 3d3/2 Eb = 12 eV 3d5/2 Eb = 11 eV 4s1/2 Eb = 9 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2260+2 1.989 –.562+0 –.890–4 .9777+2 1.988 .568+0 –.232–4 .2348+3 1.083 –.142+0 .235–2 .4801+3 1.087 –.144+0 .171–2 .2213+3 1.995 .284+0 –.102–5 .3167+3 1.048 .152+0 .191–1 .6707+3 1.041 .145+0 .174–1 .3023+4 0.751 .102–1 .135–1 .4541+4 0.762 .107–1 .129–1 .4951+2 1.997 .179+0 .501–5
200 .2210+2 1.988 –.406+0 –.950–4 .8710+2 1.990 .349+0 –.340–4 .1918+3 1.258 –.120+0 .586–2 .3897+3 1.269 –.123+0 .594–2 .1447+3 1.995 .226+0 –.118–4 .2253+3 1.415 .618–1 .210–2 .4641+3 1.413 .572–1 .159–2 .1010+4 1.046 .424–1 .215–1 .1504+4 1.053 .433–1 .212–1 .2034+2 1.996 .187+0 –.193–5
500 .2053+2 1.985 –.105+0 –.982–4 .6320+2 1.994 .486–1 –.443–4 .1108+3 1.415 .553–1 .171–1 .2219+3 1.436 .550–1 .177–1 .5837+2 1.995 .474–1 –.189–4 .8320+2 1.607 –.106–1 .166–2 .1658+3 1.617 –.106–1 .222–2 .1175+3 1.217 .193+0 .393–1 .1733+3 1.212 .194+0 .394–1 .5421+1 1.996 .528–1 –.110–4
1000 .1817+2 1.980 .199+0 –.976–4 .4015+2 1.998 –.565–1 –.468–4 .5241+2 1.439 .306+0 .275–1 .1032+3 1.465 .311+0 .279–1 .2238+2 1.998 –.601–1 –.215–4 .2532+2 1.581 .156+0 .779–2 .4937+2 1.600 .160+0 .850–2 .1502+2 1.111 .418+0 .664–1 .2199+2 1.100 .417+0 .672–1 .1707+1 1.997 –.584–1 –.172–4
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E (eV) 1500 .1615+2 1.976 .412+0 –.960–4 .2741+2 1.999 –.165–1 –.458–4 .2850+2 1.404 .495+0 .365–1 .5550+2 1.432 .505+0 .365–1 .1155+2 1.999 –.418–1 –.228–4 .1072+2 1.509 .338+0 .152–1 .2065+2 1.531 .346+0 .155–1 .3918+1 0.975 .566+0 .946–1 .5712+1 0.965 .564+0 .958–1 .8158+0 1.999 –.471–1 –.193–4
2000 .1441+2 1.971 .583+0 –.943–4 .1969+2 1.999 .687–1 –.444–4 .1705+2 1.355 .644+0 .456–1 .3291+2 1.384 .657+0 .452–1 .6928+1 1.999 .277–1 –.237–4 .5459+1 1.434 .494+0 .238–1 .1043+2 1.459 .505+0 .238–1 .1429+1 0.862 .666+0 .123+0 .2077+1 0.854 .663+0 .124+0 .4690+0 1.999 .201–1 –.205–4
3000 .1162+2 1.961 .858+0 –.905–4 .1131+2 1.995 .275+0 –.412–4 .7375+1 1.250 .866+0 .649–1 .1405+2 1.281 .883+0 .636–1 .3197+1 1.997 .217+0 –.246–4 .1942+1 1.298 .734+0 .434–1 .3664+1 1.325 .749+0 .425–1 .3216+0 0.696 .794+0 .177+0 .4651+0 0.694 .792+0 .179+0 .2069+0 1.997 .207+0 –.225–4
4000 .9510+1 1.951 .108+1 –.868–4 .7171+1 1.990 .483+0 –.384–4 .3765+1 1.151 .102+1 .843–1 .7103+1 1.182 .104+1 .822–1 .1783+1 1.992 .417+0 –.246–4 .8840+0 1.182 .907+0 .637–1 .1653+1 1.209 .924+0 .620–1 .1064+0 0.584 .876+0 .227+0 .1533+0 0.589 .876+0 .229+0 .1126+0 1.993 .408+0 –.228–4
5000 .7884+1 1.942 .127+1 –.822–4 .4861+1 1.983 .680+0 –.352–4 .2143+1 1.062 .114+1 .104+0 .4012+1 1.093 .116+1 .102+0 .1111+1 1.986 .611+0 –.238–4 .4666+0 1.083 .104+1 .846–1 .8665+0 1.110 .106+1 .823–1 .4390–1 0.495 .930+0 .273+0 .6301–1 0.507 .935+0 .275+0 .6912–1 1.987 .601+0 –.224–4
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Ga, Z = 31 Shell 1s1/2 Eb = 10371 eV 2s1/2 Eb = 1302 eV 2 p1/2 Eb = 1146 eV 2 p3/2 Eb = 1119 eV 3s1/2 Eb = 162 eV 3 p1/2 Eb = 111 eV 3 p3/2 Eb = 107 eV 3d3/2 Eb = 21 eV 3d5/2 Eb = 20 eV 4s1/2 Eb = 11 eV 4 p1/2 Eb = 6 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2101+2 1.988 –.591+0 –.103–3 .9100+2 1.987 .593+0 –.257–4 .2160+3 1.076 –.151+0 .188–2 .4424+3 1.079 –.153+0 .126–2 .2103+3 1.995 .301+0 –.305–6 .3053+3 1.035 .159+0 .226–1 .6511+3 1.028 .151+0 .206–1 .3081+4 0.727 .655–2 .132–1 .4633+4 0.740 .702–2 .125–1 .6789+2 1.996 .183+0 .468–5 .2193+2 0.747 .128+0 .110–1
200 .2055+2 1.987 –.436+0 –.110–3 .8164+2 1.989 .376+0 –.379–4 .1789+3 1.247 –.132+0 .522–2 .3642+3 1.258 –.135+0 .535–2 .1411+3 1.994 .243+0 –.127–4 .2212+3 1.397 .752–1 .338–2 .4583+3 1.394 .696–1 .276–2 .1107+4 1.027 .373–1 .213–1 .1648+4 1.035 .383–1 .210–1 .2813+2 1.996 .191+0 –.883–6 .1332+2 1.404 .102+0 –.776–3
500 .1919+2 1.984 –.131+0 –.113–3 .6044+2 1.993 .659–1 –.501–4 .1072+3 1.408 .387–1 .166–1 .2149+3 1.430 .380–1 .174–1 .5928+2 1.995 .614–1 –.217–4 .8604+2 1.603 –.154–1 .133–2 .1720+3 1.613 –.158–1 .190–2 .1411+3 1.216 .182+0 .386–1 .2082+3 1.211 .183+0 .387–1 .7544+1 1.995 .643–1 –.109–4 .4216+1 1.647 –.208–1 .377–4
1000 .1712+2 1.979 .176+0 –.112–3 .3936+2 1.997 –.566–1 –.536–4 .5280+2 1.439 .289+0 .271–1 .1041+3 1.466 .294+0 .277–1 .2342+2 1.997 –.579–1 –.251–4 .2742+2 1.587 .136+0 .701–2 .5354+2 1.607 .140+0 .783–2 .1909+2 1.128 .407+0 .648–1 .2797+2 1.116 .406+0 .656–1 .2402+1 1.997 –.548–1 –.189–4 .1180+1 1.615 .115+0 .518–2
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E (eV) 1500 .1532+2 1.974 .391+0 –.110–3 .2735+2 1.999 –.292–1 –.529–4 .2951+2 1.409 .480+0 .359–1 .5749+2 1.439 .489+0 .360–1 .1228+2 1.999 –.520–1 –.267–4 .1191+2 1.521 .315+0 .139–1 .2295+2 1.545 .323+0 .144–1 .5115+1 1.000 .561+0 .918–1 .7461+1 0.988 .559+0 .931–1 .1156+1 1.998 –.550–1 –.225–4 .4838+0 1.540 .294+0 .117–1
2000 .1377+2 1.970 .563+0 –.108–3 .1991+2 1.999 .473–1 –.516–4 .1801+2 1.365 .631+0 .447–1 .3475+2 1.396 .644+0 .442–1 .7439+1 1.999 .791–2 –.279–4 .6158+1 1.451 .472+0 .220–1 .1176+2 1.477 .483+0 .220–1 .1896+1 0.889 .667+0 .119+0 .2756+1 0.880 .664+0 .121+0 .6689+0 1.999 .129–2 –.245–4 .2421+0 1.465 .455+0 .198–1
3000 .1124+2 1.960 .841+0 –.104–3 .1167+2 1.996 .244+0 –.484–4 .8000+1 1.266 .858+0 .632–1 .1523+2 1.298 .877+0 .618–1 .3475+1 1.997 .185+0 –.290–4 .2233+1 1.319 .718+0 .406–1 .4211+1 1.348 .734+0 .398–1 .4350+0 0.722 .802+0 .171+0 .6290+0 0.718 .799+0 .174+0 .2972+0 1.997 .175+0 –.265–4 .8459–1 1.329 .704+0 .381–1
4000 .9293+1 1.950 .106+1 –.996–4 .7494+1 1.991 .446+0 –.453–4 .4158+1 1.172 .102+1 .821–1 .7834+1 1.205 .104+1 .799–1 .1953+1 1.993 .379+0 –.292–4 .1030+1 1.207 .897+0 .604–1 .1923+1 1.236 .916+0 .587–1 .1458+0 0.606 .887+0 .221+0 .2099+0 0.610 .887+0 .223+0 .1626+0 1.993 .369+0 –.270–4 .3821–1 1.212 .885+0 .576–1
5000 .7775+1 1.941 .126+1 –.950–4 .5131+1 1.984 .640+0 –.421–4 .2398+1 1.086 .114+1 .101+0 .4481+1 1.118 .117+1 .982–1 .1224+1 1.987 .569+0 –.286–4 .5484+0 1.110 .103+1 .803–1 .1017+1 1.139 .105+1 .780–1 .6073–1 0.518 .946+0 .266+0 .8715–1 0.529 .949+0 .268+0 .1002+0 1.988 .558+0 –.269–4 .2009–1 1.114 .102+1 .777–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Ge, Z = 32 Shell 1s1/2 Eb = 11107 eV 2s1/2 Eb = 1413 eV 2 p1/2 Eb = 1251 eV 2 p3/2 Eb = 1220 eV 3s1/2 Eb = 184 eV 3 p1/2 Eb = 130 eV 3 p3/2 Eb = 125 eV 3d3/2 Eb = 33 eV 3d5/2 Eb = 32 eV 4s1/2 Eb = 14 eV 4 p1/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1958+2 1.987 –.622+0 –.118–3 .8475+2 1.986 .619+0 –.282–4 .1987+3 1.068 –.160+0 .128–2 .4076+3 1.071 –.163+0 .663–3 .2007+3 1.994 .320+0 .696–6 .2942+3 1.020 .166+0 .266–1 .6314+3 1.012 .157+0 .245–1 .3049+4 0.701 .258–2 .129–1 .4586+4 0.714 .308–2 .123–1 .8193+2 1.996 .186+0 .584–5 .3320+2 0.732 .122+0 .128–1
200 .1916+2 1.986 –.464+0 –.126–3 .7650+2 1.988 .402+0 –.423–4 .1668+3 1.237 –.143+0 .455–2 .3399+3 1.249 –.147+0 .473–2 .1378+3 1.994 .259+0 –.135–4 .2169+3 1.382 .893–1 .486–2 .4521+3 1.379 .826–1 .411–2 .1181+4 1.009 .316–1 .211–1 .1760+4 1.018 .327–1 .207–1 .3463+2 1.995 .198+0 –.131–5 .2011+2 1.390 .113+0 –.360–5
500 .1796+2 1.983 –.157+0 –.129–3 .5770+2 1.992 .841–1 –.565–4 .1032+3 1.401 .222–1 .161–1 .2072+3 1.423 .210–1 .170–1 .6015+2 1.994 .758–1 –.247–4 .8858+2 1.598 –.185–1 .107–2 .1777+3 1.608 –.193–1 .165–2 .1649+3 1.214 .172+0 .382–1 .2434+3 1.210 .173+0 .383–1 .9375+1 1.995 .765–1 –.122–4 .6470+1 1.648 –.215–1 –.280–3
1000 .1614+2 1.978 .153+0 –.128–3 .3845+2 1.997 –.548–1 –.613–4 .5286+2 1.438 .273+0 .268–1 .1043+3 1.467 .277+0 .275–1 .2445+2 1.997 –.541–1 –.291–4 .2949+2 1.593 .117+0 .631–2 .5769+2 1.613 .121+0 .722–2 .2363+2 1.143 .396+0 .634–1 .3462+2 1.131 .395+0 .642–1 .3010+1 1.997 –.502–1 –.218–4 .1859+1 1.624 .955–1 .438–2
128
E (eV) 1500 .1454+2 1.973 .371+0 –.126–3 .2717+2 1.999 –.400–1 –.612–4 .3034+2 1.414 .464+0 .352–1 .5912+2 1.446 .474+0 .354–1 .1301+2 1.998 –.603–1 –.313–4 .1313+2 1.532 .293+0 .126–1 .2532+2 1.557 .300+0 .133–1 .6507+1 1.022 .555+0 .890–1 .9491+1 1.010 .553+0 .904–1 .1458+1 1.998 –.621–1 –.262–4 .7757+0 1.554 .270+0 .104–1
2000 .1315+2 1.969 .543+0 –.124–3 .2005+2 1.999 .279–1 –.597–4 .1887+2 1.373 .617+0 .438–1 .3642+2 1.407 .631+0 .434–1 .7963+1 1.999 –.978–2 –.326–4 .6899+1 1.466 .450+0 .202–1 .1318+2 1.493 .461+0 .204–1 .2452+1 0.915 .667+0 .116+0 .3563+1 0.904 .664+0 .117+0 .8478+0 1.999 –.158–1 –.286–4 .3929+0 1.482 .429+0 .178–1
3000 .1085+2 1.959 .824+0 –.119–3 .1197+2 1.996 .214+0 –.566–4 .8607+1 1.280 .850+0 .616–1 .1637+2 1.315 .870+0 .601–1 .3766+1 1.997 .155+0 –.341–4 .2552+1 1.340 .700+0 .379–1 .4808+1 1.369 .717+0 .371–1 .5737+0 0.748 .810+0 .167+0 .8293+0 0.743 .807+0 .169+0 .3795+0 1.998 .145+0 –.309–4 .1395+0 1.350 .685+0 .352–1
4000 .9063+1 1.949 .105+1 –.115–3 .7790+1 1.992 .411+0 –.534–4 .4553+1 1.190 .102+1 .796–1 .8569+1 1.225 .104+1 .773–1 .2132+1 1.994 .343+0 –.345–4 .1191+1 1.230 .884+0 .567–1 .2222+1 1.260 .905+0 .551–1 .1947+0 0.631 .900+0 .215+0 .2802+0 0.633 .898+0 .217+0 .2086+0 1.994 .332+0 –.319–4 .6364–1 1.239 .872+0 .541–1
5000 .7648+1 1.940 .124+1 –.110–3 .5387+1 1.985 .601+0 –.502–4 .2661+1 1.107 .115+1 .978–1 .4963+1 1.142 .117+1 .947–1 .1344+1 1.988 .528+0 –.342–4 .6401+0 1.135 .103+1 .758–1 .1185+1 1.166 .105+1 .734–1 .8191–1 0.543 .962+0 .260+0 .1175+0 0.552 .964+0 .262+0 .1291+0 1.989 .517+0 –.317–4 .3372–1 1.141 .102+1 .737–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables As, Z = 33 Shell 1s1/2 Eb = 11871 eV 2s1/2 Eb = 1531 eV 2 p1/2 Eb = 1362 eV 2 p3/2 Eb = 1327 eV 3s1/2 Eb = 208 eV 3 p1/2 Eb = 151 eV 3 p3/2 Eb = 145 eV 3d3/2 Eb = 46 eV 3d5/2 Eb = 45 eV 4s1/2 Eb = 17 eV 4 p1/2 Eb = 9 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1829+2 1.986 –.653+0 –.136–3 .7896+2 1.985 .645+0 –.309–4 .1830+3 1.059 –.170+0 .564–3 .3757+3 1.062 –.173+0 –.454–4 .1914+3 1.993 .340+0 .200–5 .2830+3 1.006 .173+0 .311–1 .6108+3 0.997 .163+0 .287–1 .2983+4 0.673 –.159–2 .126–1 .4488+4 0.688 –.109–2 .118–1 .9519+2 1.995 .190+0 .747–5 .4445+2 0.708 .111+0 .149–1
200 .1790+2 1.985 –.492+0 –.144–3 .7169+2 1.987 .427+0 –.470–4 .1555+3 1.228 –.155+0 .382–2 .3172+3 1.240 –.159+0 .407–2 .1343+3 1.993 .275+0 –.143–4 .2123+3 1.368 .104+0 .658–2 .4448+3 1.364 .961–1 .568–2 .1241+4 0.990 .253–1 .207–1 .1851+4 1.000 .266–1 .203–1 .4087+2 1.995 .204+0 –.150–5 .2670+2 1.373 .124+0 .894–3
500 .1683+2 1.982 –.183+0 –.147–3 .5499+2 1.992 .103+0 –.637–4 .9911+2 1.394 .575–2 .156–1 .1992+3 1.417 .394–2 .166–1 .6084+2 1.994 .906–1 –.280–4 .9072+2 1.593 –.201–1 .901–3 .1827+3 1.603 –.214–1 .147–2 .1889+3 1.212 .162+0 .379–1 .2789+3 1.208 .164+0 .379–1 .1117+2 1.995 .885–1 –.140–4 .8697+1 1.648 –.202–1 –.528–3
1000 .1522+2 1.977 .129+0 –.147–3 .3745+2 1.996 –.516–1 –.701–4 .5265+2 1.437 .256+0 .265–1 .1040+3 1.467 .260+0 .272–1 .2542+2 1.996 –.492–1 –.337–4 .3150+2 1.597 .100+0 .565–2 .6174+2 1.618 .104+0 .667–2 .2861+2 1.156 .384+0 .619–1 .4192+2 1.144 .384+0 .627–1 .3620+1 1.996 –.445–1 –.249–4 .2562+1 1.632 .779–1 .370–2
129
E (eV) 1500 .1380+2 1.972 .349+0 –.144–3 .2690+2 1.998 –.489–1 –.702–4 .3099+2 1.417 .448+0 .348–1 .6042+2 1.451 .458+0 .350–1 .1373+2 1.998 –.664–1 –.362–4 .1436+2 1.542 .270+0 .116–1 .2774+2 1.568 .278+0 .123–1 .8102+1 1.044 .548+0 .867–1 .1181+2 1.030 .546+0 .882–1 .1763+1 1.998 –.670–1 –.304–4 .1086+1 1.566 .246+0 .920–2
2000 .1255+2 1.967 .523+0 –.141–3 .2010+2 1.999 .103–1 –.689–4 .1964+2 1.381 .604+0 .431–1 .3790+2 1.416 .618+0 .427–1 .8487+1 1.999 –.253–1 –.379–4 .7670+1 1.480 .427+0 .187–1 .1466+2 1.509 .439+0 .190–1 .3105+1 0.940 .665+0 .112+0 .4511+1 0.927 .662+0 .114+0 .1030+1 1.999 –.303–1 –.332–4 .5566+0 1.498 .404+0 .161–1
3000 .1047+2 1.958 .805+0 –.136–3 .1222+2 1.997 .185+0 –.658–4 .9194+1 1.294 .841+0 .602–1 .1748+2 1.331 .862+0 .587–1 .4063+1 1.998 .127+0 –.399–4 .2894+1 1.359 .682+0 .354–1 .5450+1 1.391 .699+0 .347–1 .7411+0 0.773 .816+0 .162+0 .1071+1 0.767 .813+0 .164+0 .4643+0 1.998 .117+0 –.361–4 .2007+0 1.371 .663+0 .325–1
4000 .8823+1 1.948 .103+1 –.131–3 .8058+1 1.992 .376+0 –.625–4 .4950+1 1.208 .101+1 .775–1 .9303+1 1.245 .104+1 .751–1 .2318+1 1.994 .308+0 –.406–4 .1368+1 1.253 .871+0 .534–1 .2548+1 1.285 .893+0 .518–1 .2547+0 0.655 .911+0 .209+0 .3663+0 0.656 .909+0 .212+0 .2565+0 1.995 .295+0 –.374–4 .9246–1 1.262 .857+0 .508–1
5000 .7507+1 1.938 .122+1 –.126–3 .5628+1 1.986 .562+0 –.592–4 .2930+1 1.128 .115+1 .951–1 .5456+1 1.165 .117+1 .919–1 .1470+1 1.989 .488+0 –.404–4 .7417+0 1.160 .102+1 .719–1 .1371+1 1.193 .104+1 .695–1 .1082+0 0.566 .977+0 .253+0 .1550+0 0.573 .978+0 .256+0 .1593+0 1.990 .477+0 –.377–4 .4935–1 1.166 .101+1 .695–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables As, Z = 33 (continued) Shell 4 p3/2 Eb = 9 eV
σ β γ δ
100 .9447+2 0.720 .108+0 .146–1
200 .5464+2 1.366 .117+0 .108–2
500 .1707+2 1.652 –.217–1 .492–4
1000 .4904+1 1.650 .815–1 .472–2
E (eV) 1500 .2051+1 1.590 .253+0 .100–1
2000 .1041+1 1.525 .416+0 .165–1
3000 .3703+0 1.402 .681+0 .319–1
4000 .1689+0 1.294 .879+0 .493–1
5000 .8944–1 1.199 .103+1 .672–1
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1711+2 1.985 –.684+0 –.155–3 .7359+2 1.984 .672+0 –.338–4 .1687+3 1.051 –.181+0 –.253–3 .3484+3 1.054 –.183+0 –.857–3 .1822+3 1.993 .361+0 .367–5 .2724+3 0.991 .179+0 .359–1 .5911+3 0.981 .168+0 .332–1 .2876+4 0.644 –.586–2 .121–1 .4327+4 0.660 –.537–2 .114–1
200 .1675+2 1.984 –.521+0 –.163–3 .6721+2 1.986 .453+0 –.522–4 .1450+3 1.220 –.168+0 .300–2 .2976+3 1.232 –.171+0 .331–2 .1307+3 1.992 .293+0 –.150–4 .2076+3 1.354 .119+0 .856–2 .4375+3 1.350 .110+0 .749–2 .1284+4 0.970 .189–1 .203–1 .1915+4 0.982 .202–1 .199–1
500 .1580+2 1.981 –.210+0 –.168–3 .5235+2 1.991 .123+0 –.718–4 .9500+2 1.387 –.107–1 .151–1 .1919+3 1.411 –.131–1 .162–1 .6134+2 1.993 .106+0 –.316–4 .9259+2 1.588 –.201–1 .807–3 .1872+3 1.597 –.220–1 .136–2 .2125+3 1.208 .153+0 .377–1 .3138+3 1.206 .155+0 .377–1
1000 .1438+2 1.976 .105+0 –.167–3 .3639+2 1.995 –.465–1 –.795–4 .5221+2 1.435 .239+0 .262–1 .1035+3 1.467 .242+0 .270–1 .2633+2 1.995 –.428–1 –.387–4 .3345+2 1.601 .840–1 .507–2 .6569+2 1.622 .871–1 .619–2 .3399+2 1.168 .374+0 .610–1 .4979+2 1.155 .374+0 .618–1
E (eV) 1500 .1311+2 1.971 .326+0 –.164–3 .2654+2 1.998 –.559–1 –.803–4 .3149+2 1.420 .432+0 .344–1 .6157+2 1.456 .441+0 .346–1 .1443+2 1.997 –.706–1 –.419–4 .1561+2 1.551 .249+0 .106–1 .3018+2 1.578 .256+0 .115–1 .9893+1 1.063 .540+0 .847–1 .1442+2 1.049 .538+0 .862–1
2000 .1198+2 1.966 .502+0 –.161–3 .2007+2 1.998 –.554–2 –.792–4 .2031+2 1.388 .590+0 .425–1 .3930+2 1.425 .603+0 .421–1 .9007+1 1.998 –.389–1 –.438–4 .8469+1 1.493 .405+0 .173–1 .1619+2 1.523 .416+0 .177–1 .3857+1 0.963 .662+0 .109+0 .5602+1 0.949 .659+0 .111+0
3000 .1009+2 1.957 .786+0 –.155–3 .1242+2 1.997 .158+0 –.762–4 .9755+1 1.306 .832+0 .589–1 .1856+2 1.345 .852+0 .573–1 .4366+1 1.998 .100+0 –.464–4 .3259+1 1.377 .662+0 .330–1 .6136+1 1.411 .680+0 .325–1 .9398+0 0.798 .822+0 .157+0 .1357+1 0.790 .818+0 .160+0
4000 .8578+1 1.947 .101+1 –.150–3 .8298+1 1.993 .343+0 –.728–4 .5344+1 1.224 .101+1 .756–1 .1005+2 1.264 .103+1 .731–1 .2511+1 1.995 .273+0 –.474–4 .1560+1 1.274 .857+0 .503–1 .2903+1 1.309 .880+0 .488–1 .3270+0 0.679 .922+0 .204+0 .4700+0 0.678 .920+0 .207+0
5000 .7355+1 1.937 .120+1 –.144–3 .5852+1 1.987 .525+0 –.692–4 .3204+1 1.148 .115+1 .931–1 .5963+1 1.188 .118+1 .896–1 .1600+1 1.990 .449+0 –.473–4 .8533+0 1.185 .101+1 .686–1 .1574+1 1.220 .103+1 .662–1 .1402+0 0.587 .991+0 .247+0 .2006+0 0.592 .991+0 .250+0
Se, Z = 34 Shell 1s1/2 Eb = 12662 eV 2s1/2 Eb = 1656 eV 2 p1/2 Eb = 1479 eV 2 p3/2 Eb = 1432 eV 3s1/2 Eb = 234 eV 3 p1/2 Eb = 173 eV 3 p3/2 Eb = 166 eV 3d3/2 Eb = 61 eV 3d5/2 Eb = 60 eV
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M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Se, Z = 34 (continued) Shell 4s1/2 Eb = 20 eV 4 p1/2 Eb = 10 eV 4 p3/2 Eb = 10 eV
σ β γ δ σ β γ δ σ β γ δ
100 .1076+3 1.995 .193+0 .948–5 .5522+2 0.678 .978–1 .170–1 .1183+3 0.693 .956–1 .167–1
200 .4702+2 1.995 .210+0 –.134–5 .3308+2 1.357 .135+0 .190–2 .6816+2 1.347 .127+0 .204–2
500 .1297+2 1.994 .100+0 –.162–4 .1089+2 1.646 –.171–1 –.718–3 .2147+2 1.650 –.192–1 –.163–3
1000 .4244+1 1.995 –.375–1 –.280–4 .3285+1 1.640 .615–1 .307–2 .6306+1 1.658 .648–1 .417–2
E (eV) 1500 .2076+1 1.997 –.698–1 –.348–4 .1413+1 1.578 .223+0 .808–2 .2674+1 1.603 .230+0 .906–2
2000 .1218+1 1.998 –.427–1 –.385–4 .7325+0 1.513 .379+0 .145–1 .1372+1 1.542 .391+0 .151–1
3000 .5530+0 1.998 .904–1 –.420–4 .2682+0 1.390 .640+0 .298–1 .4952+0 1.422 .659+0 .294–1
4000 .3069+0 1.995 .261+0 –.437–4 .1248+0 1.283 .839+0 .471–1 .2280+0 1.317 .862+0 .457–1
5000 .1913+0 1.991 .437+0 –.443–4 .6708–1 1.190 .993+0 .651–1 .1215+0 1.225 .102+1 .628–1
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1602+2 1.983 –.716+0 –.177–3 .6865+2 1.983 .700+0 –.368–4 .1557+3 1.043 –.191+0 –.117–2 .3206+3 1.046 –.194+0 –.178–2 .1731+3 1.992 .384+0 .576–5 .2615+3 0.976 .184+0 .411–1 .5701+3 0.966 .173+0 .381–1
200 .1571+2 1.982 –.551+0 –.187–3 .6307+2 1.985 .480+0 –.580–4 .1354+3 1.210 –.181+0 .214–2 .2771+3 1.223 –.185+0 .252–2 .1268+3 1.992 .312+0 –.155–4 .2025+3 1.338 .134+0 .109–1 .4287+3 1.333 .124+0 .959–2
500 .1485+2 1.979 –.237+0 –.192–3 .4981+2 1.990 .143+0 –.807–4 .9091+2 1.379 –.273–1 .145–1 .1833+3 1.405 –.304–1 .158–1 .6163+2 1.992 .122+0 –.355–4 .9403+2 1.581 –.186–1 .798–3 .1908+3 1.591 –.213–1 .132–2
1000 .1359+2 1.975 .808–1 –.190–3 .3530+2 1.995 –.401–1 –.902–4 .5159+2 1.433 .222+0 .259–1 .1021+3 1.466 .225+0 .269–1 .2717+2 1.995 –.355–1 –.444–4 .3529+2 1.604 .689–1 .453–2 .6946+2 1.626 .718–1 .575–2
E (eV) 1500 .1245+2 1.970 .304+0 –.186–3 .2612+2 1.997 –.611–1 –.916–4 .3183+2 1.423 .416+0 .340–1 .6216+2 1.460 .426+0 .344–1 .1510+2 1.997 –.732–1 –.482–4 .1685+2 1.560 .228+0 .970–2 .3261+2 1.588 .235+0 .108–1
2000 .1144+2 1.965 .481+0 –.183–3 .1998+2 1.998 –.196–1 –.907–4 .2090+2 1.393 .575+0 .419–1 .4036+2 1.433 .590+0 .417–1 .9519+1 1.998 –.504–1 –.505–4 .9282+1 1.505 .382+0 .160–1 .1776+2 1.537 .394+0 .166–1
3000 .9722+1 1.955 .766+0 –.177–3 .1258+2 1.997 .132+0 –.879–4 .1029+2 1.318 .821+0 .577–1 .1954+2 1.359 .844+0 .562–1 .4672+1 1.998 .754–1 –.537–4 .3645+1 1.394 .642+0 .309–1 .6858+1 1.429 .661+0 .304–1
4000 .8330+1 1.946 .994+0 –.171–3 .8511+1 1.993 .310+0 –.845–4 .5732+1 1.239 .100+1 .739–1 .1075+2 1.281 .103+1 .713–1 .2708+1 1.995 .240+0 –.551–4 .1766+1 1.295 .841+0 .474–1 .3283+1 1.331 .865+0 .460–1
5000 .7193+1 1.936 .119+1 –.164–3 .6060+1 1.988 .488+0 –.806–4 .3480+1 1.166 .114+1 .908–1 .6463+1 1.208 .118+1 .873–1 .1735+1 1.991 .411+0 –.552–4 .9747+0 1.207 .998+0 .650–1 .1796+1 1.244 .103+1 .627–1
Br, Z = 35 Shell 1s1/2 Eb = 13481 eV 2s1/2 Eb = 1787 eV 2 p1/2 Eb = 1602 eV 2 p3/2 Eb = 1556 eV 3s1/2 Eb = 262 eV 3 p1/2 Eb = 197 eV 3 p3/2 Eb = 189 eV
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Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Br, Z = 35 (continued) Shell 3d3/2 Eb = 77 eV 3d5/2 Eb = 76 eV 4s1/2 Eb = 24 eV 4 p1/2 Eb = 12 eV 4 p3/2 Eb = 12 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2758+4 0.616 –.101–1 .116–1 .4150+4 0.633 –.966–2 .108–1 .1180+3 1.994 .198+0 .121–4 .6479+2 0.645 .838–1 .192–1 .1399+3 0.662 .826–1 .187–1
200 .1314+4 0.949 .123–1 .199–1 .1962+4 0.962 .137–1 .194–1 .5288+2 1.994 .218+0 –.857–6 .3917+2 1.338 .145+0 .306–2 .8120+2 1.330 .137+0 .317–2
500 .2357+3 1.204 .143+0 .374–1 .3481+3 1.202 .146+0 .373–1 .1477+2 1.994 .112+0 –.187–4 .1307+2 1.644 –.124–1 –.860–3 .2586+2 1.646 –.153–1 –.334–3
1000 .3974+2 1.178 .363+0 .600–1 .5821+2 1.166 .364+0 .607–1 .4879+1 1.995 –.298–1 –.318–4 .4033+1 1.646 .465–1 .250–2 .7756+1 1.665 .495–1 .368–2
E (eV) 1500 .1188+2 1.081 .531+0 .829–1 .1732+2 1.066 .530+0 .843–1 .2401+1 1.997 –.713–1 –.396–4 .1761+1 1.589 .200+0 .709–2 .3336+1 1.615 .208+0 .822–2
2000 .4715+1 0.984 .658+0 .107+0 .6844+1 0.970 .655+0 .109+0 .1414+1 1.998 –.533–1 –.440–4 .9226+0 1.527 .355+0 .130–1 .1729+1 1.557 .366+0 .137–1
3000 .1173+1 0.822 .827+0 .153+0 .1692+1 0.813 .823+0 .156+0 .6457+0 1.998 .660–1 –.486–4 .3428+0 1.408 .618+0 .274–1 .6328+0 1.442 .636+0 .272–1
4000 .4133+0 0.703 .933+0 .198+0 .5933+0 0.699 .929+0 .202+0 .3600+0 1.996 .228+0 –.507–4 .1611+0 1.304 .821+0 .439–1 .2941+0 1.340 .845+0 .427–1
5000 .1787+0 0.609 .100+1 .241+0 .2556+0 0.612 .100+1 .244+0 .2252+0 1.992 .398+0 –.516–4 .8720–1 1.214 .980+0 .613–1 .1578+0 1.250 .101+1 .590–1
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1503+2 1.982 –.748+0 –.201–3 .6401+2 1.982 .728+0 –.400–4 .1439+3 1.035 –.202+0 –.217–2 .2968+3 1.037 –.205+0 –.279–2 .1643+3 1.991 .407+0 .833–5
200 .1475+2 1.981 –.580+0 –.211–3 .5915+2 1.984 .507+0 –.642–4 .1264+3 1.202 –.194+0 .115–2 .2592+3 1.215 –.199+0 .161–2 .1228+3 1.991 .331+0 –.159–4
500 .1398+2 1.978 –.265+0 –.218–3 .4734+2 1.988 .165+0 –.906–4 .8691+2 1.372 –.439–1 .139–1 .1756+3 1.398 –.477–1 .153–1 .6173+2 1.991 .139+0 –.398–4
1000 .1285+2 1.973 .563–1 –.216–3 .3415+2 1.994 –.324–1 –.102–3 .5081+2 1.430 .204+0 .255–1 .1007+3 1.465 .207+0 .267–1 .2793+2 1.994 –.272–1 –.506–4
E (eV) 1500 .1184+2 1.968 .281+0 –.211–3 .2563+2 1.997 –.648–1 –.104–3 .3205+2 1.424 .400+0 .336–1 .6264+2 1.463 .410+0 .342–1 .1575+2 1.996 –.742–1 –.552–4
2000 .1093+2 1.964 .459+0 –.207–3 .1983+2 1.998 –.320–1 –.104–3 .2140+2 1.398 .561+0 .414–1 .4135+2 1.440 .576+0 .412–1 .1002+2 1.997 –.601–1 –.581–4
3000 .9361+1 1.954 .746+0 –.201–3 .1270+2 1.997 .108+0 –.101–3 .1079+2 1.328 .810+0 .567–1 .2049+2 1.371 .834+0 .552–1 .4978+1 1.998 .522–1 –.619–4
4000 .8082+1 1.944 .975+0 –.194–3 .8694+1 1.994 .279+0 –.975–4 .6113+1 1.253 .996+0 .723–1 .1146+2 1.298 .103+1 .696–1 .2908+1 1.996 .208+0 –.637–4
5000 .7026+1 1.935 .117+1 –.187–3 .6248+1 1.989 .453+0 –.936–4 .3758+1 1.182 .114+1 .886–1 .6969+1 1.227 .118+1 .850–1 .1874+1 1.992 .375+0 –.641–4
Kr, Z = 36 Shell 1s1/2 Eb = 14327 eV 2s1/2 Eb = 1927 eV 2 p1/2 Eb = 1731 eV 2 p3/2 Eb = 1678 eV 3s1/2 Eb = 292 eV
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M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Kr, Z = 36 (continued) Shell 3 p1/2 Eb = 222 eV 3 p3/2 Eb = 214 eV 3d3/2 Eb = 95 eV 3d5/2 Eb = 94 eV 4s1/2 Eb = 27 eV 4 p1/2 Eb = 15 eV 4 p3/2 Eb = 14 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2511+3 0.961 .189+0 .465–1 .5482+3 0.951 .177+0 .433–1 .2623+4 0.588 –.143–1 .109–1 .3948+4 0.607 –.139–1 .100–1 .1282+3 1.993 .200+0 .151–4 .7276+2 0.610 .688–1 .213–1 .1597+3 0.628 .684–1 .206–1
200 .1972+3 1.324 .150+0 .134–1 .4187+3 1.318 .139+0 .120–1 .1329+4 0.928 .565–2 .194–1 .1985+4 0.942 .709–2 .189–1 .5882+2 1.993 .224+0 –.177–6 .4487+2 1.320 .156+0 .440–2 .9401+2 1.309 .145+0 .442–2
500 .9518+2 1.575 –.157–1 .877–3 .1936+3 1.584 –.192–1 .137–2 .2578+3 1.199 .133+0 .371–1 .3807+3 1.198 .136+0 .370–1 .1662+2 1.993 .124+0 –.211–4 .1524+2 1.641 –.627–2 –.943–3 .3032+2 1.642 –.987–2 –.454–3
1000 .3705+2 1.606 .550–1 .403–2 .7303+2 1.629 .575–1 .536–2 .4580+2 1.188 .353+0 .591–1 .6708+2 1.175 .354+0 .598–1 .5533+1 1.994 –.213–1 –.362–4 .4806+1 1.652 .329–1 .197–2 .9264+1 1.671 .355–1 .323–2
E (eV) 1500 .1807+2 1.567 .207+0 .887–2 .3501+2 1.596 .215+0 .101–1 .1406+2 1.098 .523+0 .812–1 .2048+2 1.082 .522+0 .826–1 .2738+1 1.996 –.715–1 –.450–4 .2130+1 1.600 .179+0 .614–2 .4039+1 1.626 .186+0 .741–2
2000 .1011+2 1.516 .360+0 .148–1 .1934+2 1.549 .372+0 .156–1 .5676+1 1.005 .653+0 .104+0 .8234+1 0.989 .650+0 .106+0 .1618+1 1.997 –.620–1 –.500–4 .1127+1 1.541 .330+0 .115–1 .2113+1 1.571 .342+0 .124–1
3000 .4048+1 1.410 .621+0 .288–1 .7613+1 1.447 .641+0 .285–1 .1442+1 0.846 .830+0 .149+0 .2079+1 0.835 .825+0 .152+0 .7428+0 1.998 .435–1 –.559–4 .4247+0 1.426 .594+0 .252–1 .7837+0 1.462 .613+0 .251–1
4000 .1986+1 1.314 .824+0 .446–1 .3688+1 1.352 .850+0 .433–1 .5147+0 0.726 .942+0 .193+0 .7383+0 0.721 .938+0 .197+0 .4161+0 1.996 .196+0 –.585–4 .2016+0 1.325 .801+0 .409–1 .3676+0 1.362 .826+0 .397–1
5000 .1106+1 1.228 .986+0 .616–1 .2034+1 1.268 .102+1 .593–1 .2246+0 0.631 .102+1 .235+0 .3208+0 0.632 .102+1 .238+0 .2611+0 1.992 .361+0 –.595–4 .1099+0 1.236 .965+0 .576–1 .1986+0 1.275 .994+0 .554–1
σ β γ δ σ β γ δ σ β γ δ
100 .1410+2 1.981 –.769+0 –.228–3 .5978+2 1.981 .736+0 –.456–4 .1325+3 1.040 –.215+0 –.354–2
200 .1386+2 1.980 –.603+0 –.240–3 .5553+2 1.983 .522+0 –.718–4 .1175+3 1.199 –.205+0 .364–3
500 .1317+2 1.977 –.287+0 –.247–3 .4500+2 1.988 .181+0 –.101–3 .8259+2 1.367 –.573–1 .134–1
1000 .1216+2 1.972 .343–1 –.243–3 .3300+2 1.993 –.243–1 –.115–3 .4967+2 1.428 .188+0 .251–1
E (eV) 1500 .1125+2 1.967 .261+0 –.240–3 .2510+2 1.996 –.667–1 –.118–3 .3201+2 1.425 .385+0 .333–1
2000 .1043+2 1.962 .440+0 –.235–3 .1962+2 1.998 –.421–1 –.118–3 .2173+2 1.402 .547+0 .410–1
3000 .9004+1 1.953 .727+0 –.228–3 .1277+2 1.997 .860–1 –.116–3 .1122+2 1.337 .798+0 .556–1
4000 .7828+1 1.943 .954+0 –.220–3 .8848+1 1.994 .249+0 –.112–3 .6466+1 1.267 .988+0 .710–1
5000 .6849+1 1.933 .115+1 –.213–3 .6417+1 1.990 .419+0 –.108–3 .4026+1 1.197 .114+1 .862–1
Rb, Z = 37 Shell 1s1/2 Eb = 15203 eV 2s1/2 Eb = 2068 eV 2 p1/2 Eb = 1867 eV
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M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Rb, Z = 37 (continued) Shell 2 p3/2 Eb = 1808 eV 3s1/2 Eb = 325 eV 3 p1/2 Eb = 251 eV 3 p3/2 Eb = 242 eV 3d3/2 Eb = 116 eV 3d5/2 Eb = 114 eV 4s1/2 Eb = 32 eV 4 p1/2 Eb = 16 eV 4 p3/2 Eb = 15 eV 5s1/2 Eb = 4 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2735+3 1.043 –.219+0 –.409–2 .1548+3 1.990 .422+0 .884–5 .2405+3 0.980 .196+0 .486–1 .5266+3 0.969 .184+0 .452–1 .2454+4 0.588 –.182–1 .102–1 .3709+4 0.607 –.178–1 .937–2 .1408+3 1.992 .203+0 .163–4 .9290+2 0.661 .695–1 .209–1 .2066+3 0.677 .690–1 .202–1 .1321+2 1.992 .183+0 .225–4
200 .2410+3 1.213 –.212+0 .940–3 .1179+3 1.990 .344+0 –.170–4 .1905+3 1.318 .158+0 .152–1 .4058+3 1.313 .146+0 .136–1 .1298+4 0.917 .567–4 .190–1 .1944+4 0.933 .156–2 .184–1 .6644+2 1.993 .227+0 –.279–6 .5656+2 1.318 .156+0 .531–2 .1201+3 1.306 .145+0 .527–2 .4951+1 1.993 .225+0 .458–5
500 .1670+3 1.394 –.618–1 .150–1 .6130+2 1.991 .151+0 –.443–4 .9517+2 1.570 –.123–1 .105–2 .1943+3 1.579 –.166–1 .151–2 .2732+3 1.195 .124+0 .366–1 .4041+3 1.194 .127+0 .365–1 .1907+2 1.993 .132+0 –.233–4 .1914+2 1.640 –.553–3 –.902–3 .3851+2 1.641 –.493–2 –.434–3 .1219+1 1.993 .137+0 –.195–4
1000 .9854+2 1.464 .191+0 .264–1 .2850+2 1.993 –.190–1 –.573–4 .3842+2 1.607 .434–1 .360–2 .7590+2 1.631 .456–1 .502–2 .5146+2 1.196 .342+0 .582–1 .7540+2 1.184 .344+0 .588–1 .6413+1 1.994 –.133–1 –.407–4 .6132+1 1.658 .218–1 .150–2 .1194+2 1.676 .239–1 .281–2 .3853+0 1.994 –.107–1 –.392–4
134
E (eV) 1500 .6259+2 1.466 .395+0 .340–1 .1631+2 1.995 –.740–1 –.631–4 .1917+2 1.573 .189+0 .813–2 .3717+2 1.603 .197+0 .951–2 .1626+2 1.112 .515+0 .795–1 .2369+2 1.096 .514+0 .809–1 .3195+1 1.995 –.706–1 –.506–4 .2756+1 1.609 .159+0 .522–2 .5275+1 1.636 .166+0 .663–2 .1878+0 1.995 –.702–1 –.484–4
2000 .4199+2 1.446 .563+0 .410–1 .1047+2 1.997 –.676–1 –.664–4 .1089+2 1.526 .339+0 .138–1 .2084+2 1.560 .351+0 .147–1 .6689+1 1.023 .648+0 .102+0 .9703+1 1.006 .645+0 .104+0 .1896+1 1.997 –.683–1 –.568–4 .1472+1 1.553 .307+0 .104–1 .2785+1 1.584 .319+0 .115–1 .1101+0 1.997 –.689–1 –.560–4
3000 .2130+2 1.383 .823+0 .542–1 .5272+1 1.998 .317–1 –.710–4 .4450+1 1.425 .600+0 .269–1 .8367+1 1.463 .620+0 .268–1 .1741+1 0.869 .832+0 .146+0 .2509+1 0.856 .827+0 .149+0 .8755+0 1.998 .239–1 –.641–4 .5628+0 1.442 .569+0 .231–1 .1047+1 1.479 .589+0 .232–1 .5028–1 1.998 .209–1 –.625–4
4000 .1211+2 1.314 .102+1 .683–1 .3105+1 1.996 .179+0 –.733–4 .2212+1 1.333 .807+0 .422–1 .4105+1 1.373 .833+0 .409–1 .6301+0 0.749 .950+0 .189+0 .9032+0 0.742 .945+0 .193+0 .4928+0 1.996 .166+0 –.673–4 .2698+0 1.345 .780+0 .380–1 .4958+0 1.384 .805+0 .370–1 .2812–1 1.996 .164+0 –.664–4
5000 .7455+1 1.244 .117+1 .825–1 .2013+1 1.993 .340+0 –.743–4 .1244+1 1.248 .972+0 .581–1 .2284+1 1.289 .100+1 .559–1 .2777+0 0.654 .103+1 .230+0 .3962+0 0.653 .103+1 .233+0 .3104+0 1.993 .325+0 –.689–4 .1482+0 1.257 .948+0 .540–1 .2697+0 1.297 .978+0 .520–1 .1765–1 1.993 .322+0 –.685–4
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Sr, Z = 38 Shell 1s1/2 Eb = 16108 eV 2s1/2 Eb = 2219 eV 2 p1/2 Eb = 2010 eV 2 p3/2 Eb = 1943 eV 3s1/2 Eb = 361 eV 3 p1/2 Eb = 283 eV 3 p3/2 Eb = 273 eV 3d3/2 Eb = 139 eV 3d5/2 Eb = 137 eV 4s1/2 Eb = 40 eV 4 p1/2 Eb = 23 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1324+2 1.979 –.794+0 –.260–3 .5578+2 1.980 .750+0 –.515–4 .1222+3 1.041 –.229+0 –.491–2 .2526+3 1.044 –.233+0 –.540–2 .1456+3 1.989 .440+0 .976–5 .2293+3 0.988 .202+0 .509–1 .5032+3 0.976 .189+0 .474–1 .2290+4 0.586 –.225–1 .937–2 .3458+4 0.607 –.222–1 .853–2 .1510+3 1.992 .211+0 .182–4 .1086+3 0.689 .700–1 .222–1
200 .1304+2 1.978 –.627+0 –.272–3 .5208+2 1.982 .538+0 –.803–4 .1092+3 1.196 –.218+0 –.452–3 .2244+3 1.210 –.225+0 .249–3 .1128+3 1.989 .359+0 –.182–4 .1832+3 1.312 .167+0 .170–1 .3916+3 1.306 .153+0 .153–1 .1258+4 0.906 –.591–2 .185–1 .1884+4 0.923 –.434–2 .179–1 .7311+2 1.992 .233+0 –.372–6 .6581+2 1.314 .161+0 .620–2
500 .1242+2 1.975 –.309+0 –.278–3 .4272+2 1.987 .197+0 –.113–3 .7842+2 1.362 –.706–1 .129–1 .1588+3 1.390 –.758–1 .146–1 .6063+2 1.990 .164+0 –.491–4 .9470+2 1.565 –.829–2 .129–2 .1940+3 1.575 –.134–1 .172–2 .2865+3 1.190 .115+0 .362–1 .4237+3 1.190 .119+0 .360–1 .2149+2 1.992 .141+0 –.260–4 .2259+2 1.639 .589–2 –.849–3
1000 .1151+2 1.970 .128–1 –.275–3 .3182+2 1.992 –.157–1 –.129–3 .4843+2 1.425 .173+0 .248–1 .9620+2 1.463 .176+0 .263–1 .2896+2 1.992 –.104–1 –.647–4 .3962+2 1.608 .332–1 .324–2 .7844+2 1.632 .350–1 .475–2 .5713+2 1.203 .333+0 .576–1 .8369+2 1.190 .335+0 .581–1 .7312+1 1.993 –.508–2 –.458–4 .7387+1 1.662 .125–1 .113–2
135
E (eV) 1500 .1070+2 1.966 .239+0 –.270–3 .2450+2 1.995 –.670–1 –.133–3 .3185+2 1.425 .370+0 .330–1 .6234+2 1.468 .379+0 .338–1 .1682+2 1.995 –.723–1 –.715–4 .2020+2 1.579 .172+0 .748–2 .3923+2 1.610 .179+0 .901–2 .1858+2 1.126 .507+0 .783–1 .2706+2 1.109 .506+0 .797–1 .3670+1 1.995 –.682–1 –.569–4 .3372+1 1.618 .140+0 .447–2
2000 .9953+1 1.961 .420+0 –.266–3 .1935+2 1.997 –.506–1 –.134–3 .2196+2 1.405 .533+0 .405–1 .4248+2 1.451 .548+0 .406–1 .1091+2 1.996 –.735–1 –.756–4 .1165+2 1.534 .319+0 .127–1 .2232+2 1.570 .331+0 .139–1 .7788+1 1.041 .642+0 .997–1 .1129+2 1.023 .639+0 .102+0 .2189+1 1.996 –.736–1 –.642–4 .1821+1 1.564 .285+0 .919–2
3000 .8657+1 1.951 .709+0 –.258–3 .1280+2 1.997 .658–1 –.132–3 .1161+2 1.344 .787+0 .548–1 .2204+2 1.393 .813+0 .534–1 .5561+1 1.998 .131–1 –.812–4 .4861+1 1.438 .579+0 .252–1 .9138+1 1.478 .600+0 .253–1 .2076+1 0.889 .832+0 .142+0 .2989+1 0.875 .827+0 .145+0 .1017+1 1.998 .623–2 –.730–4 .7063+0 1.457 .546+0 .211–1
4000 .7577+1 1.942 .939+0 –.250–3 .8970+1 1.995 .222+0 –.128–3 .6803+1 1.277 .980+0 .694–1 .1273+2 1.327 .101+1 .667–1 .3303+1 1.996 .151+0 –.841–4 .2448+1 1.349 .789+0 .396–1 .4541+1 1.391 .816+0 .385–1 .7625+0 0.771 .957+0 .184+0 .1092+1 0.761 .951+0 .188+0 .5750+0 1.996 .139+0 –.771–4 .3421+0 1.362 .759+0 .353–1
5000 .6669+1 1.932 .113+1 –.241–3 .6566+1 1.990 .387+0 –.124–3 .4289+1 1.211 .113+1 .848–1 .7933+1 1.261 .117+1 .809–1 .2154+1 1.993 .306+0 –.851–4 .1390+1 1.267 .958+0 .554–1 .2549+1 1.310 .991+0 .533–1 .3393+0 0.673 .104+1 .224+0 .4836+0 0.671 .104+1 .228+0 .3636+0 1.993 .291+0 –.789–4 .1894+0 1.278 .932+0 .510–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Sr, Z = 38 (continued) Shell 4 p3/2 Eb = 22 eV 5s1/2 Eb = 5 eV
σ β γ δ σ β γ δ
100 .2433+3 0.703 .696–1 .214–1 .2257+2 1.991 .180+0 .236–4
200 .1407+3 1.302 .150+0 .607–2 .9107+1 1.992 .232+0 .657–5
500 .4574+2 1.640 .695–3 –.413–3 .2184+1 1.992 .145+0 –.223–4
1000 .1446+2 1.681 .142–1 .250–2 .6882+0 1.993 –.229–2 –.435–4
E (eV) 1500 .6481+1 1.646 .147+0 .602–2 .3360+0 1.995 –.675–1 –.554–4
2000 .3456+1 1.597 .297+0 .105–1 .1976+0 1.996 –.745–1 –.637–4
3000 .1317+1 1.496 .566+0 .214–1 .9048–1 1.998 .400–2 –.709–4
4000 .6299+0 1.403 .785+0 .344–1 .5078–1 1.996 .137+0 –.763–4
5000 .3451+0 1.320 .964+0 .491–1 .3196–1 1.994 .289+0 –.780–4
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1246+2 1.978 –.825+0 –.293–3 .5220+2 1.979 .772+0 –.566–4 .1133+3 1.038 –.242+0 –.643–2 .2344+3 1.041 –.247+0 –.691–2 .1376+3 1.988 .464+0 .120–4 .2186+3 0.984 .208+0 .554–1 .4824+3 0.971 .194+0 .515–1 .2154+4 0.571 –.269–1 .828–2
200 .1228+2 1.976 –.654+0 –.307–3 .4895+2 1.981 .560+0 –.891–4 .1019+3 1.191 –.232+0 –.159–2 .2097+3 1.206 –.239+0 –.777–3 .1083+3 1.988 .377+0 –.189–4 .1764+3 1.303 .179+0 .196–1 .3794+3 1.297 .164+0 .176–1 .1229+4 0.889 –.126–1 .178–1
500 .1173+2 1.974 –.334+0 –.314–3 .4060+2 1.985 .217+0 –.126–3 .7466+2 1.355 –.856–1 .123–1 .1514+3 1.385 –.918–1 .142–1 .6001+2 1.989 .179+0 –.544–4 .9426+2 1.558 –.292–2 .162–2 .1940+3 1.568 –.909–2 .199–2 .3005+3 1.183 .105+0 .358–1
1000 .1092+2 1.969 –.104–1 –.312–3 .3069+2 1.991 –.564–2 –.145–3 .4723+2 1.422 .158+0 .246–1 .9394+2 1.462 .159+0 .263–1 .2941+2 1.992 –.636–3 –.732–4 .4079+2 1.609 .234–1 .290–2 .8103+2 1.633 .247–1 .451–2 .6317+2 1.208 .324+0 .570–1
E (eV) 1500 .1018+2 1.964 .218+0 –.307–3 .2391+2 1.995 –.668–1 –.151–3 .3166+2 1.425 .355+0 .328–1 .6202+2 1.470 .365+0 .338–1 .1732+2 1.994 –.703–1 –.815–4 .2124+2 1.584 .156+0 .686–2 .4133+2 1.616 .163+0 .856–2 .2111+2 1.138 .498+0 .767–1
2000 .9506+1 1.959 .399+0 –.300–3 .1907+2 1.997 –.580–1 –.151–3 .2217+2 1.408 .518+0 .401–1 .4289+2 1.456 .534+0 .403–1 .1134+2 1.996 –.784–1 –.860–4 .1243+2 1.543 .299+0 .118–1 .2384+2 1.579 .311+0 .132–1 .9002+1 1.057 .636+0 .977–1
3000 .8325+1 1.950 .689+0 –.291–3 .1280+2 1.997 .464–1 –.150–3 .1198+2 1.352 .775+0 .540–1 .2274+2 1.402 .801+0 .526–1 .5852+1 1.997 –.431–2 –.925–4 .5287+1 1.451 .558+0 .236–1 .9943+1 1.493 .579+0 .238–1 .2455+1 0.910 .832+0 .139+0
4000 .7331+1 1.940 .919+0 –.282–3 .9074+1 1.995 .195+0 –.147–3 .7134+1 1.288 .970+0 .682–1 .1334+2 1.340 .100+1 .654–1 .3504+1 1.996 .125+0 –.961–4 .2698+1 1.365 .769+0 .373–1 .5002+1 1.409 .798+0 .364–1 .9144+0 0.792 .962+0 .180+0
5000 .6490+1 1.931 .112+1 –.273–3 .6700+1 1.991 .354+0 –.142–3 .4553+1 1.224 .113+1 .831–1 .8410+1 1.277 .117+1 .791–1 .2299+1 1.994 .273+0 –.976–4 .1545+1 1.285 .943+0 .525–1 .2833+1 1.331 .976+0 .504–1 .4109+0 0.694 .105+1 .219+0
Y, Z = 39 Shell 1s1/2 Eb = 17042 eV 2s1/2 Eb = 2376 eV 2 p1/2 Eb = 2158 eV 2 p3/2 Eb = 2083 eV 3s1/2 Eb = 398 eV 3 p1/2 Eb = 316 eV 3 p3/2 Eb = 304 eV 3d3/2 Eb = 163 eV
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M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Y, Z = 39 (continued) Shell 3d5/2 Eb = 161 eV 4s1/2 Eb = 49 eV 4 p1/2 Eb = 30 eV 4 p3/2 Eb = 29 eV 4d3/2 Eb = 6 eV 5s1/2 Eb = 6 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3251+4 0.593 –.267–1 .744–2 .1554+3 1.991 .222+0 .222–4 .1165+3 0.680 .636–1 .242–1 .2630+3 0.693 .638–1 .232–1 .1765+3 0.056 .191–1 –.177–1 .2676+2 1.990 .183+0 .272–4
200 .1840+4 0.908 –.110–1 .172–1 .7816+2 1.991 .243+0 .417–6 .7242+2 1.303 .169+0 .762–2 .1558+3 1.290 .157+0 .742–2 .1363+3 0.882 –.161–1 .321–2 .1097+2 1.991 .235+0 .890–5
500 .4444+3 1.185 .109+0 .355–1 .2362+2 1.991 .151+0 –.288–4 .2542+2 1.636 .140–1 –.776–3 .5169+2 1.636 .784–2 –.377–3 .2874+2 1.266 .729–1 .247–1 .2650+1 1.991 .155+0 –.243–4
1000 .9250+2 1.196 .326+0 .575–1 .8125+1 1.992 .407–2 –.516–4 .8472+1 1.666 .385–2 .787–3 .1662+2 1.685 .509–2 .223–2 .5197+1 1.262 .285+0 .463–1 .8331+0 1.992 .706–2 –.483–4
E (eV) 1500 .3072+2 1.120 .498+0 .782–1 .4106+1 1.994 –.654–1 –.643–4 .3923+1 1.626 .123+0 .379–2 .7551+1 1.654 .130+0 .548–2 .1610+1 1.174 .467+0 .667–1 .4078+0 1.994 –.645–1 –.620–4
2000 .1304+2 1.039 .633+0 .999–1 .2460+1 1.996 –.777–1 –.724–4 .2141+1 1.575 .263+0 .807–2 .4066+1 1.609 .275+0 .955–2 .6543+0 1.081 .611+0 .882–1 .2403+0 1.996 –.786–1 –.711–4
3000 .3531+1 0.894 .826+0 .142+0 .1150+1 1.997 –.103–1 –.829–4 .8417+0 1.472 .523+0 .193–1 .1570+1 1.512 .543+0 .198–1 .1690+0 0.920 .811+0 .130+0 .1104+0 1.997 –.127–1 –.812–4
4000 .1308+1 0.781 .956+0 .184+0 .6528+0 1.997 .113+0 –.880–4 .4116+0 1.380 .737+0 .327–1 .7574+0 1.423 .764+0 .321–1 .6116–1 0.799 .946+0 .172+0 .6215–1 1.997 .111+0 –.862–4
5000 .5850+0 0.690 .105+1 .223+0 .4143+0 1.994 .258+0 –.904–4 .2295+0 1.297 .914+0 .478–1 .4179+0 1.341 .947+0 .460–1 .2696–1 0.698 .104+1 .212+0 .3924–1 1.994 .256+0 –.894–4
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1174+2 1.976 –.855+0 –.330–3 .4899+2 1.977 .794+0 –.623–4 .1053+3 1.033 –.255+0 –.795–2 .2182+3 1.037 –.260+0 –.842–2
200 .1159+2 1.975 –.682+0 –.346–3 .4612+2 1.979 .582+0 –.986–4 .9539+2 1.184 –.245+0 –.271–2 .1965+3 1.200 –.254+0 –.179–2
500 .1110+2 1.972 –.360+0 –.354–3 .3865+2 1.984 .237+0 –.141–3 .7113+2 1.349 –.101+0 .116–1 .1445+3 1.380 –.108+0 .138–1
1000 .1036+2 1.967 –.344–1 –.350–3 .2961+2 1.990 .559–2 –.162–3 .4603+2 1.418 .140+0 .241–1 .9166+2 1.460 .141+0 .260–1
E (eV) 1500 .9694+1 1.962 .196+0 –.345–3 .2332+2 1.994 –.648–1 –.170–3 .3141+2 1.424 .339+0 .325–1 .6160+2 1.471 .348+0 .337–1
2000 .9084+1 1.958 .377+0 –.338–3 .1877+2 1.996 –.641–1 –.171–3 .2231+2 1.410 .503+0 .398–1 .4320+2 1.460 .518+0 .401–1
3000 .8006+1 1.948 .668+0 –.328–3 .1278+2 1.997 .283–1 –.170–3 .1233+2 1.358 .761+0 .532–1 .2339+2 1.412 .788+0 .519–1
4000 .7091+1 1.939 .900+0 –.319–3 .9160+1 1.995 .169+0 –.167–3 .7452+1 1.298 .960+0 .670–1 .1393+2 1.353 .996+0 .643–1
5000 .6311+1 1.929 .110+1 –.309–3 .6822+1 1.991 .323+0 –.162–3 .4812+1 1.237 .112+1 .814–1 .8880+1 1.292 .116+1 .774–1
Zr, Z = 40 Shell 1s1/2 Eb = 18002 eV 2s1/2 Eb = 2536 eV 2 p1/2 Eb = 2311 eV 2 p3/2 Eb = 2227 eV
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M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Zr, Z = 40 (continued) Shell 3s1/2 Eb = 435 eV 3 p1/2 Eb = 349 eV 3 p3/2 Eb = 335 eV 3d3/2 Eb = 187 eV 3d5/2 Eb = 184 eV 4s1/2 Eb = 56 eV 4 p1/2 Eb = 35 eV 4 p3/2 Eb = 33 eV 4d3/2 Eb = 8 eV 5s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1306+3 1.987 .485+0 .148–4 .2089+3 0.978 .213+0 .599–1 .4636+3 0.964 .198+0 .557–1 .2039+4 0.556 –.310–1 .704–2 .3087+4 0.579 –.308–1 .618–2 .1599+3 1.990 .229+0 .268–4 .1237+3 0.667 .553–1 .258–1 .2834+3 0.681 .559–1 .245–1 .2001+3 −.024 .345–1 –.197–1 .2972+2 1.989 .186+0 .313–4
200 .1042+3 1.987 .395+0 –.194–4 .1703+3 1.291 .191+0 .223–1 .3683+3 1.285 .175+0 .201–1 .1202+4 0.872 –.195–1 .170–1 .1804+4 0.892 –.179–1 .163–1 .8303+2 1.991 .251+0 .173–5 .7856+2 1.289 .174+0 .900–2 .1709+3 1.276 .161+0 .870–2 .1675+3 0.856 –.174–1 .104–2 .1230+2 1.991 .238+0 .123–4
500 .5941+2 1.988 .195+0 –.599–4 .9380+2 1.551 .352–2 .203–2 .1940+3 1.561 –.379–2 .233–2 .3140+3 1.176 .952–1 .353–1 .4650+3 1.178 .991–1 .350–1 .2573+2 1.991 .162+0 –.315–4 .2819+2 1.633 .233–1 –.663–3 .5765+2 1.631 .160–1 –.308–3 .3743+2 1.266 .611–1 .231–1 .3013+1 1.991 .166+0 –.269–4
1000 .2983+2 1.991 .100–1 –.819–4 .4190+2 1.609 .143–1 .259–2 .8350+2 1.634 .149–1 .427–2 .6935+2 1.214 .312+0 .563–1 .1016+3 1.202 .315+0 .567–1 .8934+1 1.992 .138–1 –.575–4 .9548+1 1.670 –.362–2 .486–3 .1879+2 1.688 –.299–2 .197–2 .7017+1 1.273 .270+0 .445–1 .9444+0 1.992 .169–1 –.541–4
138
E (eV) 1500 .1781+2 1.993 –.667–1 –.921–4 .2225+2 1.588 .139+0 .624–2 .4340+2 1.621 .145+0 .811–2 .2379+2 1.150 .489+0 .755–1 .3463+2 1.132 .489+0 .768–1 .4540+1 1.993 –.612–1 –.722–4 .4478+1 1.634 .105+0 .314–2 .8634+1 1.662 .112+0 .497–2 .2219+1 1.190 .453+0 .643–1 .4633+0 1.993 –.600–1 –.700–4
2000 .1176+2 1.995 –.820–1 –.974–4 .1320+2 1.550 .278+0 .109–1 .2536+2 1.588 .290+0 .125–1 .1032+2 1.073 .629+0 .957–1 .1494+2 1.054 .627+0 .979–1 .2732+1 1.995 –.804–1 –.814–4 .2467+1 1.586 .241+0 .705–2 .4691+1 1.620 .252+0 .871–2 .9139+0 1.100 .600+0 .850–1 .2737+0 1.995 –.811–1 –.794–4
3000 .6141+1 1.997 –.201–1 –.105–3 .5725+1 1.464 .535+0 .220–1 .1077+2 1.507 .557+0 .225–1 .2875+1 0.931 .830+0 .136+0 .4134+1 0.913 .825+0 .139+0 .1284+1 1.997 –.254–1 –.935–4 .9828+0 1.487 .498+0 .175–1 .1833+1 1.529 .519+0 .182–1 .2400+0 0.944 .807+0 .126+0 .1262+0 1.997 –.274–1 –.914–4
4000 .3706+1 1.996 .994–1 –.109–3 .2958+1 1.380 .749+0 .351–1 .5483+1 1.426 .778+0 .344–1 .1086+1 0.814 .967+0 .176+0 .1553+1 0.801 .960+0 .180+0 .7317+0 1.996 .890–1 –.998–4 .4850+0 1.397 .714+0 .304–1 .8917+0 1.441 .742+0 .299–1 .8782–1 0.821 .947+0 .167+0 .7121–1 1.997 .862–1 –.985–4
5000 .2445+1 1.994 .241+0 –.111–3 .1710+1 1.302 .926+0 .497–1 .3132+1 1.350 .961+0 .477–1 .4928+0 0.715 .106+1 .214+0 .7009+0 0.708 .105+1 .218+0 .4659+0 1.994 .227+0 –.103–3 .2724+0 1.315 .894+0 .448–1 .4952+0 1.362 .928+0 .431–1 .3904–1 0.720 .105+1 .206+0 .4507–1 1.994 .224+0 –.101–3
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Nb, Z = 41 Shell 1s1/2 Eb = 18990 eV 2s1/2 Eb = 2702 eV 2 p1/2 Eb = 2469 eV 2 p3/2 Eb = 2375 eV 3s1/2 Eb = 473 eV 3 p1/2 Eb = 384 eV 3 p3/2 Eb = 367 eV 3d3/2 Eb = 212 eV 3d5/2 Eb = 209 eV 4s1/2 Eb = 62 eV 4 p1/2 Eb = 40 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1108+2 1.974 –.890+0 –.370–3 .4607+2 1.976 .824+0 –.671–4 .9836+2 1.023 –.267+0 –.951–2 .2041+3 1.026 –.272+0 –.100–1 .1244+3 1.985 .512+0 .198–4 .1992+3 0.959 .217+0 .668–1 .4456+3 0.944 .200+0 .619–1 .1947+4 0.533 –.345–1 .566–2 .2947+4 0.557 –.344–1 .479–2 .1613+3 1.988 .234+0 .344–4 .1239+3 0.620 .384–1 .278–1
200 .1095+2 1.973 –.715+0 –.389–3 .4354+2 1.978 .611+0 –.108–3 .8962+2 1.175 –.260+0 –.407–2 .1850+3 1.190 –.269+0 –.307–2 .1006+3 1.986 .419+0 –.188–4 .1642+3 1.275 .207+0 .260–1 .3581+3 1.267 .189+0 .235–1 .1184+4 0.848 –.270–1 .159–1 .1778+4 0.870 –.255–1 .153–1 .8676+2 1.990 .260+0 .449–5 .8195+2 1.264 .181+0 .109–1
500 .1052+2 1.970 –.389+0 –.399–3 .3684+2 1.983 .260+0 –.157–3 .6795+2 1.342 –.118+0 .108–1 .1382+3 1.374 –.127+0 .132–1 .5886+2 1.987 .214+0 –.657–4 .9327+2 1.542 .119–1 .258–2 .1941+3 1.552 .327–2 .277–2 .3287+3 1.166 .837–1 .348–1 .4869+3 1.170 .880–1 .344–1 .2765+2 1.990 .175+0 –.341–4 .3042+2 1.627 .349–1 –.509–3
1000 .9843+1 1.966 –.605–1 –.394–3 .2857+2 1.989 .186–1 –.182–3 .4490+2 1.414 .122+0 .236–1 .8954+2 1.458 .122+0 .258–1 .3023+2 1.990 .222–1 –.918–4 .4295+2 1.608 .573–2 .230–2 .8597+2 1.634 .554–2 .407–2 .7595+2 1.218 .300+0 .555–1 .1113+3 1.206 .304+0 .559–1 .9671+1 1.991 .248–1 –.640–4 .1047+2 1.673 –.102–1 .207–3
139
E (eV) 1500 .9241+1 1.961 .170+0 –.387–3 .2274+2 1.993 –.611–1 –.190–3 .3116+2 1.424 .320+0 .321–1 .6117+2 1.472 .329+0 .335–1 .1828+2 1.992 –.615–1 –.103–3 .2326+2 1.592 .122+0 .565–2 .4549+2 1.626 .128+0 .768–2 .2670+2 1.163 .480+0 .746–1 .3884+2 1.144 .481+0 .759–1 .4936+1 1.993 –.555–1 –.803–4 .4965+1 1.641 .879–1 .255–2
2000 .8687+1 1.956 .354+0 –.381–3 .1846+2 1.995 –.690–1 –.193–3 .2243+2 1.412 .486+0 .393–1 .4347+2 1.464 .502+0 .399–1 .1218+2 1.994 –.844–1 –.110–3 .1398+2 1.557 .258+0 .100–1 .2692+2 1.597 .270+0 .118–1 .1176+2 1.089 .622+0 .939–1 .1702+2 1.068 .620+0 .961–1 .2981+1 1.994 –.820–1 –.912–4 .2761+1 1.596 .219+0 .609–2
3000 .7701+1 1.947 .647+0 –.370–3 .1275+2 1.997 .112–1 –.193–3 .1265+2 1.364 .747+0 .525–1 .2401+2 1.420 .775+0 .514–1 .6431+1 1.996 –.349–1 –.119–3 .6175+1 1.475 .513+0 .206–1 .1163+2 1.521 .535+0 .213–1 .3346+1 0.950 .828+0 .133+0 .4806+1 0.931 .822+0 .136+0 .1408+1 1.996 –.395–1 –.105–3 .1114+1 1.501 .474+0 .159–1
4000 .6858+1 1.937 .879+0 –.359–3 .9230+1 1.995 .143+0 –.189–3 .7763+1 1.307 .949+0 .660–1 .1450+2 1.365 .986+0 .632–1 .3911+1 1.996 .754–1 –.124–3 .3231+1 1.395 .728+0 .331–1 .5987+1 1.443 .758+0 .325–1 .1281+1 0.834 .970+0 .171+0 .1829+1 0.820 .963+0 .176+0 .8050+0 1.996 .657–1 –.113–3 .5541+0 1.413 .691+0 .281–1
5000 .6135+1 1.927 .108+1 –.348–3 .6931+1 1.992 .292+0 –.185–3 .5071+1 1.248 .111+1 .799–1 .9350+1 1.306 .116+1 .758–1 .2595+1 1.994 .210+0 –.127–3 .1884+1 1.319 .908+0 .470–1 .3449+1 1.369 .944+0 .452–1 .5866+0 0.736 .107+1 .209+0 .8333+0 0.727 .106+1 .214+0 .5140+0 1.995 .196+0 –.117–3 .3133+0 1.333 .873+0 .419–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Nb, Z = 41 (continued) Shell 4 p3/2 Eb = 38 eV 4d3/2 Eb = 7 eV 5s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ
100 .2864+3 0.637 .409–1 .264–1 .1769+3 −.178 .583–1 –.229–1 .2651+2 1.987 .187+0 .382–4
200 .1794+3 1.251 .167+0 .105–1 .1741+3 0.812 –.168–1 –.154–2 .1071+2 1.990 .238+0 .172–4
500 .6238+2 1.625 .263–1 –.208–3 .4164+2 1.262 .480–1 .214–1 .2705+1 1.990 .177+0 –.251–4
1000 .2061+2 1.691 –.103–1 .173–2 .8024+1 1.283 .254+0 .427–1 .8511+0 1.991 .283–1 –.602–4
E (eV) 1500 .9569+1 1.670 .938–1 .451–2 .2583+1 1.205 .438+0 .619–1 .4175+0 1.992 –.544–1 –.780–4
2000 .5243+1 1.631 .230+0 .796–2 .1076+1 1.119 .587+0 .818–1 .2471+0 1.994 –.827–1 –.883–4
3000 .2072+1 1.544 .495+0 .168–1 .2867+0 0.966 .802+0 .122+0 .1143+0 1.996 –.410–1 –.103–3
4000 .1016+1 1.460 .720+0 .278–1 .1060+0 0.843 .947+0 .162+0 .6464–1 1.996 .629–1 –.111–3
5000 .5677+0 1.382 .908+0 .404–1 .4747–1 0.742 .105+1 .200+0 .4100–1 1.995 .193+0 –.115–3
100 .1047+2 1.973 –.923+0 –.415–3 .4337+2 1.975 .848+0 –.732–4 .9191+2 1.017 –.280+0 –.112–1 .1910+3 1.020 –.285+0 –.117–1 .1186+3 1.984 .534+0 .241–4 .1916+3 0.949 .219+0 .716–1 .4293+3 0.933 .202+0 .666–1
200 .1036+2 1.972 –.745+0 –.436–3 .4113+2 1.977 .635+0 –.119–3 .8421+2 1.168 –.274+0 –.537–2 .1741+3 1.183 –.284+0 –.427–2 .9702+2 1.984 .438+0 –.184–4 .1593+3 1.261 .219+0 .292–1 .3481+3 1.254 .199+0 .264–1
500 .9969+1 1.969 –.416+0 –.448–3 .3513+2 1.982 .282+0 –.174–3 .6485+2 1.335 –.135+0 .100–1 .1321+3 1.368 –.144+0 .126–1 .5820+2 1.986 .231+0 –.717–4 .9281+2 1.534 .205–1 .319–2 .1937+3 1.544 .105–1 .329–2
1000 .9360+1 1.964 –.855–1 –.442–3 .2757+2 1.988 .317–1 –.203–3 .4370+2 1.411 .104+0 .231–1 .8728+2 1.455 .104+0 .256–1 .3056+2 1.989 .343–1 –.102–3 .4395+2 1.607 –.129–2 .207–2 .8815+2 1.633 –.230–2 .390–2
E (eV) 1500 .8813+1 1.959 .146+0 –.434–3 .2215+2 1.992 –.567–1 –.213–3 .3081+2 1.422 .303+0 .317–1 .6056+2 1.473 .311+0 .333–1 .1872+2 1.991 –.558–1 –.116–3 .2423+2 1.596 .106+0 .511–2 .4746+2 1.631 .112+0 .731–2
2000 .8309+1 1.954 .332+0 –.428–3 .1813+2 1.994 –.725–1 –.217–3 .2247+2 1.413 .470+0 .390–1 .4359+2 1.467 .486+0 .397–1 .1258+2 1.993 –.856–1 –.124–3 .1475+2 1.564 .239+0 .922–2 .2843+2 1.604 .250+0 .112–1
3000 .7407+1 1.945 .626+0 –.415–3 .1268+2 1.996 –.417–2 –.217–3 .1293+2 1.369 .733+0 .519–1 .2455+2 1.428 .761+0 .508–1 .6714+1 1.996 –.477–1 –.134–3 .6630+1 1.486 .491+0 .192–1 .1248+2 1.533 .513+0 .202–1
4000 .6630+1 1.935 .859+0 –.403–3 .9279+1 1.995 .120+0 –.214–3 .8052+1 1.316 .937+0 .649–1 .1504+2 1.376 .975+0 .622–1 .4113+1 1.996 .532–1 –.140–3 .3511+1 1.409 .707+0 .312–1 .6502+1 1.459 .737+0 .308–1
5000 .5959+1 1.926 .106+1 –.392–3 .7024+1 1.992 .263+0 –.210–3 .5319+1 1.259 .110+1 .784–1 .9800+1 1.320 .115+1 .742–1 .2744+1 1.994 .181+0 –.144–3 .2066+1 1.335 .888+0 .445–1 .3777+1 1.387 .926+0 .428–1
Mo, Z = 42 Shell 1s1/2 Eb = 20006 eV 2s1/2 Eb = 2872 eV 2 p1/2 Eb = 2631 eV 2 p3/2 Eb = 2526 eV 3s1/2 Eb = 511 eV 3 p1/2 Eb = 416 eV 3 p3/2 Eb = 399 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
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TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Mo, Z = 42 (continued) Shell 3d3/2 Eb = 236 eV 3d5/2 Eb = 234 eV 4s1/2 Eb = 68 eV 4 p1/2 Eb = 44 eV 4 p3/2 Eb = 41 eV 4d3/2 Eb = 8 eV 4d5/2 Eb = 8 eV 5s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1864+4 0.518 –.374–1 .432–2 .2811+4 0.543 –.376–1 .347–2 .1640+3 1.987 .239+0 .414–4 .1284+3 0.597 .270–1 .290–1 .3016+3 0.616 .304–1 .274–1 .1831+3 −.283 .775–1 –.228–1 .2810+3 −.212 .769–1 –.236–1 .2792+2 1.986 .185+0 .448–4
200 .1160+4 0.829 –.338–1 .147–1 .1738+4 0.853 –.324–1 .141–1 .9068+2 1.988 .267+0 .714–5 .8674+2 1.246 .184+0 .125–1 .1920+3 1.232 .169+0 .120–1 .1985+3 0.777 –.136–1 –.351–2 .2956+3 0.820 –.144–1 –.321–2 .1133+2 1.988 .240+0 .201–4
500 .3410+3 1.157 .724–1 .342–1 .5044+3 1.162 .771–1 .338–1 .2968+2 1.989 .186+0 –.366–4 .3304+2 1.622 .462–1 –.297–3 .6817+2 1.618 .362–1 –.495–4 .5064+2 1.259 .360–1 .198–1 .7393+2 1.268 .398–1 .197–1 .2903+1 1.989 .187+0 –.269–4
1000 .8235+2 1.221 .288+0 .549–1 .1205+3 1.210 .293+0 .552–1 .1048+2 1.990 .354–1 –.709–4 .1154+2 1.676 –.151–1 –.218–4 .2280+2 1.694 –.160–1 .152–2 .1007+2 1.292 .238+0 .410–1 .1452+2 1.279 .243+0 .412–1 .9155+0 1.990 .391–1 –.651–4
E (eV) 1500 .2967+2 1.173 .469+0 .734–1 .4312+2 1.154 .471+0 .747–1 .5373+1 1.992 –.494–1 –.895–4 .5534+1 1.648 .725–1 .203–2 .1068+2 1.677 .779–1 .411–2 .3301+1 1.220 .423+0 .596–1 .4731+1 1.199 .425+0 .608–1 .4494+0 1.992 –.478–1 –.862–4
2000 .1327+2 1.103 .613+0 .919–1 .1919+2 1.082 .612+0 .942–1 .3257+1 1.994 –.823–1 –.102–3 .3104+1 1.605 .198+0 .523–2 .5900+1 1.641 .209+0 .729–2 .1393+1 1.137 .575+0 .788–1 .1986+1 1.113 .574+0 .810–1 .2664+0 1.993 –.818–1 –.991–4
3000 .3854+1 0.969 .825+0 .130+0 .5530+1 0.948 .819+0 .133+0 .1546+1 1.996 –.517–1 –.118–3 .1268+1 1.514 .450+0 .143–1 .2358+1 1.558 .471+0 .155–1 .3769+0 0.987 .796+0 .118+0 .5333+0 0.964 .791+0 .122+0 .1237+0 1.996 –.538–1 –.115–3
4000 .1496+1 0.855 .972+0 .168+0 .2133+1 0.838 .964+0 .172+0 .8870+0 1.996 .441–1 –.127–3 .6361+0 1.429 .667+0 .259–1 .1165+1 1.477 .697+0 .259–1 .1407+0 0.865 .946+0 .157+0 .1979+0 0.847 .939+0 .162+0 .7012–1 1.996 .415–1 –.125–3
5000 .6916+0 0.757 .108+1 .204+0 .9811+0 0.746 .107+1 .209+0 .5679+0 1.995 .168+0 –.132–3 .3619+0 1.351 .851+0 .391–1 .6549+0 1.401 .888+0 .378–1 .6353–1 0.764 .105+1 .194+0 .8892–1 0.751 .105+1 .200+0 .4457–1 1.995 .164+0 –.130–3
σ β γ δ σ β γ δ
100 .9903+1 1.971 –.950+0 –.464–3 .4086+2 1.973 .865+0 –.813–4
200 .9804+1 1.970 –.773+0 –.488–3 .3886+2 1.975 .654+0 –.132–3
500 .9458+1 1.967 –.442+0 –.502–3 .3347+2 1.980 .301+0 –.193–3
1000 .8906+1 1.962 –.109+0 –.496–3 .2657+2 1.987 .446–1 –.226–3
E (eV) 1500 .8408+1 1.957 .124+0 –.487–3 .2155+2 1.991 –.514–1 –.238–3
2000 .7948+1 1.953 .310+0 –.479–3 .1778+2 1.994 –.743–1 –.243–3
3000 .7122+1 1.943 .604+0 –.465–3 .1259+2 1.996 –.178–1 –.244–3
4000 .6407+1 1.934 .839+0 –.452–3 .9303+1 1.995 .975–1 –.241–3
5000 .5784+1 1.924 .104+1 –.440–3 .7098+1 1.993 .235+0 –.237–3
Tc, Z = 43 Shell 1s1/2 Eb = 21050 eV 2s1/2 Eb = 3048 eV
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Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Tc, Z = 43 (continued) Shell 2 p1/2 Eb = 2800 eV 2 p3/2 Eb = 2683 eV 3s1/2 Eb = 551 eV 3 p1/2 Eb = 451 eV 3 p3/2 Eb = 432 eV 3d3/2 Eb = 263 eV 3d5/2 Eb = 259 eV 4s1/2 Eb = 74 eV 4 p1/2 Eb = 49 eV 4 p3/2 Eb = 45 eV 4d3/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .8583+2 1.015 –.294+0 –.129–1 .1786+3 1.018 –.299+0 –.134–1 .1128+3 1.983 .552+0 .272–4 .1837+3 0.949 .223+0 .746–1 .4134+3 0.933 .205+0 .693–1 .1761+4 0.514 –.407–1 .308–2 .2670+4 0.540 –.408–1 .223–2 .1681+3 1.986 .244+0 .467–4 .1361+3 0.605 .247–1 .299–1 .3244+3 0.623 .281–1 .281–1 .2273+3 −.310 .825–1 –.179–1
200 .7902+2 1.163 –.288+0 –.664–2 .1636+3 1.179 –.299+0 –.541–2 .9329+2 1.983 .454+0 –.187–4 .1538+3 1.253 .227+0 .317–1 .3377+3 1.245 .206+0 .287–1 .1120+4 0.816 –.400–1 .136–1 .1684+4 0.840 –.385–1 .129–1 .9484+2 1.987 .271+0 .921–5 .9249+2 1.235 .185+0 .137–1 .2071+3 1.220 .170+0 .131–1 .2442+3 0.753 –.886–2 –.469–2
500 .6176+2 1.329 –.149+0 .933–2 .1260+3 1.363 –.160+0 .122–1 .5730+2 1.985 .246+0 –.782–4 .9178+2 1.527 .285–1 .383–2 .1924+3 1.536 .172–1 .383–2 .3483+3 1.148 .620–1 .335–1 .5165+3 1.155 .668–1 .330–1 .3182+2 1.988 .195+0 –.394–4 .3594+2 1.617 .565–1 –.495–4 .7470+2 1.612 .451–1 .147–3 .6499+2 1.256 .259–1 .182–1
1000 .4241+2 1.407 .883–1 .227–1 .8483+2 1.453 .865–1 .254–1 .3077+2 1.987 .460–1 –.113–3 .4468+2 1.606 –.673–2 .190–2 .8992+2 1.632 –.860–2 .380–2 .8808+2 1.223 .277+0 .544–1 .1291+3 1.212 .282+0 .546–1 .1136+2 1.989 .454–1 –.780–4 .1276+2 1.678 –.183–1 –.203–3 .2532+2 1.695 –.200–1 .136–2 .1333+2 1.301 .223+0 .394–1
142
E (eV) 1500 .3036+2 1.421 .286+0 .314–1 .5974+2 1.474 .294+0 .332–1 .1909+2 1.990 –.495–1 –.129–3 .2507+2 1.599 .919–1 .463–2 .4923+2 1.634 .970–1 .699–2 .3255+2 1.182 .459+0 .723–1 .4734+2 1.163 .461+0 .736–1 .5851+1 1.991 –.429–1 –.994–4 .6182+1 1.653 .589–1 .158–2 .1197+2 1.683 .637–1 .377–2 .4455+1 1.235 .407+0 .575–1
2000 .2242+2 1.413 .454+0 .386–1 .4353+2 1.470 .469+0 .395–1 .1293+2 1.993 –.853–1 –.139–3 .1547+2 1.570 .220+0 .847–2 .2985+2 1.611 .231+0 .107–1 .1481+2 1.117 .605+0 .904–1 .2141+2 1.094 .604+0 .926–1 .3560+1 1.993 –.811–1 –.114–3 .3499+1 1.613 .178+0 .445–2 .6665+1 1.650 .189+0 .670–2 .1904+1 1.155 .561+0 .761–1
3000 .1315+2 1.374 .718+0 .513–1 .2498+2 1.435 .747+0 .503–1 .6983+1 1.995 –.587–1 –.151–3 .7075+1 1.496 .469+0 .180–1 .1333+2 1.545 .491+0 .192–1 .4391+1 0.987 .821+0 .127+0 .6298+1 0.965 .816+0 .131+0 .1700+1 1.995 –.621–1 –.132–3 .1447+1 1.526 .425+0 .129–1 .2695+1 1.572 .446+0 .143–1 .5237+0 1.008 .789+0 .114+0
4000 .8311+1 1.323 .925+0 .640–1 .1552+2 1.386 .964+0 .613–1 .4309+1 1.996 .329–1 –.158–3 .3791+1 1.422 .685+0 .293–1 .7020+1 1.474 .716+0 .292–1 .1728+1 0.874 .972+0 .164+0 .2463+1 0.856 .964+0 .169+0 .9786+0 1.996 .244–1 –.143–3 .7323+0 1.444 .644+0 .239–1 .1342+1 1.493 .674+0 .241–1 .1976+0 0.886 .944+0 .152+0
5000 .5552+1 1.269 .109+1 .771–1 .1022+2 1.333 .114+1 .728–1 .2891+1 1.994 .154+0 –.162–3 .2251+1 1.350 .869+0 .421–1 .4112+1 1.404 .908+0 .406–1 .8071+0 0.777 .108+1 .199+0 .1144+1 0.764 .107+1 .205+0 .6283+0 1.995 .141+0 –.149–3 .4194+0 1.367 .829+0 .365–1 .7588+0 1.419 .867+0 .354–1 .8990–1 0.785 .106+1 .189+0
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Tc, Z = 43 (continued) Shell 4d5/2 Eb = 8 eV 5s1/2 Eb = 7 eV
σ β γ δ σ β γ δ
100 .3507+3 −.235 .831–1 –.192–1 .3575+2 1.984 .184+0 .490–4
200 .3656+3 0.799 –.100–1 –.443–2 .1484+2 1.987 .241+0 .239–4
500 .9529+2 1.266 .297–1 .181–1 .3817+1 1.988 .196+0 –.289–4
1000 .1931+2 1.288 .228+0 .395–1 .1202+1 1.989 .492–1 –.729–4
E (eV) 1500 .6406+1 1.213 .410+0 .586–1 .5900+0 1.991 –.411–1 –.950–4
2000 .2724+1 1.130 .561+0 .782–1 .3503+0 1.993 –.809–1 –.110–3
3000 .7434+0 0.983 .784+0 .118+0 .1631+0 1.995 –.636–1 –.130–3
4000 .2787+0 0.866 .936+0 .157+0 .9271–1 1.996 .215–1 –.140–3
5000 .1262+0 0.770 .105+1 .195+0 .5904–1 1.995 .137+0 –.147–3
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .9378+1 1.969 –.988+0 –.517–3 .3858+2 1.972 .898+0 –.863–4 .8063+2 1.003 –.305+0 –.147–1 .1681+3 1.005 –.311+0 –.153–1 .1078+3 1.981 .581+0 .351–4 .1757+3 0.925 .223+0 .825–1 .3985+3 0.908 .204+0 .766–1 .1701+4 0.492 –.421–1 .188–2
200 .9295+1 1.968 –.808+0 –.545–3 .3682+2 1.974 .686+0 –.143–3 .7462+2 1.153 –.304+0 –.828–2 .1547+3 1.169 –.315+0 –.700–2 .9009+2 1.982 .480+0 –.164–4 .1485+3 1.234 .243+0 .364–1 .3286+3 1.225 .220+0 .329–1 .1102+4 0.790 –.468–1 .121–1
500 .8988+1 1.965 –.474+0 –.563–3 .3197+2 1.979 .328+0 –.213–3 .5912+2 1.321 –.168+0 .834–2 .1208+3 1.356 –.180+0 .114–1 .5657+2 1.983 .267+0 –.846–4 .9092+2 1.516 .405–1 .476–2 .1919+3 1.525 .273–1 .459–2 .3604+3 1.136 .496–1 .328–1
1000 .8485+1 1.960 –.137+0 –.556–3 .2564+2 1.985 .607–1 –.252–3 .4130+2 1.402 .691–1 .222–1 .8273+2 1.450 .662–1 .252–1 .3101+2 1.986 .607–1 –.126–3 .4546+2 1.604 –.121–1 .175–2 .9192+2 1.631 –.150–1 .370–2 .9480+2 1.225 .264+0 .537–1
E (eV) 1500 .8031+1 1.956 .985–1 –.547–3 .2097+2 1.990 –.447–1 –.266–3 .2997+2 1.419 .269+0 .310–1 .5906+2 1.474 .275+0 .332–1 .1947+2 1.989 –.420–1 –.145–3 .2595+2 1.601 .776–1 .415–2 .5113+2 1.638 .819–1 .669–2 .3582+2 1.190 .447+0 .711–1
2000 .7611+1 1.951 .286+0 –.537–3 .1743+2 1.993 –.753–1 –.272–3 .2240+2 1.414 .436+0 .382–1 .4353+2 1.473 .451+0 .394–1 .1330+2 1.992 –.842–1 –.156–3 .1621+2 1.575 .201+0 .773–2 .3136+2 1.618 .211+0 .102–1 .1654+2 1.130 .596+0 .887–1
3000 .6854+1 1.941 .581+0 –.521–3 .1250+2 1.995 –.309–1 –.274–3 .1338+2 1.378 .702+0 .507–1 .2543+2 1.441 .731+0 .499–1 .7258+1 1.995 –.692–1 –.169–3 .7539+1 1.506 .446+0 .167–1 .1422+2 1.556 .469+0 .182–1 .4996+1 1.005 .817+0 .124+0
4000 .6193+1 1.932 .817+0 –.507–3 .9320+1 1.995 .757–1 –.272–3 .8573+1 1.330 .912+0 .631–1 .1600+2 1.396 .952+0 .605–1 .4510+1 1.995 .132–1 –.177–3 .4086+1 1.434 .662+0 .276–1 .7568+1 1.489 .694+0 .277–1 .1991+1 0.894 .973+0 .160+0
5000 .5614+1 1.922 .102+1 –.493–3 .7165+1 1.993 .207+0 –.268–3 .5789+1 1.278 .108+1 .758–1 .1065+2 1.345 .113+1 .715–1 .3042+1 1.994 .127+0 –.183–3 .2447+1 1.365 .848+0 .398–1 .4468+1 1.421 .888+0 .386–1 .9385+0 0.797 .109+1 .195+0
Ru, Z = 44 Shell 1s1/2 Eb = 22123 eV 2s1/2 Eb = 3230 eV 2 p1/2 Eb = 2973 eV 2 p3/2 Eb = 2844 eV 3s1/2 Eb = 592 eV 3 p1/2 Eb = 488 eV 3 p3/2 Eb = 466 eV 3d3/2 Eb = 290 eV
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TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Ru, Z = 44 (continued) Shell 3d5/2 Eb = 286 eV 4s1/2 Eb = 81 eV 4 p1/2 Eb = 53 eV 4 p3/2 Eb = 49 eV 4d3/2 Eb = 8 eV 4d5/2 Eb = 8 eV 5s1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2578+4 0.518 –.423–1 .101–2 .1655+3 1.984 .250+0 .599–4 .1330+3 0.544 .305–2 .313–1 .3203+3 0.566 .877–2 .294–1 .1804+3 −.513 .109+0 –.176–1 .2788+3 −.432 .112+0 –.199–1 .2956+2 1.982 .179+0 .611–4
200 .1657+4 0.816 –.456–1 .114–1 .9655+2 1.986 .282+0 .148–4 .9391+2 1.204 .186+0 .160–1 .2119+3 1.189 .171+0 .153–1 .2395+3 0.695 –.620–3 –.669–2 .3578+3 0.746 –.233–2 –.642–2 .1219+2 1.986 .245+0 .271–4
500 .5345+3 1.144 .548–1 .323–1 .3348+2 1.987 .210+0 –.416–4 .3793+2 1.608 .715–1 .291–3 .7910+2 1.602 .584–1 .421–3 .6951+2 1.246 .140–1 .165–1 .1016+3 1.260 .176–1 .164–1 .3223+1 1.987 .207+0 –.322–4
1000 .1389+3 1.214 .269+0 .538–1 .1208+2 1.988 .581–1 –.860–4 .1368+2 1.680 –.210–1 –.390–3 .2718+2 1.696 –.237–1 .119–2 .1466+2 1.308 .206+0 .377–1 .2114+2 1.297 .212+0 .378–1 .1022+1 1.988 .614–1 –.778–4
E (eV) 1500 .5207+2 1.171 .450+0 .723–1 .6247+1 1.990 –.353–1 –.111–3 .6692+1 1.659 .452–1 .113–2 .1296+2 1.689 .494–1 .346–2 .4970+1 1.248 .390+0 .553–1 .7114+1 1.226 .394+0 .564–1 .5028+0 1.990 –.326–1 –.105–3
2000 .2390+2 1.107 .596+0 .909–1 .3813+1 1.992 –.792–1 –.127–3 .3816+1 1.622 .158+0 .371–2 .7262+1 1.659 .168+0 .616–2 .2148+1 1.171 .546+0 .733–1 .3058+1 1.145 .547+0 .753–1 .2991+0 1.992 –.783–1 –.123–3
3000 .7160+1 0.981 .811+0 .128+0 .1829+1 1.995 –.720–1 –.147–3 .1597+1 1.538 .401+0 .115–1 .2967+1 1.585 .422+0 .132–1 .5991+0 1.028 .781+0 .110+0 .8459+0 1.002 .776+0 .114+0 .1397+0 1.994 –.730–1 –.144–3
4000 .2835+1 0.873 .964+0 .165+0 .1057+1 1.995 .523–2 –.160–3 .8144+0 1.458 .619+0 .219–1 .1488+1 1.510 .650+0 .224–1 .2280+0 0.908 .942+0 .148+0 .3199+0 0.885 .934+0 .153+0 .7959–1 1.995 .273–2 –.157–3
5000 .1329+1 0.782 .108+1 .201+0 .6800+0 1.995 .115+0 –.167–3 .4691+0 1.383 .806+0 .339–1 .8459+0 1.438 .845+0 .332–1 .1044+0 0.806 .106+1 .183+0 .1458+0 0.789 .105+1 .189+0 .5079–1 1.995 .111+0 –.164–3
σ β γ δ σ β γ δ σ β γ δ
100 .8889+1 1.967 –.102+1 –.576–3 .3644+2 1.970 .924+0 –.933–4 .7573+2 0.996 –.317+0 –.165–1
200 .8819+1 1.966 –.840+0 –.608–3 .3488+2 1.972 .712+0 –.157–3 .7039+2 1.145 –.318+0 –.980–2
500 .8545+1 1.963 –.503+0 –.628–3 .3051+2 1.977 .351+0 –.235–3 .5648+2 1.314 –.185+0 .739–2
1000 .8089+1 1.958 –.163+0 –.621–3 .2472+2 1.984 .764–1 –.279–3 .4011+2 1.398 .510–1 .216–1
E (eV) 1500 .7673+1 1.954 .735–1 –.611–3 .2038+2 1.988 –.369–1 –.297–3 .2950+2 1.417 .250+0 .306–1
2000 .7289+1 1.949 .262+0 –.601–3 .1706+2 1.992 –.748–1 –.304–3 .2230+2 1.414 .418+0 .378–1
3000 .6594+1 1.939 .559+0 –.582–3 .1238+2 1.995 –.422–1 –.307–3 .1356+2 1.382 .686+0 .501–1
4000 .5984+1 1.930 .795+0 –.566–3 .9315+1 1.995 .557–1 –.305–3 .8807+1 1.337 .898+0 .623–1
5000 .5447+1 1.921 .999+0 –.552–3 .7215+1 1.993 .180+0 –.302–3 .6010+1 1.287 .107+1 .746–1
Rh, Z = 45 Shell 1s1/2 Eb = 23225 eV 2s1/2 Eb = 3418 eV 2 p1/2 Eb = 3152 eV
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M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Rh, Z = 45 (continued) Shell 2 p3/2 Eb = 3010 eV 3s1/2 Eb = 634 eV 3 p1/2 Eb = 526 eV 3 p3/2 Eb = 501 eV 3d3/2 Eb = 318 eV 3d5/2 Eb = 313 eV 4s1/2 Eb = 87 eV 4 p1/2 Eb = 58 eV 4 p3/2 Eb = 53 eV 4d3/2 Eb = 9 eV 4d5/2 Eb = 9 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1581+3 0.997 –.324+0 –.172–1 .1029+3 1.980 .605+0 .419–4 .1682+3 0.912 .224+0 .882–1 .3840+3 0.894 .204+0 .818–1 .1632+4 0.479 –.436–1 .838–3 .2479+4 0.506 –.439–1 –.382–4 .1655+3 1.982 .254+0 .714–4 .1333+3 0.513 –.933–2 .322–1 .3265+3 0.538 –.238–2 .301–1 .1708+3 −.629 .119+0 –.124–1 .2647+3 −.546 .125+0 –.159–1
200 .1462+3 1.161 –.331+0 –.843–2 .8684+2 1.980 .501+0 –.147–4 .1433+3 1.220 .254+0 .402–1 .3192+3 1.210 .230+0 .364–1 .1073+4 0.770 –.528–1 .107–1 .1617+4 0.799 –.516–1 .995–2 .9891+2 1.985 .288+0 .199–4 .9635+2 1.182 .186+0 .178–1 .2202+3 1.167 .170+0 .170–1 .2541+3 0.650 .880–2 –.779–2 .3802+3 0.707 .670–2 –.758–2
500 .1156+3 1.350 –.198+0 .107–1 .5569+2 1.982 .286+0 –.912–4 .8975+2 1.507 .518–1 .572–2 .1905+3 1.516 .368–1 .539–2 .3685+3 1.124 .379–1 .320–1 .5472+3 1.134 .433–1 .314–1 .3528+2 1.986 .222+0 –.438–4 .4017+2 1.601 .851–1 .670–3 .8433+2 1.593 .703–1 .735–3 .7906+2 1.237 .427–2 .148–1 .1155+3 1.253 .770–2 .147–1
1000 .8048+2 1.447 .469–1 .250–1 .3116+2 1.985 .748–1 –.139–3 .4605+2 1.601 –.158–1 .165–2 .9352+2 1.629 –.199–1 .365–2 .1009+3 1.225 .250+0 .530–1 .1479+3 1.216 .256+0 .531–1 .1289+2 1.987 .700–1 –.940–4 .1475+2 1.681 –.219–1 –.529–3 .2940+2 1.697 –.257–1 .105–2 .1719+2 1.315 .190+0 .361–1 .2477+2 1.304 .196+0 .361–1
145
E (eV) 1500 .5821+2 1.474 .256+0 .331–1 .1980+2 1.988 –.335–1 –.161–3 .2673+2 1.603 .643–1 .373–2 .5283+2 1.640 .679–1 .643–2 .3901+2 1.198 .435+0 .702–1 .5672+2 1.179 .439+0 .713–1 .6690+1 1.989 –.271–1 –.122–3 .7280+1 1.664 .330–1 .751–3 .1413+2 1.694 .365–1 .318–2 .5920+1 1.260 .374+0 .534–1 .8467+1 1.238 .378+0 .544–1
2000 .4338+2 1.475 .433+0 .392–1 .1363+2 1.990 –.819–1 –.174–3 .1690+2 1.580 .182+0 .706–2 .3277+2 1.624 .193+0 .974–2 .1828+2 1.142 .586+0 .872–1 .2642+2 1.118 .586+0 .894–1 .4095+1 1.991 –.761–1 –.140–3 .4183+1 1.629 .139+0 .305–2 .7969+1 1.667 .149+0 .570–2 .2588+1 1.187 .531+0 .707–1 .3681+1 1.160 .532+0 .727–1
3000 .2578+2 1.447 .716+0 .495–1 .7520+1 1.994 –.780–1 –.190–3 .7992+1 1.515 .424+0 .156–1 .1509+2 1.567 .446+0 .173–1 .5632+1 1.021 .812+0 .122+0 .8067+1 0.996 .807+0 .126+0 .1975+1 1.994 –.799–1 –.164–3 .1771+1 1.550 .376+0 .102–1 .3290+1 1.598 .397+0 .122–1 .7330+0 1.047 .772+0 .106+0 .1034+1 1.019 .767+0 .110+0
4000 .1644+2 1.405 .939+0 .598–1 .4706+1 1.995 –.458–2 –.199–3 .4382+1 1.446 .640+0 .260–1 .8117+1 1.502 .673+0 .264–1 .2273+1 0.912 .972+0 .157+0 .3234+1 0.890 .963+0 .162+0 .1144+1 1.995 –.122–1 –.178–3 .9106+0 1.472 .594+0 .200–1 .1662+1 1.525 .625+0 .209–1 .2816+0 0.929 .939+0 .143+0 .3944+0 0.904 .931+0 .148+0
5000 .1105+2 1.356 .112+1 .703–1 .3190+1 1.994 .102+0 –.205–3 .2646+1 1.379 .827+0 .376–1 .4831+1 1.437 .868+0 .366–1 .1082+1 0.817 .109+1 .190+0 .1530+1 0.799 .108+1 .197+0 .7383+0 1.995 .901–1 –.187–3 .5277+0 1.399 .783+0 .315–1 .9500+0 1.455 .823+0 .310–1 .1299+0 0.827 .106+1 .178+0 .1810+0 0.808 .105+1 .184+0
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Rh, Z = 45 (continued) Shell 5s1/2 Eb = 7 eV
σ β γ δ
100 .2990+2 1.980 .176+0 .707–4
200 .1249+2 1.984 .248+0 .317–4
500 .3355+1 1.986 .218+0 –.340–4
1000 .1069+1 1.987 .732–1 –.865–4
E (eV) 1500 .5263+0 1.989 –.242–1 –.116–3
2000 .3133+0 1.991 –.751–1 –.135–3
3000 .1467+0 1.994 –.809–1 –.161–3
4000 .8380–1 1.995 –.146–1 –.175–3
5000 .5356–1 1.995 .866–1 –.183–3
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .8433+1 1.965 –.106+1 –.638–3 .3449+2 1.968 .960+0 –.978–4 .7132+2 0.982 –.328+0 –.185–1 .1492+3 0.982 –.335+0 –.194–1 .9844+2 1.978 .635+0 .527–4 .1611+3 0.886 .221+0 .969–1 .3703+3 0.866 .200+0 .899–1 .1587+4 0.460 –.435–1 .550–4 .2410+4 0.487 –.439–1 –.842–3
200 .8376+1 1.964 –.881+0 –.679–3 .3311+2 1.970 .749+0 –.169–3 .6661+2 1.132 –.334+0 –.116–1 .1386+3 1.147 –.347+0 –.102–1 .8388+2 1.979 .530+0 –.996–5 .1384+3 1.195 .268+0 .458–1 .3105+3 1.184 .241+0 .413–1 .1054+4 0.742 –.586–1 .896–2 .1588+4 0.772 –.577–1 .821–2
500 .8133+1 1.961 –.535+0 –.699–3 .2916+2 1.975 .378+0 –.258–3 .5408+2 1.307 –.204+0 .622–2 .1109+3 1.343 –.218+0 .984–2 .5486+2 1.980 .308+0 –.977–4 .8865+2 1.496 .659–1 .695–2 .1894+3 1.505 .490–1 .640–2 .3783+3 1.110 .251–1 .311–1 .5617+3 1.122 .307–1 .304–1
1000 .7719+1 1.956 –.192+0 –.693–3 .2385+2 1.982 .944–1 –.309–3 .3901+2 1.393 .313–1 .210–1 .7842+2 1.444 .258–1 .247–1 .3130+2 1.983 .909–1 –.153–3 .4664+2 1.598 –.187–1 .160–2 .9517+2 1.626 –.241–1 .362–2 .1075+3 1.225 .237+0 .526–1 .1575+3 1.216 .243+0 .525–1
E (eV) 1500 .7338+1 1.952 .465–1 –.682–3 .1982+2 1.987 –.275–1 –.329–3 .2905+2 1.415 .230+0 .301–1 .5741+2 1.473 .235+0 .329–1 .2012+2 1.987 –.236–1 –.178–3 .2750+2 1.604 .512–1 .332–2 .5456+2 1.642 .539–1 .618–2 .4244+2 1.205 .422+0 .694–1 .6168+2 1.186 .427+0 .703–1
2000 .6986+1 1.947 .236+0 –.670–3 .1670+2 1.990 –.730–1 –.338–3 .2219+2 1.413 .399+0 .373–1 .4323+2 1.477 .413+0 .391–1 .1396+2 1.989 –.783–1 –.194–3 .1759+2 1.585 .164+0 .640–2 .3420+2 1.630 .173+0 .933–2 .2018+2 1.154 .576+0 .859–1 .2914+2 1.129 .577+0 .880–1
3000 .6347+1 1.938 .536+0 –.651–3 .1225+2 1.994 –.527–1 –.344–3 .1373+2 1.385 .670+0 .496–1 .2612+2 1.453 .700+0 .492–1 .7781+1 1.993 –.858–1 –.212–3 .8456+1 1.524 .402+0 .145–1 .1599+2 1.577 .424+0 .165–1 .6329+1 1.037 .806+0 .119+0 .9057+1 1.011 .801+0 .123+0
4000 .5783+1 1.928 .775+0 –.633–3 .9302+1 1.994 .366–1 –.343–3 .9032+1 1.342 .884+0 .615–1 .1686+2 1.413 .927+0 .591–1 .4902+1 1.994 –.215–1 –.223–3 .4687+1 1.457 .618+0 .244–1 .8687+1 1.515 .651+0 .251–1 .2586+1 0.930 .970+0 .153+0 .3674+1 0.905 .962+0 .159+0
5000 .5283+1 1.919 .974+0 –.616–3 .7256+1 1.993 .154+0 –.338–3 .6227+1 1.296 .106+1 .735–1 .1145+2 1.368 .111+1 .693–1 .3340+1 1.994 .772–1 –.230–3 .2854+1 1.393 .804+0 .356–1 .5209+1 1.454 .847+0 .349–1 .1241+1 0.837 .109+1 .187+0 .1753+1 0.817 .108+1 .193+0
Pd, Z = 46 Shell 1s1/2 Eb = 24357 eV 2s1/2 Eb = 3611 eV 2 p1/2 Eb = 3337 eV 2 p3/2 Eb = 3180 eV 3s1/2 Eb = 677 eV 3 p1/2 Eb = 565 eV 3 p3/2 Eb = 537 eV 3d3/2 Eb = 347 eV 3d5/2 Eb = 342 eV
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Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Pd, Z = 46 (continued) Shell 4s1/2 Eb = 93 eV 4 p1/2 Eb = 63 eV 4 p3/2 Eb = 57 eV 4d3/2 Eb = 9 eV 4d5/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1631+3 1.979 .258+0 .901–4 .1286+3 0.443 –.325–1 .327–1 .3206+3 0.473 –.235–1 .305–1 .1252+3 −.811 .134+0 –.800–2 .1946+3 −.749 .149+0 –.137–1
200 .1003+3 1.983 .298+0 .290–4 .9658+2 1.139 .183+0 .205–1 .2236+3 1.125 .167+0 .195–1 .2423+3 0.579 .230–1 –.906–2 .3630+3 0.642 .205–1 –.892–2
500 .3693+2 1.984 .236+0 –.454–4 .4200+2 1.591 .102+0 .117–2 .8872+2 1.581 .851–1 .115–2 .8314+2 1.223 –.513–2 .130–1 .1211+3 1.242 –.202–2 .129–1
1000 .1365+2 1.986 .834–1 –.102–3 .1571+2 1.681 –.215–1 –.654–3 .3141+2 1.696 –.266–1 .907–3 .1860+2 1.320 .173+0 .346–1 .2667+2 1.310 .180+0 .346–1
E (eV) 1500 .7113+1 1.988 –.177–1 –.134–3 .7825+1 1.669 .214–1 .391–3 .1519+2 1.698 .240–1 .292–2 .6496+1 1.273 .357+0 .516–1 .9234+1 1.250 .362+0 .524–1
2000 .4365+1 1.990 –.719–1 –.155–3 .4527+1 1.637 .120+0 .243–2 .8623+1 1.675 .130+0 .527–2 .2869+1 1.203 .515+0 .682–1 .4054+1 1.176 .517+0 .701–1
3000 .2113+1 1.993 –.868–1 –.182–3 .1938+1 1.560 .352+0 .899–2 .3595+1 1.610 .373+0 .113–1 .8236+0 1.067 .761+0 .103+0 .1153+1 1.037 .757+0 .107+0
4000 .1229+1 1.994 –.286–1 –.199–3 .1004+1 1.485 .570+0 .182–1 .1829+1 1.540 .601+0 .194–1 .3191+0 0.948 .935+0 .138+0 .4438+0 0.921 .926+0 .144+0
5000 .7946+0 1.994 .661–1 –.209–3 .5852+0 1.415 .759+0 .292–1 .1050+1 1.473 .799+0 .290–1 .1481+0 0.850 .106+1 .173+0 .2049+0 0.828 .105+1 .180+0
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .8009+1 1.963 –.109+1 –.709–3 .3263+2 1.967 .979+0 –.108–3 .6703+2 0.979 –.342+0 –.204–1 .1405+3 0.979 –.349+0 –.213–1 .9365+2 1.976 .655+0 .590–4
200 .7959+1 1.962 –.907+0 –.751–3 .3139+2 1.969 .768+0 –.186–3 .6284+2 1.129 –.348+0 –.131–1 .1310+3 1.144 –.362+0 –.116–1 .8047+2 1.977 .547+0 –.917–5
500 .7743+1 1.959 –.563+0 –.778–3 .2783+2 1.974 .400+0 –.284–3 .5158+2 1.301 –.219+0 .533–2 .1060+3 1.338 –.235+0 .924–2 .5366+2 1.979 .325+0 –.105–3
1000 .7367+1 1.954 –.217+0 –.770–3 .2297+2 1.981 .110+0 –.342–3 .3778+2 1.389 .143–1 .204–1 .7606+2 1.441 .754–2 .245–1 .3123+2 1.982 .105+0 –.168–3
E (eV) 1500 .7017+1 1.950 .223–1 –.759–3 .1923+2 1.986 –.182–1 –.365–3 .2848+2 1.412 .213+0 .297–1 .5635+2 1.473 .217+0 .328–1 .2032+2 1.985 –.141–1 –.197–3
2000 .6694+1 1.945 .213+0 –.747–3 .1631+2 1.989 –.703–1 –.376–3 .2198+2 1.413 .382+0 .369–1 .4286+2 1.478 .395+0 .390–1 .1422+2 1.988 –.741–1 –.215–3
3000 .6107+1 1.935 .513+0 –.724–3 .1209+2 1.993 –.612–1 –.383–3 .1383+2 1.387 .654+0 .491–1 .2632+2 1.458 .684+0 .490–1 .8013+1 1.992 –.918–1 –.236–3
4000 .5585+1 1.926 .751+0 –.704–3 .9261+1 1.994 .194–1 –.382–3 .9214+1 1.347 .869+0 .608–1 .1720+2 1.421 .912+0 .585–1 .5084+1 1.994 –.362–1 –.248–3
5000 .5121+1 1.917 .956+0 –.688–3 .7276+1 1.993 .131+0 –.380–3 .6419+1 1.302 .105+1 .724–1 .1179+2 1.378 .110+1 .683–1 .3482+1 1.994 .555–1 –.257–3
Ag, Z = 47 Shell 1s1/2 Eb = 25520 eV 2s1/2 Eb = 3812 eV 2 p1/2 Eb = 3530 eV 2 p3/2 Eb = 3357 eV 3s1/2 Eb = 724 eV
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Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Ag, Z = 47 (continued) Shell 3 p1/2 Eb = 608 eV 3 p3/2 Eb = 577 eV 3d3/2 Eb = 379 eV 3d5/2 Eb = 373 eV 4s1/2 Eb = 101 eV 4 p1/2 Eb = 69 eV 4 p3/2 Eb = 63 eV 4d3/2 Eb = 11 eV 4d5/2 Eb = 10 eV 5s1/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1537+3 0.884 .225+0 .101+0 .3552+3 0.863 .202+0 .933–1 .1505+4 0.459 –.455–1 –.755–3 .2289+4 0.487 –.459–1 –.164–2 .1621+3 1.977 .264+0 .101–3 .1311+3 0.447 –.341–1 .335–1 .3297+3 0.476 –.248–1 .314–1 .1455+3 −.816 .109+0 .394–2 .2278+3 −.750 .128+0 –.270–2 .2965+2 1.974 .169+0 .947–4
200 .1329+3 1.190 .277+0 .489–1 .2998+3 1.178 .248+0 .441–1 .1013+4 0.730 –.636–1 .763–2 .1528+4 0.762 –.628–1 .688–2 .1016+3 1.981 .303+0 .342–4 .9917+2 1.131 .182+0 .218–1 .2316+3 1.117 .166+0 .207–1 .2738+3 0.550 .323–1 –.851–2 .4130+3 0.618 .296–1 –.851–2 .1284+2 1.981 .255+0 .447–4
500 .8686+2 1.487 .768–1 .803–2 .1866+3 1.496 .580–1 .731–2 .3802+3 1.100 .145–1 .303–1 .5652+3 1.113 .203–1 .295–1 .3849+2 1.983 .246+0 –.476–4 .4417+2 1.583 .114+0 .162–2 .9390+2 1.573 .956–1 .155–2 .9830+2 1.215 –.120–1 .115–1 .1440+3 1.236 –.917–2 .115–1 .3560+1 1.984 .239+0 –.352–4
1000 .4684+2 1.595 –.201–1 .162–2 .9599+2 1.623 –.267–1 .366–2 .1125+3 1.224 .223+0 .517–1 .1650+3 1.216 .230+0 .516–1 .1446+2 1.985 .949–1 –.111–3 .1685+2 1.682 –.199–1 –.727–3 .3381+2 1.695 –.262–1 .820–3 .2274+2 1.325 .157+0 .329–1 .3277+2 1.316 .164+0 .328–1 .1151+1 1.985 .981–1 –.103–3
148
E (eV) 1500 .2808+2 1.605 .405–1 .299–2 .5588+2 1.644 .423–1 .600–2 .4547+2 1.211 .410+0 .685–1 .6608+2 1.192 .415+0 .694–1 .7575+1 1.986 –.872–2 –.148–3 .8472+1 1.673 .122–1 .979–4 .1650+2 1.702 .140–1 .272–2 .8066+1 1.283 .341+0 .498–1 .1152+2 1.261 .346+0 .505–1 .5679+0 1.986 –.558–2 –.140–3
2000 .1817+2 1.588 .147+0 .582–2 .3542+2 1.635 .157+0 .898–2 .2196+2 1.164 .565+0 .845–1 .3171+2 1.139 .567+0 .865–1 .4664+1 1.989 –.671–1 –.172–3 .4937+1 1.643 .104+0 .189–2 .9423+1 1.682 .113+0 .491–2 .3604+1 1.217 .500+0 .660–1 .5116+1 1.189 .503+0 .678–1 .3382+0 1.988 –.652–1 –.163–3
3000 .8883+1 1.531 .381+0 .135–1 .1682+2 1.587 .403+0 .158–1 .7027+1 1.053 .800+0 .117+0 .1005+2 1.025 .796+0 .121+0 .2270+1 1.992 –.918–1 –.202–3 .2138+1 1.570 .328+0 .791–2 .3969+1 1.621 .349+0 .105–1 .1051+1 1.085 .750+0 .995–1 .1479+1 1.054 .747+0 .103+0 .1593+0 1.992 –.929–1 –.196–3
4000 .4980+1 1.468 .595+0 .230–1 .9233+1 1.528 .629+0 .240–1 .2908+1 0.948 .969+0 .150+0 .4128+1 0.922 .960+0 .156+0 .1325+1 1.994 –.428–1 –.220–3 .1117+1 1.498 .544+0 .166–1 .2034+1 1.554 .576+0 .181–1 .4115+0 0.969 .930+0 .134+0 .5747+0 0.940 .922+0 .140+0 .9140–1 1.994 –.456–1 –.217–3
5000 .3058+1 1.405 .783+0 .336–1 .5580+1 1.468 .826+0 .332–1 .1409+1 0.854 .109+1 .182+0 .1989+1 0.833 .108+1 .189+0 .8589+0 1.994 .447–1 –.233–3 .6549+0 1.428 .735+0 .270–1 .1175+1 1.489 .776+0 .271–1 .1924+0 0.870 .106+1 .168+0 .2671+0 0.845 .105+1 .175+0 .5864–1 1.994 .411–1 –.229–3
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Cd, Z = 48 Shell 1s1/2 Eb = 26715 eV 2s1/2 Eb = 4022 eV 2 p1/2 Eb = 3732 eV 2 p3/2 Eb = 3542 eV 3s1/2 Eb = 775 eV 3 p1/2 Eb = 655 eV 3 p3/2 Eb = 621 eV 3d3/2 Eb = 415 eV 3d5/2 Eb = 408 eV 4s1/2 Eb = 112 eV 4 p1/2 Eb = 78 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .7615+1 1.961 –.112+1 –.787–3 .3089+2 1.965 .999+0 –.119–3 .6304+2 0.977 –.356+0 –.223–1 .1323+3 0.976 –.363+0 –.233–1 .8890+2 1.975 .676+0 .661–4 .1462+3 0.882 .228+0 .104+0 .3394+3 0.860 .205+0 .965–1 .1415+4 0.457 –.479–1 –.162–2 .2154+4 0.487 –.484–1 –.251–2 .1594+3 1.975 .274+0 .114–3 .1321+3 0.453 –.345–1 .351–1
200 .7569+1 1.960 –.935+0 –.833–3 .2977+2 1.967 .789+0 –.204–3 .5929+2 1.124 –.362+0 –.146–1 .1237+3 1.140 –.377+0 –.129–1 .7699+2 1.975 .567+0 –.782–5 .1272+3 1.182 .285+0 .520–1 .2885+3 1.170 .254+0 .469–1 .9667+3 0.719 –.688–1 .630–2 .1460+4 0.753 –.681–1 .555–2 .1020+3 1.979 .311+0 .406–4 .1009+3 1.121 .183+0 .233–1
500 .7375+1 1.957 –.590+0 –.864–3 .2655+2 1.972 .421+0 –.312–3 .4917+2 1.295 –.235+0 .439–2 .1012+3 1.333 –.253+0 .860–2 .5231+2 1.977 .343+0 –.113–3 .8479+2 1.479 .879–1 .919–2 .1831+3 1.488 .670–1 .828–2 .3793+3 1.089 .411–2 .295–1 .5642+3 1.104 .102–1 .287–1 .3983+2 1.982 .256+0 –.501–4 .4613+2 1.576 .126+0 .212–2
1000 .7035+1 1.952 –.242+0 –.852–3 .2211+2 1.979 .126+0 –.376–3 .3654+2 1.384 –.237–2 .198–1 .7368+2 1.439 –.106–1 .242–1 .3106+2 1.981 .119+0 –.183–3 .4685+2 1.592 –.204–1 .168–2 .9642+2 1.620 –.285–1 .373–2 .1169+3 1.222 .210+0 .512–1 .1715+3 1.215 .218+0 .509–1 .1524+2 1.983 .106+0 –.121–3 .1798+2 1.681 –.171–1 –.768–3
149
E (eV) 1500 .6714+1 1.948 –.192–2 –.840–3 .1864+2 1.984 –.810–2 –.403–3 .2786+2 1.410 .195+0 .292–1 .5521+2 1.472 .198+0 .327–1 .2046+2 1.984 –.388–2 –.217–3 .2854+2 1.605 .308–1 .271–2 .5700+2 1.645 .316–1 .586–2 .4836+2 1.216 .399+0 .680–1 .7029+2 1.197 .405+0 .688–1 .8040+1 1.985 .625–3 –.161–3 .9135+1 1.676 .417–2 –.158–3
2000 .6417+1 1.943 .189+0 –.830–3 .1591+2 1.988 –.665–1 –.417–3 .2172+2 1.412 .365+0 .366–1 .4240+2 1.480 .378+0 .390–1 .1444+2 1.987 –.690–1 –.238–3 .1869+2 1.591 .132+0 .531–2 .3653+2 1.639 .141+0 .871–2 .2373+2 1.173 .555+0 .835–1 .3425+2 1.148 .558+0 .854–1 .4969+1 1.987 –.617–1 –.189–3 .5364+1 1.649 .891–1 .142–2
3000 .5876+1 1.933 .491+0 –.805–3 .1192+2 1.992 –.683–1 –.426–3 .1389+2 1.389 .638+0 .487–1 .2646+2 1.463 .668+0 .488–1 .8227+1 1.991 –.967–1 –.262–3 .9292+1 1.538 .360+0 .125–1 .1761+2 1.595 .382+0 .152–1 .7749+1 1.067 .794+0 .115+0 .1108+2 1.038 .791+0 .119+0 .2431+1 1.991 –.956–1 –.223–3 .2349+1 1.580 .306+0 .693–2
4000 .5394+1 1.924 .729+0 –.784–3 .9204+1 1.993 .363–2 –.426–3 .9372+1 1.352 .855+0 .601–1 .1750+2 1.429 .899+0 .580–1 .5258+1 1.993 –.496–1 –.276–3 .5269+1 1.478 .573+0 .216–1 .9774+1 1.540 .607+0 .229–1 .3249+1 0.965 .967+0 .147+0 .4608+1 0.937 .959+0 .153+0 .1425+1 1.993 –.556–1 –.244–3 .1238+1 1.510 .520+0 .150–1
5000 .4963+1 1.915 .935+0 –.766–3 .7280+1 1.993 .109+0 –.424–3 .6594+1 1.309 .103+1 .714–1 .1211+2 1.387 .109+1 .674–1 .3620+1 1.993 .349–1 –.287–3 .3263+1 1.416 .762+0 .318–1 .5953+1 1.482 .806+0 .317–1 .1590+1 0.872 .110+1 .179+0 .2241+1 0.848 .108+1 .186+0 .9264+0 1.993 .244–1 –.259–3 .7302+0 1.442 .711+0 .249–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Cd, Z = 48 (continued) Shell 4 p3/2 Eb = 71 eV 4d3/2 Eb = 14 eV 4d5/2 Eb = 13 eV 5s1/2 Eb = 9 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3372+3 0.481 –.249–1 .328–1 .1687+3 −.814 .818–1 .167–1 .2650+3 −.743 .104+0 .919–2 .3802+2 1.972 .175+0 .104–3
200 .2386+3 1.106 .166+0 .221–1 .3026+3 0.524 .417–1 –.744–2 .4585+3 0.596 .390–1 –.765–2 .1639+2 1.979 .252+0 .536–4
500 .9889+2 1.564 .106+0 .198–2 .1131+3 1.205 –.175–1 .101–1 .1662+3 1.229 –.151–1 .101–1 .4595+1 1.982 .245+0 –.343–4
1000 .3627+2 1.695 –.248–1 .756–3 .2704+2 1.329 .142+0 .314–1 .3908+2 1.321 .149+0 .312–1 .1499+1 1.984 .109+0 –.109–3
E (eV) 1500 .1786+2 1.705 .500–2 .254–2 .9749+1 1.294 .325+0 .482–1 .1396+2 1.271 .332+0 .488–1 .7418+0 1.985 .380–2 –.152–3
2000 .1027+2 1.688 .971–1 .462–2 .4405+1 1.231 .484+0 .640–1 .6268+1 1.202 .488+0 .657–1 .4428+0 1.987 –.597–1 –.181–3
3000 .4369+1 1.631 .327+0 .985–2 .1306+1 1.103 .738+0 .963–1 .1840+1 1.070 .735+0 .100+0 .2089+0 1.991 –.956–1 –.216–3
4000 .2256+1 1.568 .551+0 .169–1 .5164+0 0.989 .924+0 .130+0 .7224+0 0.957 .916+0 .136+0 .1202+0 1.993 –.577–1 –.239–3
5000 .1310+1 1.504 .753+0 .254–1 .2432+0 0.889 .106+1 .163+0 .3381+0 0.862 .105+1 .170+0 .7724–1 1.993 .212–1 –.254–3
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .7247+1 1.959 –.115+1 –.874–3 .2924+2 1.964 .102+1 –.132–3 .5930+2 0.976 –.371+0 –.241–1 .1246+3 0.975 –.379+0 –.251–1 .8421+2 1.973 .696+0 .726–4 .1385+3 0.884 .235+0 .107+0
200 .7203+1 1.957 –.963+0 –.928–3 .2822+2 1.965 .808+0 –.225–3 .5593+2 1.119 –.376+0 –.157–1 .1169+3 1.135 –.392+0 –.139–1 .7345+2 1.973 .585+0 –.638–5 .1213+3 1.173 .291+0 .544–1
500 .7029+1 1.955 –.615+0 –.958–3 .2532+2 1.970 .441+0 –.344–3 .4683+2 1.290 –.250+0 .353–2 .9649+2 1.329 –.269+0 .807–2 .5083+2 1.975 .359+0 –.122–3 .8238+2 1.472 .980–1 .103–1
1000 .6720+1 1.950 –.266+0 –.947–3 .2125+2 1.977 .142+0 –.416–3 .3528+2 1.380 –.182–1 .194–1 .7124+2 1.436 –.279–1 .241–1 .3078+2 1.979 .134+0 –.201–3 .4662+2 1.588 –.200–1 .179–2
E (eV) 1500 .6426+1 1.945 –.253–1 –.933–3 .1805+2 1.983 .224–2 –.446–3 .2721+2 1.407 .179+0 .289–1 .5398+2 1.471 .180+0 .327–1 .2052+2 1.982 .641–2 –.239–3 .2887+2 1.605 .224–1 .247–2
2000 .6153+1 1.941 .166+0 –.921–3 .1549+2 1.987 –.619–1 –.462–3 .2141+2 1.411 .348+0 .363–1 .4184+2 1.481 .360+0 .390–1 .1461+2 1.985 –.632–1 –.263–3 .1914+2 1.594 .118+0 .485–2
3000 .5654+1 1.931 .468+0 –.893–3 .1172+2 1.991 –.742–1 –.473–3 .1391+2 1.391 .622+0 .483–1 .2651+2 1.467 .652+0 .487–1 .8420+1 1.990 –.100+0 –.290–3 .9674+1 1.545 .340+0 .117–1
4000 .5208+1 1.922 .708+0 –.870–3 .9128+1 1.993 –.108–1 –.474–3 .9501+1 1.356 .840+0 .596–1 .1774+2 1.436 .885+0 .577–1 .5422+1 1.992 –.617–1 –.307–3 .5549+1 1.487 .552+0 .203–1
5000 .4807+1 1.912 .914+0 –.852–3 .7269+1 1.992 .875–1 –.474–3 .6752+1 1.315 .102+1 .706–1 .1240+2 1.396 .108+1 .666–1 .3752+1 1.993 .158–1 –.319–3 .3466+1 1.428 .741+0 .301–1
In, Z = 49 Shell 1s1/2 Eb = 27944 eV 2s1/2 Eb = 4242 eV 2 p1/2 Eb = 3943 eV 2 p3/2 Eb = 3735 eV 3s1/2 Eb = 830 eV 3 p1/2 Eb = 707 eV
150
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables In, Z = 49 (continued) Shell 3 p3/2 Eb = 669 eV 3d3/2 Eb = 455 eV 3d5/2 Eb = 447 eV 4s1/2 Eb = 126 eV 4 p1/2 Eb = 90 eV 4 p3/2 Eb = 82 eV 4d3/2 Eb = 21 eV 4d5/2 Eb = 20 eV 5s1/2 Eb = 10 eV 5 p1/2 Eb = 5 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3232+3 0.861 .209+0 .987–1 .1316+4 0.459 –.511–1 –.256–2 .2005+4 0.490 –.517–1 –.344–2 .1550+3 1.973 .288+0 .127–3 .1322+3 0.474 –.300–1 .374–1 .3414+3 0.499 –.203–1 .349–1 .1995+3 −.779 .610–1 .285–1 .3143+3 −.695 .852–1 .206–1 .4922+2 1.969 .177+0 .112–3 .1459+2 0.093 –.475–1 .169–1
200 .2766+3 1.161 .258+0 .489–1 .9155+3 0.714 –.740–1 .507–2 .1384+4 0.749 –.734–1 .433–2 .1013+3 1.978 .321+0 .475–4 .1018+3 1.112 .185+0 .245–1 .2433+3 1.096 .168+0 .231–1 .3277+3 0.514 .502–1 –.591–2 .4980+3 0.590 .476–1 –.634–2 .2167+2 1.977 .251+0 .615–4 .8057+1 0.973 .129+0 .193–1
500 .1789+3 1.480 .751–1 .924–2 .3749+3 1.079 –.574–2 .287–1 .5581+3 1.096 .583–3 .278–1 .4087+2 1.980 .266+0 –.530–4 .4776+2 1.569 .138+0 .261–2 .1032+3 1.556 .115+0 .240–2 .1269+3 1.196 –.216–1 .889–2 .1870+3 1.222 –.195–1 .893–2 .6080+1 1.981 .250+0 –.318–4 .3105+1 1.580 .152+0 .119–2
1000 .9640+2 1.617 –.296–1 .387–2 .1205+3 1.220 .198+0 .507–1 .1767+3 1.213 .206+0 .502–1 .1596+2 1.982 .118+0 –.131–3 .1905+2 1.680 –.137–1 –.795–3 .3865+2 1.693 –.228–1 .715–3 .3149+2 1.332 .128+0 .300–1 .4562+2 1.325 .136+0 .298–1 .1996+1 1.982 .119+0 –.117–3 .1116+1 1.698 –.108–1 –.118–2
151
E (eV) 1500 .5787+2 1.646 .222–1 .578–2 .5101+2 1.220 .388+0 .674–1 .7414+2 1.201 .394+0 .681–1 .8492+1 1.984 .994–2 –.176–3 .9792+1 1.679 –.246–2 –.383–3 .1923+2 1.708 –.264–2 .240–2 .1156+2 1.303 .310+0 .466–1 .1658+2 1.281 .317+0 .471–1 .9895+0 1.984 .130–1 –.166–3 .5475+0 1.693 –.773–2 –.773–3
2000 .3751+2 1.642 .126+0 .848–2 .2543+2 1.181 .546+0 .827–1 .3671+2 1.156 .549+0 .845–1 .5272+1 1.986 –.557–1 –.207–3 .5794+1 1.654 .753–1 .996–3 .1113+2 1.694 .826–1 .436–2 .5285+1 1.244 .470+0 .621–1 .7532+1 1.214 .475+0 .637–1 .5910+0 1.986 –.535–1 –.197–3 .3156+0 1.666 .669–1 .448–3
3000 .1837+2 1.603 .362+0 .147–1 .8484+1 1.081 .789+0 .113+0 .1212+2 1.050 .786+0 .117+0 .2594+1 1.990 –.981–1 –.246–3 .2567+1 1.589 .284+0 .605–2 .4784+1 1.641 .305+0 .926–2 .1593+1 1.120 .727+0 .936–1 .2248+1 1.085 .725+0 .975–1 .2794+0 1.990 –.980–1 –.238–3 .1361+0 1.596 .275+0 .526–2
4000 .1030+2 1.551 .586+0 .220–1 .3604+1 0.981 .966+0 .145+0 .5107+1 0.951 .957+0 .151+0 .1527+1 1.992 –.669–1 –.270–3 .1364+1 1.521 .496+0 .136–1 .2490+1 1.581 .528+0 .158–1 .6368+0 1.007 .918+0 .126+0 .8919+0 0.974 .910+0 .132+0 .1611+0 1.992 –.687–1 –.264–3 .7128–1 1.526 .487+0 .126–1
5000 .6324+1 1.495 .786+0 .303–1 .1781+1 0.890 .110+1 .175+0 .2507+1 0.864 .109+1 .182+0 .9958+0 1.993 .557–2 –.287–3 .8102+0 1.455 .687+0 .229–1 .1455+1 1.519 .730+0 .238–1 .3021+0 0.908 .106+1 .158+0 .4205+0 0.878 .105+1 .165+0 .1037+0 1.993 .262–2 –.281–3 .4194–1 1.461 .679+0 .220–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Sn, Z = 50 Shell 1s1/2 Eb = 29204 eV 2s1/2 Eb = 4469 eV 2 p1/2 Eb = 4160 eV 2 p3/2 Eb = 3933 eV 3s1/2 Eb = 888 eV 3 p1/2 Eb = 761 eV 3 p3/2 Eb = 719 eV 3d3/2 Eb = 498 eV 3d5/2 Eb = 489 eV 4s1/2 Eb = 141 eV 4 p1/2 Eb = 102 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .6905+1 1.956 –.118+1 –.969–3 .2771+2 1.962 .104+1 –.146–3 .5589+2 0.973 –.385+0 –.259–1 .1176+3 0.973 –.394+0 –.269–1 .7977+2 1.971 .719+0 .806–4 .1314+3 0.883 .239+0 .110+0 .3080+3 0.859 .211+0 .101+0 .1221+4 0.460 –.545–1 –.359–2 .1861+4 0.492 –.551–1 –.447–2 .1505+3 1.971 .302+0 .142–3 .1324+3 0.487 –.261–1 .398–1
200 .6862+1 1.955 –.989+0 –.102–2 .2678+2 1.964 .827+0 –.248–3 .5284+2 1.116 –.390+0 –.172–1 .1106+3 1.133 –.408+0 –.153–1 .7004+2 1.972 .604+0 –.562–5 .1157+3 1.169 .298+0 .573–1 .2652+3 1.155 .263+0 .514–1 .8656+3 0.706 –.796–1 .374–2 .1309+4 0.743 –.792–1 .300–2 .1004+3 1.976 .331+0 .548–4 .1027+3 1.107 .188+0 .260–1
500 .6704+1 1.952 –.641+0 –.106–2 .2415+2 1.969 .461+0 –.377–3 .4462+2 1.285 –.265+0 .255–2 .9209+2 1.325 –.286+0 .743–2 .4930+2 1.974 .377+0 –.132–3 .7997+2 1.464 .109+0 .116–1 .1746+3 1.472 .836–1 .103–1 .3691+3 1.069 –.156–1 .280–1 .5499+3 1.088 –.906–2 .270–1 .4181+2 1.979 .276+0 –.559–4 .4935+2 1.562 .149+0 .319–2
1000 .6423+1 1.948 –.290+0 –.105–2 .2043+2 1.976 .159+0 –.457–3 .3407+2 1.376 –.342–1 .188–1 .6888+2 1.433 –.455–1 .240–1 .3043+2 1.977 .148+0 –.219–3 .4631+2 1.585 –.188–1 .195–2 .9621+2 1.613 –.300–1 .403–2 .1235+3 1.217 .186+0 .502–1 .1813+3 1.212 .195+0 .497–1 .1667+2 1.981 .129+0 –.142–3 .2012+2 1.679 –.924–2 –.791–3
152
E (eV) 1500 .6154+1 1.943 –.490–1 –.103–2 .1747+2 1.981 .133–1 –.492–3 .2655+2 1.404 .162+0 .285–1 .5275+2 1.470 .162+0 .328–1 .2055+2 1.981 .173–1 –.263–3 .2914+2 1.605 .149–1 .227–2 .5863+2 1.646 .134–1 .572–2 .5354+2 1.223 .376+0 .669–1 .7781+2 1.204 .384+0 .674–1 .8948+1 1.983 .197–1 –.193–3 .1047+2 1.682 –.810–2 –.583–3
2000 .5902+1 1.938 .143+0 –.102–2 .1508+2 1.985 –.565–1 –.511–3 .2108+2 1.409 .332+0 .359–1 .4125+2 1.482 .343+0 .390–1 .1475+2 1.984 –.567–1 –.290–3 .1954+2 1.596 .104+0 .442–2 .3841+2 1.646 .111+0 .829–2 .2713+2 1.189 .535+0 .818–1 .3914+2 1.163 .540+0 .835–1 .5581+1 1.985 –.493–1 –.227–3 .6240+1 1.659 .625–1 .600–3
3000 .5441+1 1.929 .445+0 –.989–3 .1152+2 1.990 –.789–1 –.523–3 .1390+2 1.392 .606+0 .480–1 .2652+2 1.471 .636+0 .487–1 .8599+1 1.989 –.103+0 –.321–3 .1004+2 1.551 .321+0 .109–1 .1910+2 1.611 .342+0 .142–1 .9239+1 1.093 .783+0 .112+0 .1319+2 1.062 .780+0 .116+0 .2762+1 1.989 –.996–1 –.270–3 .2796+1 1.597 .264+0 .524–2
4000 .5028+1 1.920 .687+0 –.965–3 .9041+1 1.992 –.240–1 –.527–3 .9612+1 1.359 .827+0 .592–1 .1796+2 1.442 .873+0 .575–1 .5578+1 1.991 –.727–1 –.341–3 .5827+1 1.495 .532+0 .192–1 .1083+2 1.561 .566+0 .213–1 .3977+1 0.995 .963+0 .142+0 .5631+1 0.964 .954+0 .148+0 .1632+1 1.991 –.770–1 –.298–3 .1499+1 1.531 .473+0 .124–1
5000 .4655+1 1.910 .893+0 –.945–3 .7247+1 1.992 .676–1 –.527–3 .6897+1 1.320 .101+1 .697–1 .1266+2 1.405 .107+1 .659–1 .3881+1 1.992 –.210–2 –.354–3 .3670+1 1.438 .719+0 .285–1 .6697+1 1.508 .765+0 .290–1 .1984+1 0.907 .110+1 .172+0 .2791+1 0.878 .109+1 .179+0 .1068+1 1.992 –.119–1 –.318–3 .8955+0 1.467 .663+0 .211–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Sn, Z = 50 (continued) Shell 4 p3/2 Eb = 93 eV 4d3/2 Eb = 29 eV 4d5/2 Eb = 28 eV 5s1/2 Eb = 12 eV 5 p1/2 Eb = 7 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .3460+3 0.510 –.166–1 .370–1 .2286+3 −.744 .420–1 .403–1 .3606+3 −.652 .682–1 .319–1 .5767+2 1.966 .179+0 .123–3 .2072+2 0.102 –.473–1 .178–1
200 .2482+3 1.090 .170+0 .245–1 .3491+3 0.496 .588–1 –.390–2 .5318+3 0.576 .564–1 –.460–2 .2586+2 1.975 .254+0 .675–4 .1153+2 0.968 .127+0 .198–1
500 .1076+3 1.548 .125+0 .291–2 .1400+3 1.185 –.250–1 .779–2 .2068+3 1.214 –.233–1 .786–2 .7314+1 1.979 .258+0 –.325–4 .4439+1 1.573 .163+0 .153–2
1000 .4108+2 1.691 –.198–1 .691–3 .3604+2 1.334 .114+0 .287–1 .5229+2 1.328 .122+0 .284–1 .2413+1 1.981 .129+0 –.127–3 .1608+1 1.698 –.537–2 –.122–2
E (eV) 1500 .2064+2 1.710 –.938–2 .227–2 .1346+2 1.311 .294+0 .450–1 .1934+2 1.289 .303+0 .455–1 .1200+1 1.983 .226–1 –.180–3 .7950+0 1.697 –.127–1 –.952–3
2000 .1203+2 1.699 .690–1 .414–2 .6231+1 1.256 .455+0 .602–1 .8888+1 1.226 .461+0 .617–1 .7180+0 1.985 –.467–1 –.216–3 .4608+0 1.672 .542–1 .562–4
3000 .5222+1 1.651 .284+0 .876–2 .1908+1 1.136 .715+0 .910–1 .2695+1 1.100 .714+0 .949–1 .3400+0 1.989 –.990–1 –.261–3 .2002+0 1.606 .254+0 .442–2
4000 .2738+1 1.593 .505+0 .150–1 .7712+0 1.024 .910+0 .122+0 .1081+1 0.988 .902+0 .128+0 .1965+0 1.991 –.782–1 –.290–3 .1056+0 1.538 .462+0 .113–1
5000 .1609+1 1.533 .706+0 .223–1 .3687+0 0.927 .105+1 .154+0 .5133+0 0.895 .104+1 .161+0 .1268+0 1.992 –.147–1 –.310–3 .6250–1 1.474 .654+0 .201–1
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .6585+1 1.954 –.121+1 –.107–2 .2630+2 1.960 .105+1 –.160–3 .5273+2 0.971 –.399+0 –.277–1 .1111+3 0.970 –.409+0 –.287–1 .7556+2 1.969 .741+0 .898–4
200 .6541+1 1.953 –.102+1 –.113–2 .2544+2 1.962 .847+0 –.272–3 .4997+2 1.113 –.405+0 –.188–1 .1047+3 1.130 –.424+0 –.167–1 .6675+2 1.970 .624+0 –.460–5
500 .6398+1 1.950 –.666+0 –.117–2 .2304+2 1.967 .481+0 –.414–3 .4254+2 1.280 –.280+0 .158–2 .8791+2 1.321 –.303+0 .682–2 .4776+2 1.972 .394+0 –.142–3
1000 .6143+1 1.945 –.315+0 –.116–2 .1964+2 1.974 .176+0 –.503–3 .3288+2 1.371 –.502–1 .183–1 .6658+2 1.431 –.632–1 .239–1 .3003+2 1.976 .163+0 –.240–3
E (eV) 1500 .5895+1 1.941 –.727–1 –.114–2 .1690+2 1.979 .250–1 –.542–3 .2588+2 1.401 .145+0 .280–1 .5149+2 1.469 .144+0 .327–1 .2052+2 1.979 .287–1 –.288–3
2000 .5663+1 1.936 .119+0 –.113–2 .1467+2 1.984 –.500–1 –.563–3 .2073+2 1.408 .314+0 .355–1 .4062+2 1.482 .324+0 .391–1 .1486+2 1.982 –.494–1 –.318–3
3000 .5238+1 1.927 .422+0 –.109–2 .1131+2 1.989 –.827–1 –.579–3 .1387+2 1.393 .590+0 .476–1 .2648+2 1.475 .620+0 .486–1 .8762+1 1.987 –.104+0 –.354–3
4000 .4855+1 1.917 .666+0 –.107–2 .8944+1 1.991 –.361–1 –.585–3 .9702+1 1.362 .813+0 .587–1 .1813+2 1.448 .859+0 .573–1 .5727+1 1.990 –.826–1 –.377–3
5000 .4508+1 1.908 .871+0 –.105–2 .7215+1 1.991 .488–1 –.586–3 .7027+1 1.325 .995+0 .690–1 .1290+2 1.413 .105+1 .653–1 .4006+1 1.991 –.188–1 –.393–3
Sb, Z = 51 Shell 1s1/2 Eb = 30496 eV 2s1/2 Eb = 4703 eV 2 p1/2 Eb = 4385 eV 2 p3/2 Eb = 4137 eV 3s1/2 Eb = 949 eV
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Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Sb, Z = 51 (continued) Shell 3 p1/2 Eb = 817 eV 3 p3/2 Eb = 771 eV 3d3/2 Eb = 542 eV 3d5/2 Eb = 533 eV 4s1/2 Eb = 157 eV 4 p1/2 Eb = 114 eV 4 p3/2 Eb = 104 eV 4d3/2 Eb = 38 eV 4d5/2 Eb = 37 eV 5s1/2 Eb = 15 eV 5 p1/2 Eb = 8 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1247+3 0.880 .242+0 .113+0 .2936+3 0.855 .213+0 .103+0 .1134+4 0.459 –.578–1 –.468–2 .1726+4 0.493 –.587–1 –.556–2 .1460+3 1.968 .317+0 .159–3 .1328+3 0.497 –.219–1 .422–1 .3508+3 0.517 –.126–1 .391–1 .2574+3 −.705 .257–1 .515–1 .4063+3 −.605 .534–1 .426–1 .6532+2 1.963 .182+0 .137–3 .2709+2 0.105 –.472–1 .186–1
200 .1104+3 1.164 .304+0 .602–1 .2543+3 1.150 .268+0 .538–1 .8191+3 0.698 –.851–1 .234–2 .1238+4 0.737 –.850–1 .161–2 .9928+2 1.973 .342+0 .632–4 .1035+3 1.102 .191+0 .275–1 .2532+3 1.084 .171+0 .258–1 .3676+3 0.477 .670–1 –.142–2 .5612+3 0.561 .650–1 –.242–2 .2972+2 1.973 .258+0 .750–4 .1494+2 0.957 .125+0 .203–1
500 .7756+2 1.457 .119+0 .129–1 .1702+3 1.465 .918–1 .114–1 .3629+3 1.060 –.256–1 .271–1 .5403+3 1.080 –.188–1 .262–1 .4263+2 1.977 .287+0 –.588–4 .5086+2 1.555 .160+0 .377–2 .1119+3 1.539 .134+0 .341–2 .1524+3 1.174 –.274–1 .675–2 .2254+3 1.207 –.263–1 .686–2 .8514+1 1.978 .264+0 –.330–4 .5747+1 1.567 .173+0 .183–2
1000 .4592+2 1.580 –.169–1 .215–2 .9583+2 1.610 –.298–1 .423–2 .1263+3 1.214 .173+0 .498–1 .1852+3 1.209 .184+0 .492–1 .1736+2 1.979 .141+0 –.154–3 .2118+2 1.678 –.406–2 –.769–3 .4351+2 1.689 –.163–1 .682–3 .4067+2 1.335 .101+0 .275–1 .5907+2 1.331 .109+0 .271–1 .2829+1 1.979 .140+0 –.136–3 .2100+1 1.698 .870–3 –.125–2
154
E (eV) 1500 .2933+2 1.604 .814–2 .210–2 .5925+2 1.646 .539–2 .569–2 .5597+2 1.226 .363+0 .661–1 .8130+2 1.207 .372+0 .665–1 .9399+1 1.981 .297–1 –.210–3 .1115+2 1.684 –.127–1 –.755–3 .2209+2 1.712 –.152–1 .216–2 .1547+2 1.319 .278+0 .433–1 .2224+2 1.298 .287+0 .437–1 .1412+1 1.981 .325–1 –.195–3 .1046+1 1.700 –.168–1 –.113–2
2000 .1990+2 1.598 .914–1 .402–2 .3924+2 1.648 .973–1 .813–2 .2880+2 1.196 .525+0 .811–1 .4153+2 1.170 .531+0 .828–1 .5891+1 1.983 –.421–1 –.248–3 .6696+1 1.664 .505–1 .246–3 .1295+2 1.704 .560–1 .394–2 .7241+1 1.268 .441+0 .585–1 .1034+2 1.237 .447+0 .599–1 .8460+0 1.983 –.396–1 –.235–3 .6090+0 1.677 .424–1 –.297–3
3000 .1039+2 1.557 .302+0 .101–1 .1981+2 1.618 .323+0 .138–1 .1002+2 1.105 .776+0 .110+0 .1428+2 1.073 .775+0 .114+0 .2933+1 1.987 –.100+0 –.297–3 .3033+1 1.605 .243+0 .447–2 .5678+1 1.659 .263+0 .829–2 .2254+1 1.152 .703+0 .883–1 .3183+1 1.114 .703+0 .922–1 .4016+0 1.987 –.993–1 –.286–3 .2668+0 1.614 .233+0 .363–2
4000 .6099+1 1.503 .511+0 .181–1 .1134+2 1.572 .545+0 .205–1 .4369+1 1.010 .960+0 .140+0 .6178+1 0.977 .952+0 .146+0 .1740+1 1.990 –.858–1 –.328–3 .1639+1 1.541 .449+0 .111–1 .2999+1 1.604 .481+0 .141–1 .9207+0 1.042 .902+0 .119+0 .1290+1 1.004 .895+0 .125+0 .2325+0 1.990 –.866–1 –.319–3 .1416+0 1.549 .437+0 .997–2
5000 .3875+1 1.449 .698+0 .269–1 .7071+1 1.521 .744+0 .278–1 .2200+1 0.923 .110+1 .169+0 .3091+1 0.893 .109+1 .176+0 .1142+1 1.991 –.281–1 –.351–3 .9855+0 1.479 .639+0 .193–1 .1772+1 1.547 .682+0 .209–1 .4435+0 0.946 .105+1 .149+0 .6175+0 0.911 .104+1 .157+0 .1503+0 1.991 –.306–1 –.343–3 .8424–1 1.485 .629+0 .181–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Sb, Z = 51 (continued) Shell 5 p3/2 Eb = 8 eV
σ β γ δ
100 .6269+2 0.183 –.482–1 .191–1
200 .3384+2 0.970 .120+0 .206–1
500 .1178+2 1.545 .147+0 .201–2
1000 .4035+1 1.704 –.119–1 .891–4
E (eV) 1500 .1942+1 1.725 –.195–1 .167–2
2000 .1106+1 1.715 .479–1 .335–2
3000 .4697+0 1.667 .252+0 .747–2
4000 .2440+0 1.611 .470+0 .130–1
5000 .1427+0 1.553 .672+0 .199–1
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .6286+1 1.951 –.123+1 –.119–2 .2497+2 1.958 .108+1 –.175–3 .4978+2 0.967 –.414+0 –.295–1 .1050+3 0.966 –.424+0 –.305–1 .7166+2 1.966 .765+0 .100–3 .1182+3 0.877 .245+0 .115+0 .2799+3 0.851 .214+0 .106+0 .1051+4 0.458 –.611–1 –.581–2 .1602+4 0.493 –.621–1 –.669–2
200 .6241+1 1.950 –.104+1 –.125–2 .2417+2 1.960 .867+0 –.298–3 .4729+2 1.109 –.420+0 –.203–1 .9928+2 1.126 –.440+0 –.180–1 .6365+2 1.967 .645+0 –.266–5 .1053+3 1.156 .311+0 .630–1 .2439+3 1.142 .271+0 .563–1 .7740+3 0.690 –.907–1 .862–3 .1172+4 0.731 –.907–1 .138–3
500 .6110+1 1.947 –.692+0 –.129–2 .2200+2 1.965 .502+0 –.453–3 .4056+2 1.275 –.296+0 .583–3 .8396+2 1.317 –.320+0 .619–2 .4624+2 1.970 .412+0 –.153–3 .7512+2 1.449 .130+0 .143–1 .1658+3 1.457 .100+0 .125–1 .3555+3 1.050 –.357–1 .263–1 .5301+3 1.072 –.287–1 .252–1
1000 .5878+1 1.943 –.340+0 –.128–2 .1888+2 1.972 .193+0 –.553–3 .3172+2 1.367 –.663–1 .177–1 .6433+2 1.428 –.811–1 .238–1 .2960+2 1.974 .179+0 –.261–3 .4542+2 1.576 –.144–1 .239–2 .9528+2 1.606 –.291–1 .447–2 .1285+3 1.210 .161+0 .493–1 .1886+3 1.207 .172+0 .486–1
E (eV) 1500 .5651+1 1.938 –.967–1 –.126–2 .1634+2 1.978 .373–1 –.597–3 .2521+2 1.398 .129+0 .276–1 .5024+2 1.468 .126+0 .328–1 .2046+2 1.977 .406–1 –.315–3 .2946+2 1.603 .223–2 .196–2 .5975+2 1.645 –.189–2 .569–2 .5825+2 1.228 .350+0 .656–1 .8464+2 1.210 .360+0 .658–1
2000 .5437+1 1.933 .960–1 –.124–2 .1426+2 1.982 –.430–1 –.621–3 .2036+2 1.406 .298+0 .352–1 .3995+2 1.483 .306+0 .392–1 .1494+2 1.980 –.415–1 –.350–3 .2021+2 1.599 .794–1 .366–2 .3999+2 1.651 .843–1 .801–2 .3044+2 1.202 .514+0 .804–1 .4389+2 1.176 .521+0 .819–1
3000 .5043+1 1.924 .400+0 –.121–2 .1109+2 1.988 –.855–1 –.641–3 .1382+2 1.394 .575+0 .474–1 .2640+2 1.478 .604+0 .487–1 .8911+1 1.986 –.105+0 –.391–3 .1073+2 1.562 .284+0 .941–2 .2049+2 1.625 .304+0 .134–1 .1080+2 1.117 .769+0 .109+0 .1540+2 1.083 .768+0 .113+0
4000 .4688+1 1.915 .644+0 –.118–2 .8836+1 1.990 –.471–1 –.649–3 .9773+1 1.365 .797+0 .580–1 .1827+2 1.453 .843+0 .568–1 .5867+1 1.989 –.914–1 –.417–3 .6365+1 1.511 .489+0 .168–1 .1185+2 1.581 .524+0 .197–1 .4776+1 1.025 .956+0 .137+0 .6749+1 0.990 .949+0 .143+0
5000 .4365+1 1.906 .847+0 –.116–2 .7173+1 1.991 .310–1 –.647–3 .7144+1 1.331 .981+0 .685–1 .1311+2 1.421 .104+1 .649–1 .4127+1 1.991 –.343–1 –.433–3 .4078+1 1.459 .676+0 .256–1 .7446+1 1.533 .723+0 .269–1 .2428+1 0.940 .110+1 .166+0 .3408+1 0.907 .109+1 .174+0
Te, Z = 52 Shell 1s1/2 Eb = 31820 eV 2s1/2 Eb = 4945 eV 2 p1/2 Eb = 4618 eV 2 p3/2 Eb = 4347 eV 3s1/2 Eb = 1012 eV 3 p1/2 Eb = 876 eV 3 p3/2 Eb = 825 eV 3d3/2 Eb = 589 eV 3d5/2 Eb = 578 eV
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Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Te, Z = 52 (continued) Shell 4s1/2 Eb = 174 eV 4 p1/2 Eb = 127 eV 4 p3/2 Eb = 117 eV 4d3/2 Eb = 48 eV 4d5/2 Eb = 46 eV 5s1/2 Eb = 18 eV 5 p1/2 Eb = 9 eV 5 p3/2 Eb = 9 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .1414+3 1.966 .333+0 .178–3 .1324+3 0.504 –.181–1 .448–1 .3519+3 0.522 –.919–2 .415–1 .2841+3 −.667 .110–1 .621–1 .4514+3 −.563 .399–1 .526–1 .7247+2 1.959 .186+0 .154–3 .3331+2 0.104 –.473–1 .193–1 .7845+2 0.184 –.478–1 .197–1
200 .9796+2 1.971 .354+0 .733–4 .1040+3 1.093 .193+0 .291–1 .2563+3 1.074 .173+0 .273–1 .3830+3 0.460 .753–1 .150–2 .5880+3 0.548 .736–1 .161–3 .3339+2 1.970 .261+0 .840–4 .1816+2 0.943 .122+0 .207–1 .4186+2 0.956 .117+0 .210–1
500 .4334+2 1.975 .298+0 –.617–4 .5221+2 1.548 .171+0 .439–2 .1157+3 1.530 .143+0 .396–2 .1640+3 1.163 –.291–1 .580–2 .2434+3 1.199 –.284–1 .593–2 .9694+1 1.976 .271+0 –.329–4 .6993+1 1.562 .183+0 .210–2 .1454+2 1.538 .155+0 .230–2
1000 .1801+2 1.977 .152+0 –.167–3 .2221+2 1.676 .188–2 –.727–3 .4586+2 1.686 –.121–1 .688–3 .4532+2 1.336 .876–1 .263–1 .6596+2 1.333 .966–1 .259–1 .3246+1 1.978 .150+0 –.146–3 .2580+1 1.698 .782–2 –.127–2 .5016+1 1.702 –.672–2 .290–4
E (eV) 1500 .9844+1 1.979 .402–1 –.228–3 .1182+2 1.685 –.163–1 –.905–3 .2353+2 1.713 –.201–1 .207–2 .1755+2 1.326 .262+0 .419–1 .2527+2 1.305 .272+0 .421–1 .1625+1 1.980 .426–1 –.211–3 .1293+1 1.703 –.198–1 –.129–2 .2427+1 1.728 –.238–1 .155–2
2000 .6202+1 1.982 –.345–1 –.271–3 .7157+1 1.668 .395–1 –.813–4 .1389+2 1.708 .441–1 .377–2 .8314+1 1.279 .426+0 .567–1 .1188+2 1.248 .433+0 .580–1 .9755+0 1.982 –.318–1 –.256–3 .7566+0 1.683 .314–1 –.626–3 .1388+1 1.720 .358–1 .315–2
3000 .3106+1 1.986 –.100+0 –.326–3 .3277+1 1.612 .224+0 .376–2 .6147+1 1.668 .243+0 .789–2 .2628+1 1.166 .691+0 .858–1 .3714+1 1.127 .691+0 .896–1 .4640+0 1.986 –.987–1 –.313–3 .3339+0 1.623 .213+0 .289–2 .5929+0 1.676 .232+0 .704–2
4000 .1851+1 1.989 –.935–1 –.362–3 .1785+1 1.551 .425+0 .985–2 .3270+1 1.615 .458+0 .132–1 .1085+1 1.059 .893+0 .115+0 .1521+1 1.019 .886+0 .121+0 .2691+0 1.989 –.940–1 –.350–3 .1784+0 1.559 .414+0 .881–2 .3096+0 1.622 .446+0 .122–1
5000 .1218+1 1.990 –.428–1 –.385–3 .1080+1 1.492 .614+0 .178–1 .1943+1 1.561 .658+0 .198–1 .5269+0 0.965 .105+1 .146+0 .7334+0 0.928 .104+1 .153+0 .1743+0 1.990 –.452–1 –.377–3 .1066+0 1.498 .603+0 .164–1 .1819+0 1.566 .647+0 .186–1
σ β γ δ σ β γ δ
100 .6006+1 1.949 –.126+1 –.131–2 .2373+2 1.956 .110+1 –.191–3
200 .5960+1 1.948 –.107+1 –.137–2 .2299+2 1.958 .889+0 –.326–3
500 .5839+1 1.945 –.717+0 –.141–2 .2101+2 1.963 .522+0 –.496–3
1000 .5627+1 1.940 –.365+0 –.141–2 .1815+2 1.970 .211+0 –.607–3
E (eV) 1500 .5419+1 1.936 –.121+0 –.139–2 .1580+2 1.976 .502–1 –.656–3
2000 .5221+1 1.931 .724–1 –.137–2 .1385+2 1.980 –.351–1 –.684–3
3000 .4857+1 1.922 .377+0 –.134–2 .1087+2 1.986 –.872–1 –.707–3
4000 .4527+1 1.912 .622+0 –.131–2 .8721+1 1.989 –.570–1 –.717–3
5000 .4227+1 1.903 .825+0 –.128–2 .7122+1 1.990 .145–1 –.716–3
I, Z = 53 Shell 1s1/2 Eb = 33176 eV 2s1/2 Eb = 5195 eV
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Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables I, Z = 53 (continued) Shell 2 p1/2 Eb = 4858 eV 2 p3/2 Eb = 4563 eV 3s1/2 Eb = 1078 eV 3 p1/2 Eb = 937 eV 3 p3/2 Eb = 881 eV 3d3/2 Eb = 638 eV 3d5/2 Eb = 626 eV 4s1/2 Eb = 193 eV 4 p1/2 Eb = 141 eV 4 p3/2 Eb = 131 eV 4d3/2 Eb = 58 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .4705+2 0.964 –.428+0 –.312–1 .9940+2 0.962 –.439+0 –.323–1 .6795+2 1.964 .789+0 .112–3 .1122+3 0.872 .246+0 .118+0 .2669+3 0.845 .213+0 .108+0 .9738+3 0.455 –.644–1 –.696–2 .1485+4 0.493 –.655–1 –.786–2 .1363+3 1.963 .351+0 .200–3 .1313+3 0.508 –.146–1 .475–1 .3514+3 0.523 –.607–2 .442–1 .3100+3 −.632 –.239–2 .718–1
200 .4482+2 1.105 –.435+0 –.220–1 .9422+2 1.122 –.457+0 –.195–1 .6069+2 1.965 .666+0 –.547–6 .1004+3 1.150 .317+0 .661–1 .2339+3 1.135 .275+0 .589–1 .7313+3 0.682 –.965–1 –.713–3 .1107+4 0.724 –.966–1 –.143–2 .9618+2 1.969 .368+0 .849–4 .1040+3 1.085 .196+0 .309–1 .2584+3 1.065 .175+0 .290–1 .3969+3 0.440 .828–1 .494–2
500 .3869+2 1.270 –.310+0 –.415–3 .8022+2 1.314 –.337+0 .557–2 .4473+2 1.968 .430+0 –.164–3 .7271+2 1.442 .140+0 .157–1 .1614+3 1.450 .108+0 .137–1 .3477+3 1.041 –.459–1 .252–1 .5186+3 1.064 –.387–1 .242–1 .4387+2 1.973 .309+0 –.647–4 .5339+2 1.541 .182+0 .501–2 .1192+3 1.523 .152+0 .450–2 .1751+3 1.153 –.298–1 .492–2
1000 .3060+2 1.362 –.826–1 .171–1 .6216+2 1.425 –.992–1 .237–1 .2912+2 1.972 .194+0 –.284–3 .4487+2 1.572 –.112–1 .269–2 .9460+2 1.601 –.278–1 .475–2 .1303+3 1.207 .148+0 .488–1 .1914+3 1.204 .160+0 .480–1 .1861+2 1.976 .165+0 –.180–3 .2318+2 1.673 .854–2 –.665–3 .4815+2 1.682 –.732–2 .709–3 .5003+2 1.336 .751–1 .251–1
157
E (eV) 1500 .2455+2 1.394 .112+0 .272–1 .4899+2 1.467 .108+0 .328–1 .2037+2 1.975 .531–1 –.345–3 .2953+2 1.601 –.288–2 .186–2 .6014+2 1.645 –.849–2 .572–2 .6038+2 1.229 .338+0 .651–1 .8774+2 1.212 .349+0 .652–1 .1027+2 1.978 .510–1 –.248–3 .1249+2 1.687 –.189–1 –.103–2 .2496+2 1.714 –.241–1 .199–2 .1972+2 1.333 .247+0 .405–1
2000 .1999+2 1.404 .281+0 .348–1 .3926+2 1.483 .288+0 .393–1 .1500+2 1.979 –.330–1 –.384–3 .2048+2 1.600 .681–1 .334–2 .4066+2 1.653 .719–1 .792–2 .3204+2 1.208 .503+0 .797–1 .4619+2 1.181 .511+0 .811–1 .6509+1 1.980 –.265–1 –.296–3 .7620+1 1.672 .295–1 –.378–3 .1484+2 1.712 .330–1 .363–2 .9449+1 1.289 .410+0 .550–1
3000 .1374+2 1.394 .558+0 .470–1 .2628+2 1.481 .587+0 .488–1 .9044+1 1.984 –.105+0 –.430–3 .1104+2 1.566 .265+0 .872–2 .2114+2 1.631 .286+0 .131–1 .1161+2 1.127 .762+0 .107+0 .1654+2 1.093 .761+0 .111+0 .3280+1 1.984 –.991–1 –.357–3 .3526+1 1.619 .205+0 .309–2 .6629+1 1.675 .224+0 .752–2 .3033+1 1.181 .678+0 .834–1
4000 .9826+1 1.367 .781+0 .575–1 .1838+2 1.459 .828+0 .567–1 .6000+1 1.988 –.990–1 –.460–3 .6625+1 1.518 .468+0 .158–1 .1235+2 1.590 .503+0 .190–1 .5198+1 1.039 .953+0 .135+0 .7340+1 1.002 .946+0 .141+0 .1962+1 1.987 –.100+0 –.397–3 .1935+1 1.560 .402+0 .875–2 .3550+1 1.626 .434+0 .125–1 .1266+1 1.076 .883+0 .112+0
5000 .7248+1 1.335 .967+0 .679–1 .1330+2 1.429 .103+1 .645–1 .4243+1 1.990 –.487–1 –.478–3 .4280+1 1.468 .655+0 .242–1 .7819+1 1.545 .702+0 .259–1 .2668+1 0.955 .110+1 .163+0 .3740+1 0.921 .109+1 .171+0 .1296+1 1.989 –.563–1 –.424–3 .1178+1 1.503 .589+0 .162–1 .2121+1 1.574 .634+0 .187–1 .6192+0 0.983 .104+1 .141+0
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables I, Z = 53 (continued) Shell 4d5/2 Eb = 56 eV 5s1/2 Eb = 20 eV 5 p1/2 Eb = 10 eV 5 p3/2 Eb = 10 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .4922+3 −.523 .276–1 .620–1 .7981+2 1.955 .188+0 .172–3 .3945+2 0.098 –.475–1 .200–1 .9425+2 0.180 –.480–1 .203–1
200 .6101+3 0.532 .818–1 .322–2 .3712+2 1.967 .264+0 .941–4 .2130+2 0.927 .119+0 .212–1 .4982+2 0.944 .115+0 .214–1
500 .2602+3 1.191 –.298–1 .508–2 .1088+2 1.974 .276+0 –.331–4 .8205+1 1.554 .192+0 .238–2 .1727+2 1.530 .163+0 .260–2
1000 .7287+2 1.334 .843–1 .247–1 .3672+1 1.976 .161+0 –.156–3 .3059+1 1.697 .155–1 –.127–2 .6002+1 1.700 –.923–3 –.155–4
E (eV) 1500 .2841+2 1.312 .257+0 .406–1 .1843+1 1.978 .530–1 –.228–3 .1542+1 1.706 –.217–1 –.143–2 .2917+1 1.729 –.273–1 .143–2
2000 .1350+2 1.258 .419+0 .562–1 .1108+1 1.980 –.236–1 –.278–3 .9068+0 1.688 .214–1 –.926–3 .1674+1 1.725 .248–1 .297–2
3000 .4286+1 1.140 .679+0 .871–1 .5283+0 1.984 –.973–1 –.342–3 .4030+0 1.631 .194+0 .220–2 .7196+0 1.685 .212+0 .665–2
4000 .1773+1 1.034 .877+0 .118+0 .3069+0 1.987 –.100+0 –.384–3 .2166+0 1.569 .390+0 .768–2 .3777+0 1.633 .423+0 .115–1
5000 .8615+0 0.944 .103+1 .149+0 .1991+0 1.989 –.582–1 –.412–3 .1301+0 1.509 .578+0 .148–1 .2229+0 1.580 .622+0 .174–1
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .5740+1 1.946 –.130+1 –.144–2 .2257+2 1.954 .112+1 –.207–3 .4450+2 0.959 –.442+0 –.330–1 .9415+2 0.957 –.453+0 –.341–1 .6434+2 1.961 .815+0 .126–3 .1064+3 0.867 .248+0 .122+0
200 .5697+1 1.945 –.110+1 –.151–2 .2189+2 1.955 .910+0 –.356–3 .4251+2 1.100 –.449+0 –.236–1 .8950+2 1.118 –.473+0 –.210–1 .5778+2 1.963 .690+0 .256–5 .9576+2 1.142 .322+0 .692–1
500 .5583+1 1.942 –.743+0 –.155–2 .2007+2 1.961 .543+0 –.542–3 .3693+2 1.265 –.326+0 –.146–2 .7669+2 1.309 –.354+0 .492–2 .4316+2 1.965 .449+0 –.176–3 .7031+2 1.434 .151+0 .172–1
1000 .5390+1 1.937 –.391+0 –.155–2 .1745+2 1.968 .229+0 –.665–3 .2951+2 1.358 –.989–1 .165–1 .6004+2 1.422 –.118+0 .236–1 .2858+2 1.969 .211+0 –.309–3 .4423+2 1.567 –.729–2 .303–2
E (eV) 1500 .5199+1 1.933 –.145+0 –.153–2 .1527+2 1.974 .638–1 –.719–3 .2389+2 1.391 .953–1 .268–1 .4774+2 1.466 .893–1 .329–1 .2022+2 1.973 .662–1 –.377–3 .2953+2 1.600 –.721–2 .179–2
2000 .5016+1 1.928 .485–1 –.151–2 .1346+2 1.978 –.264–1 –.752–3 .1960+2 1.402 .264+0 .345–1 .3855+2 1.483 .270+0 .394–1 .1501+2 1.977 –.237–1 –.421–3 .2070+2 1.601 .576–1 .304–2
3000 .4678+1 1.919 .354+0 –.147–2 .1065+2 1.985 –.879–1 –.779–3 .1365+2 1.394 .542+0 .467–1 .2613+2 1.483 .570+0 .488–1 .9157+1 1.982 –.104+0 –.473–3 .1134+2 1.570 .248+0 .807–2
4000 .4372+1 1.910 .599+0 –.144–2 .8599+1 1.988 –.658–1 –.791–3 .9862+1 1.369 .766+0 .571–1 .1846+2 1.464 .813+0 .566–1 .6121+1 1.986 –.105+0 –.507–3 .6876+1 1.525 .448+0 .148–1
5000 .4092+1 1.901 .803+0 –.141–2 .7064+1 1.989 –.905–3 –.792–3 .7338+1 1.338 .953+0 .673–1 .1347+2 1.435 .102+1 .642–1 .4353+1 1.988 –.620–1 –.527–3 .4479+1 1.477 .633+0 .229–1
Xe, Z = 54 Shell 1s1/2 Eb = 34565 eV 2s1/2 Eb = 5452 eV 2 p1/2 Eb = 5106 eV 2 p3/2 Eb = 4785 eV 3s1/2 Eb = 1149 eV 3 p1/2 Eb = 1001 eV
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Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001
M. B. TRZHASKOVSKAYA, V. I. NEFEDOV, and V. G. YARZHEMSKY
Photoelectron Angular Distribution
TABLE. Subshell Photoionization Cross Sections and Angular Distribution Parameters for Atoms with 1 ≤ Z ≤ 54 See page 106 for Explanation of Tables Xe, Z = 54 (continued) Shell 3 p3/2 Eb = 939 eV 3d3/2 Eb = 689 eV 3d5/2 Eb = 676 eV 4s1/2 Eb = 213 eV 4 p1/2 Eb = 157 eV 4 p3/2 Eb = 147 eV 4d3/2 Eb = 69 eV 4d5/2 Eb = 67 eV 5s1/2 Eb = 23 eV 5 p1/2 Eb = 13 eV 5 p3/2 Eb = 12 eV
σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ σ β γ δ
100 .2545+3 0.838 .212+0 .111+0 .9035+3 0.452 –.676–1 –.814–2 .1378+4 0.491 –.688–1 –.905–2 .1312+3 1.960 .369+0 .226–3 .1292+3 0.509 –.115–1 .507–1 .3479+3 0.523 –.331–2 .472–1 .3331+3 −.600 –.147–1 .809–1 .5282+3 −.488 .162–1 .709–1 .8597+2 1.951 .191+0 .194–3 .4467+2 0.089 –.485–1 .208–1 .1090+3 0.172 –.490–1 .210–1
200 .2244+3 1.126 .278+0 .614–1 .6909+3 0.674 –.102+0 –.237–2 .1046+4 0.719 –.103+0 –.307–2 .9426+2 1.966 .383+0 .985–4 .1033+3 1.075 .200+0 .328–1 .2589+3 1.054 .178+0 .308–1 .4079+3 0.422 .901–1 .882–2 .6277+3 0.519 .901–1 .669–2 .4061+2 1.964 .267+0 .106–3 .2417+2 0.910 .117+0 .219–1 .5754+2 0.929 .113+0 .219–1
500 .1571+3 1.442 .116+0 .149–1 .3394+3 1.031 –.562–1 .242–1 .5065+3 1.056 –.488–1 .231–1 .4428+2 1.971 .321+0 –.672–4 .5432+2 1.533 .194+0 .572–2 .1222+3 1.513 .162+0 .513–2 .1853+3 1.141 –.298–1 .415–2 .2758+3 1.183 –.304–1 .434–2 .1205+2 1.972 .283+0 –.325–4 .9364+1 1.546 .202+0 .266–2 .1995+2 1.520 .170+0 .290–2
1000 .9378+2 1.597 –.261–1 .506–2 .1318+3 1.202 .135+0 .484–1 .1936+3 1.201 .148+0 .474–1 .1918+2 1.974 .177+0 –.194–3 .2409+2 1.671 .159–1 –.583–3 .5032+2 1.679 –.195–2 .745–3 .5471+2 1.335 .630–1 .240–1 .7976+2 1.335 .725–1 .235–1 .4102+1 1.975 .172+0 –.165–3 .3535+1 1.696 .240–1 –.128–2 .6996+1 1.697 .547–2 –.553–4
159
E (eV) 1500 .6043+2 1.643 –.144–1 .578–2 .6238+2 1.230 .325+0 .646–1 .9064+2 1.213 .337+0 .646–1 .1069+2 1.976 .622–1 –.269–3 .1313+2 1.688 –.205–1 –.114–2 .2637+2 1.715 –.273–1 .192–2 .2196+2 1.339 .231+0 .392–1 .3164+2 1.318 .242+0 .392–1 .2064+1 1.976 .635–1 –.246–3 .1793+1 1.709 –.227–1 –.155–2 .3417+1 1.731 –.297–1 .132–2
2000 .4126+2 1.654 .601–1 .787–2 .3359+2 1.213 .492+0 .790–1 .4842+2 1.186 .500+0 .803–1 .6812+1 1.978 –.179–1 –.322–3 .8078+1 1.675 .204–1 –.647–3 .1579+2 1.715 .228–1 .351–2 .1064+2 1.299 .394+0 .533–1 .1521+2 1.267 .404+0 .544–1 .1244+1 1.979 –.149–1 –.301–3 .1060+1 1.692 .127–1 –.117–2 .1968+1 1.729 .149–1 .284–2
3000 .2176+2 1.637 .267+0 .128–1 .1242+2 1.138 .754+0 .106+0 .1768+2 1.102 .754+0 .110+0 .3455+1 1.983 –.973–1 –.390–3 .3778+1 1.626 .187+0 .246–2 .7120+1 1.683 .205+0 .720–2 .3468+1 1.195 .664+0 .810–1 .4899+1 1.153 .667+0 .847–1 .5943+0 1.983 –.953–1 –.373–3 .4747+0 1.638 .175+0 .153–2 .8511+0 1.693 .193+0 .627–2
4000 .1284+2 1.599 .482+0 .185–1 .5635+1 1.052 .948+0 .133+0 .7949+1 1.014 .942+0 .139+0 .2075+1 1.986 –.105+0 –.435–3 .2090+1 1.569 .380+0 .772–2 .3840+1 1.636 .412+0 .118–1 .1462+1 1.093 .873+0 .109+0 .2048+1 1.049 .868+0 .115+0 .3458+0 1.986 –.105+0 –.420–3 .2566+0 1.579 .367+0 .660–2 .4489+0 1.644 .399+0 .108–1
5000 .8190+1 1.556 .681+0 .250–1 .2920+1 0.970 .110+1 .160+0 .4088+1 0.934 .109+1 .168+0 .1375+1 1.988 –.686–1 –.465–3 .1280+1 1.513 .565+0 .148–1 .2306+1 1.587 .610+0 .177–1 .7207+0 1.001 .104+1 .137+0 .1002+1 0.959 .103+1 .146+0 .2247+0 1.988 –.702–1 –.452–3 .1550+0 1.521 .552+0 .134–1 .2660+0 1.593 .597+0 .164–1
Atomic Data and Nuclear Data Tables, Vol. 77, No. 1, January 2001