Corrigendum to ‘Scintillation efficiency for low energy nuclear recoils in liquid xenon dark matter detectors’ [Astroparticle Physics 61 (2015) 56-61]

Astroparticle Physics 72 (2016) 109

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Corrigendum

Corrigendum to ‘Scintillation efficiency for low energy nuclear recoils in liquid xenon dark matter detectors’ [Astroparticle Physics 61 (2015) 56-61] Wei Mu a,∗, Xiaonu Xiong b, Xiangdong Ji a,b,c a b c

INPAC, Department of Physics, and Shanghai Key Lab for Particle Physics and Cosmology, Shanghai Jiao Tong University, Shanghai 200240, PR China Center for High-Energy Physics, Peking University, Beijing 100080, PR China Maryland Center for Fundamental Physics, University of Maryland, College Park, MD 20742, USA

The authors regret to point out a typo issue in Eq. (18) on page 60. The correction is as follow: Page 60, Section 4, Eq. (18) change

Leff (Enr ) = qnc (Enr ) × to

0.840 1.417 − 0.245 ln (1 + 4.822Enr ) −0.840 Enr



Leff (Enr ) = qnc (Enr ) ×

.



1.417 −

0.840 0.245 ln (1 + 4.822Enr ) . 0.840 Enr

The authors would like to apologise for any inconvenience caused.

∗

DOI of original article: 10.1016/j.astropartphys.2014.06.010 Corresponding author. Tel.: +8618317186663, Fax.: +862154741040. E-mail addresses: [email protected], [email protected] (W. Mu), [email protected] (X. Ji).

http://dx.doi.org/10.1016/j.astropartphys.2015.06.003 0927-6505/© 2015 Elsevier B.V. All rights reserved.