The titanosaurian dinosaur Atsinganosaurus velauciensis (Sauropoda) from the Upper Cretaceous of southern France: New material, phylogenetic affinities, and palaeobiogeographical implications

The titanosaurian dinosaur Atsinganosaurus velauciensis (Sauropoda) from the Upper Cretaceous of southern France: New material, phylogenetic affinities, and palaeobiogeographical implications

Accepted Manuscript The titanosaurian dinosaur Atsinganosaurus velauciensis (Sauropoda) from the Upper Cretaceous of southern France: New material, ph...

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Accepted Manuscript The titanosaurian dinosaur Atsinganosaurus velauciensis (Sauropoda) from the Upper Cretaceous of southern France: New material, phylogenetic affinities, and palaeobiogeographical implications Verónica Díez Díaz, Géraldine Garcia, Xabier Pereda Suberbiola, Benjamin JentgenCeschino, Koen Stein, Pascal Godefroit, Xavier Valentin PII:

S0195-6671(18)30042-9

DOI:

10.1016/j.cretres.2018.06.015

Reference:

YCRES 3908

To appear in:

Cretaceous Research

Received Date: 31 January 2018 Revised Date:

2 May 2018

Accepted Date: 20 June 2018

Please cite this article as: Díez Díaz, Veró., Garcia, Gé., Pereda Suberbiola, X., Jentgen-Ceschino, B., Stein, K., Godefroit, P., Valentin, X., The titanosaurian dinosaur Atsinganosaurus velauciensis (Sauropoda) from the Upper Cretaceous of southern France: New material, phylogenetic affinities, and palaeobiogeographical implications, Cretaceous Research (2018), doi: 10.1016/j.cretres.2018.06.015. This is a PDF file of an unedited manuscript that has been accepted for publication. As a service to our customers we are providing this early version of the manuscript. The manuscript will undergo copyediting, typesetting, and review of the resulting proof before it is published in its final form. Please note that during the production process errors may be discovered which could affect the content, and all legal disclaimers that apply to the journal pertain.

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ACCEPTED MANUSCRIPT The titanosaurian dinosaur Atsinganosaurus velauciensis (Sauropoda) from the

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Upper Cretaceous of southern France: new material, phylogenetic affinities, and

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palaeobiogeographical implications

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Verónica Díez Díaz 1,2, Géraldine Garcia 3, Xabier Pereda Suberbiola 4, Benjamin Jentgen-

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Ceschino 5,6, Koen Stein 5,7, Pascal Godefroit 7, and Xavier Valentin 3,8

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43, 10115 Berlin, Germany;

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Humboldt Universität, Berlin, Germany;

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Laboratoire de Paléontologie, Evolution, Paléoécosystèmes et Paléoprimatologie (PALEVOPRIM,

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Museum für Naturkunde, Leibniz-Institut für Evolutions-und Biodiversitätsforschung, Invalidenstraße

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UMR7262 CNRS INEE), Université de Poitiers, 6, rue Michel-Brunet, 86073 Poitiers cedex, France;

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Estratigrafía y Paleontología, Apartado 644, 48080 Bilbao, Spain;

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Earth System Science – AMGC, Vrije Universiteit Brussel, Pleinlaan 2, 1050 Brussels, Belgium;

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Evolution & Diversity Dynamics Lab, Liège University, Allée du six Août, 14, 4000 Liège, Belgium;

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Directorate ‘Earth and History of Life’, Royal Belgian Institute of Natural Sciences, 1000 Brussels,

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Belgium;

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Universidad del País Vasco/Euskal Herriko Unibertsitatea, Facultad de Ciencia y Tecnología, Dpto.

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Palaios Association, 86300 Valdivienne, France.

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Abstract

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New remains of the titanosaurian sauropod Atsinganosaurus velauciensis from its Upper

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Cretaceous type horizon and type locality in Velaux-La Bastide Neuve (Bouches-du-Rhône

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Department, Provence) in southern France are described. This locality is considered to be

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upper Campanian (Argiles et Grès à Reptiles Formation, Aix-en-Provence Basin). The new

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material consists of skull fragments, including a partial braincase, isolated teeth, elements of

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ACCEPTED MANUSCRIPT the axial skeleton (cervical, dorsal and caudal vertebrae, ribs), and appendicular bones

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(scapula, humeri, ulna, metacarpals, ilia, ischia, femur, tibia, metatarsal). Histological

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investigation shows that the analysed individuals were mature. The emended diagnosis of

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Atsinganosaurus velauciensis includes a pubic peduncle of the ilium with a posterior concave

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surface in its distal half, surrounded by two sharp ridges. Equations for predicting body mass

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and size in sauropods suggest a body size up to 12 meters and a body mass of at least 3.5-5

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tonnes for the largest individuals.

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A phylogenetic analysis including 29 sauropod taxa was performed, with the European

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titanosaurs Atsinganosaurus, Ampelosaurus, Lirainosaurus, Lohuecotitan, Paludititan (Late

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Cretaceous) and Normanniasaurus (Early Cretaceous) all scored in the same analysis for the

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first time. Atsinganosaurus and Ampelosaurus form a clade that is phylogenetically proximal to

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Lirainosaurus within Lithostrotia – a clade here named Lirainosaurinae nov. – whereas

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Lohuecotitan and Paludititan form a clade towards the base of Lithostrotia. Normanniasaurus

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is resolved outside Lithostrotia, but within Titanosauria. From a palaeobiogeographical

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perspective, the phylogenetic results suggest that European titanosaurs belong to at least

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three distinct lineages and that two lithostrotian lineages were present during the latest

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Cretaceous in the European archipelago.

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Key Words: Atsinganosaurus, Lirainosaurinae, Titanosauria, Late Cretaceous, France,

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palaeobiogeography

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INTRODUCTION

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Recent studies have shown that the biodiversity of European titanosaurian sauropods was

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quite high during the Late Cretaceous, especially between the Campanian and early

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Maastrichtian (see e.g. Díez Díaz et al., 2015, 2016; Fondevilla, 2017; Vila et al., 2012, 2016).

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ACCEPTED MANUSCRIPT Five titanosaurian taxa have been described in Europe so far: Lirainosaurus astibiae, from the

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upper Campanian of Laño and Chera, Spain (Sanz et al., 1999; Company et al., 2009; Díez Díaz

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et al., 2011, 2012a, 2013a, 2013b, 2015); Lohuecotitan pandafilandi, from the upper

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Campanian-lower Maastrichtian of Lo Hueco, Spain (Díez Díaz et al., 2016); Atsinganosaurus

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velauciensis, from the upper Campanian of Velaux-La Bastide Neuve, France (Garcia et al.,

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2010); Ampelosaurus atacis, from the lower Maastrichtian of Bellevue, France (Le Loeuff, 1995,

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2005); and Paludititan nalatzensis, from the lower Maastrichtian of Nǎlaţ-Vad, Romania (Csiki

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et al., 2010). However, their diversity was likely even higher:

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1) The status of Magyarosaurus, from the Maastrichtian of Romania, is still uncertain, and a revision of all the recovered material is needed (see Csiki et al., 2010).

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2) Numerous isolated or poorly preserved titanosaurian remains were found in the Upper Cretaceous of southeastern France and northeastern Spain during the second half of

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the 19th century and the 20th century. These remains were assigned to the species

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Titanosaurus indicus and Hypselosaurus priscus (Matheron, 1869; Depéret, 1899;

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Lapparent and Aguirre, 1956, 1957; Masriera and Ullastre, 1988), both now considered

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nomina dubia (Le Loeuff, 1993; Wilson and Upchurch, 2003). This material also needs a

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detailed revision.

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3) At several sites of Spain and southern France cranial, dental and appendicular elements representing more than one titanosaurian morphotype have been found

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(Vila et al., 2012; Díez Díaz et al., 2012b, 2014, 2015; Páramo et al., 2015a, b).

Thus, at least seven titanosaurian taxa have so far been identified from the Campanian-

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Maastrichtian of Europe. Detailed studies and comprehension of these last sauropod faunas,

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especially in the Ibero-Armorican Island, is of great importance for understanding dinosaur

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biodiversity in Europe, just before the Cretaceous-Palaeogene (K-Pg) event (see Csiki-Sava et

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al., 2015, Vila et al., 2016; Fondevilla et al., 2016) that led to the extinction of all non-avian

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dinosaurs.

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Atsinganosaurus velauciensis is represented by several partially articulated specimens, some of which were described by Garcia et al. (2010). In 2009 and 2012, renewed excavation

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campaigns at the Velaux-La Bastide Neuve locality (Provence, France) led to the recovery of

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more material (Figure 1). The specimens described in this publication derive from sequence 2

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(Cincotta et al., 2015), as do the holotype and referred specimens of this taxon described in

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Garcia et al. (2010). This sequence occurs in the Argiles et Grès à Reptiles Formation (Aix-en-

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Provence Basin), which is upper Campanian. Dinosaur specimens represent 38% of the

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vertebrate remains collected during the 2009 and 2012 campaigns in Velaux-La Bastide Neuve

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(Cincotta et al. 2015), with most of these representing titanosaurs. The vertebrate fauna is

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abundant and diversified including rhabdodontid dinosaurs (Matheronodon provincialis

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[Godefroit et al. 2017] and Rhabdodon priscus), ankylosaurian remains, theropod teeth, the

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ontogenetic cranial and postcranial elements of the eusuchian crocodyliform Allodaposuchus

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precedens (Martin et al. 2016) , pleurodiran and cryptodiran turtle shells, an azhdarchid

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pterosaur (Vullo et al. in press), hybodont shark teeth, and mawsoniid bones. Sequence 2

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constitutes a coarse-grained conglomeratic sandstone lens. The fossil material was transported

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over rather short distances and accumulated together within a river channel, in a fluvial

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environment (Cincotta et al., 2015).

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The discovery of abundant titanosaurian cranial and postcranial remains provides new

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information on the French titanosaur Atsinganosaurus velauciensis, thereby facilitating the

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emendation of its diagnosis, better definition of its morphological features, and more precise

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assessment of its phylogenetic affinities. This will, in turn, enhance our understanding of the

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palaeobiogeographical history of Late Cretaceous sauropod faunas.

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METHODOLOGY

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Taxonomic description We use “Romerian” terms (Wilson, 2006) for anatomical structures (e.g. “centrum”, not

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“corpus”) and their orientations (e.g. “anterior”, not “cranial’”). The landmark-based

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terminology for vertebral laminae (Wilson, 1999) and fossae (Wilson et al., 2011) is used in the

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discussion of vertebral anatomy and in Figures 3-5. For the identification of the caudal

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vertebrae we follow suggestions made by Díez Díaz et al. (2013a). All measurements are

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provided in Tables 1-5.

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For brevity and clarity, Atsinganosaurus velauciensis is mainly compared with

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European titanosaurian taxa: Ampelosaurus atacis from Bellevue (Aude, France; Le Loeuff,

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1995, 2005), Normanniasaurus genceyi from Le Havre (Normandy, France; Le Loeuff et al.,

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2013), Lirainosaurus astibiae from Laño (Condado de Treviño, Spain; Sanz et al., 1999; Díez

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Díaz et al., 2011, 2013a, b) and Chera (Valencia, Spain; Company et al., 2009; Díez Díaz et al.,

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2015), Lohuecotitan pandafilandi from Lo Hueco (Cuenca, Spain; Díez Díaz et al., 2016),

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Paludititan nalatzensis from Nǎlat-Vad (Haţeg Basin, Romania; Csiki et al., 2010), and the

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material from the Haţeg Basin (Romania) referred to Magyarosaurus dacus (Nopcsa, 1915;

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Huene, 1932) housed in the NHMUK. All the comparisons, except for Normanniasaurus genceyi

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and Paludititan nalatzensis, are based on first-hand observations by the senior author (VDD).

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However, several comparisons have been made with other titanosaurs on the basis of

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important anatomical and phylogenetically important features that will help to distinguish

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Atsinganosaurus and the other European taxa from other members within Titanosauria.

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Histological methods

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In order to determine the ontogenetic stage of the new specimens, we sampled humeri and

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femora housed in the collection in the Moulin Seigneurial of Velaux (MMS/VBN.09.126,

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MMS/VBN.09.A.018, and MMS/VBN.00.12 – see table 6). In addition, we also sampled two

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very long (± 200 cm) and slender bony elements (MMS/VBN.09.51a and b), hypothesized to be

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cervical ribs. The long bone specimens were core-sampled (diameter of 1 cm) at or near the

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mid-shaft in posterior or anterior position, according to the standardized core location, when

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possible (Stein and Sander 2009; Sander et al., 2011). A fragment of the rib was also sectioned

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longitudinally and transversely to look for tendon fibres. Most of the cores broke during the

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drilling process because of their low mineralization, but were glued and restored before thin

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sectioning. All thin sections were prepared using standard lapidary methods with a thickness of

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40 µm. Observations were made with an Olympus petrographic microscope, BX50F-3 model,

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equipped with 5x and 10x objectives. Pictures were taken with a Leica camera and processed

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in Leica Application suite.

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Phylogenetic analysis

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To establish the relationships of Atsinganosaurus, a phylogenetic analysis was performed using

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the data matrix proposed by Salgado et al. (2015). This data matrix was analyzed using TNT 1.1

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(Goloboff et al., 2008) to find the most parsimonious trees (MPTs). For the first time, all the

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European taxa were included in the same analysis: Sallam et al. (2018) scored all the European

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titanosaurs from the Campanian-Maastrichtian of Europe, but this is the first time that

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Normannaisaurus is also included in the analysis. We have scored from first hand the European

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titanosaurs Atsinganosaurus, Ampelosaurus, Lirainosaurus and Lohuecotitan, and

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Normanniasaurus and Paludititan from the literature. We have also scored the titanosauriform

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Malarguesaurus (González Riga et al., 2009) first-hand in order to enhance the resolution of

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the relationships of basal forms. We used a heuristic tree search performing 1000 replications

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of Wagner trees (using random addition sequences) followed by tree bisection reconnection

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(TBR) as swapping algorithm, saving 100 trees per replicate. All characters were treated as

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unordered and unweighted.

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ACCEPTED MANUSCRIPT Institutional Abbreviations: FAM, Fox-Amphoux-Métisson, Mairie de Fox-Amphoux (Fox-

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Amphoux Council), Fox-Amphoux, France; MCNA, Museo de Ciencias Naturales de

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Álava/Arabako Natur Zientzien Museoa, Vitoria-Gasteiz, Spain; MDE, Musée des Dinosaures,

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Espéraza, France; MMS/VBN, Musée Moulin Seigneurial /Velaux-La Bastide Neuve, Bouches-

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du-Rhône, France; NHMUK, Natural History Museum, London, United Kingdom; UP, Université

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de Poitiers, Vienne, France.

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Anatomical Abbreviations: acdl, anterior centrodiapophyseal lamina; acpl, anterior

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centroparapophyseal lamina; ADW, anterodorsal pterygoid wing; AVW, anteroventral

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ectopterygoid wing; Bo, basioccipital; Bs, basisphenoid; cpol, centropostzygapophyseal lamina;

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cprl, centroprezygapophyseal lamina; D, diapophysis; ICA, internal carotid artery; iped,

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ischiadic peduncle; Ls+Os, laterosphenoid-orbitosphenoid complex; NS, neural spine; PA,

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parapophysis; pcdl, posterior centrodiapophyseal lamina; pcpl, posterior centroparapophyseal

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lamina; PO, postzygapophysis; pocdf, postzygocentrodiapophyseal fossa; podl,

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postzygodiapophyseal lamina; posdf, postzygospinodiapophyseal fossa; posl, postspinal

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lamina; pped, pubic peduncle; PR, prootic; prdl, posterior centrodiapophyseal lamina; PRE,

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prezygapophysis; prsl, prespinal lamina; PVW, posteroventral quadrate wing; sdf,

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spinodiapophyseal fossa; spof, spinopostzygapophyseal fossa; spol, spinopostzygapophyseal

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lamina; sprf, spinoprezygapophyseal fossa; sprl, spinoprezygapophyseal lamina.

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SYSTEMATIC PALAEONTOLOGY

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Dinosauria Owen, 1842

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Saurischia Seeley, 1887

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Sauropoda Marsh, 1878

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ACCEPTED MANUSCRIPT Titanosauriformes Salgado, Coria and Calvo, 1997

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Titanosauria Bonaparte and Coria, 1993

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Lithostrotia Upchurch, Barrett and Dodson, 2004

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Lirainosaurinae new taxon

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Etymology. After the Spanish titanosaur Lirainosaurus astibiae.

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Definition. Lirainosaurinae is phylogenetically defined as Lirainosaurus astibiae, Ampelosaurus

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atacis, their common ancestor, and all of its descendants.

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Atsinganosaurus velauciensis Garcia, Amico, Fournier, Thouand and Valentin, 2010

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Holotype. UP/VBN.93.01.a–d: four articulated posterior dorsal vertebrae, housed in the

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collections of the Université de Poitiers, France.

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Referred specimens. Université de Poitiers, France: UP/VBN.93.12a–c: three cervical vertebrae;

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UP/VBN.93.11: scapula; UP/VBN.93.10: metatarsal; UP/VBN.93.03-08: caudal vertebrae.

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Musée Moulin Seigneurial /Velaux-La Bastide Neuve, France: MMS/VBN.02.03, 22 and 53:

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teeth; MMS/VBN.02.78a–b: scapulocoracoid; MMS/VBN.02.99: isolated dorsal vertebra;

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MMS/VBN.02.82: sacrum; MMS/VBN.02.109: tibia; MMS/VBN.02.110: caudal vertebra.

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Musée Moulin Seigneurial /Velaux-La Bastide Neuve, France: MMS/VBN.00.12: humerus;

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MMS/VBN.00.01-03: three caudal vertebrae.

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ACCEPTED MANUSCRIPT Muséum d’Histoire Naturelle d’Aix-en-Provence, France (donated by X. Valentin):

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VBN.93.MHNA.99.21: tooth; VBN.93.MHNA.99.52: humerus; VBN.93.MHNA.99.32-34: caudal

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vertebrae.

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Type locality. La Bastide Neuve, Velaux; Aix-en-Provence Basin, Bouches-du-Rhône, France

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(Figure 1A).

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Type horizon. ‘Begudian’ (local stage) sandstones, upper Campanian, Upper Cretaceous (Garcia

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et al. 2010, Cincotta et al., 2015).

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Newly referred material. MMS/VBN.09.41: occipital condyle; MMS/VBN.09.167: braincase

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fragment; MMS/VBN.09.158a: left pterygoid; MMS/VBN.93.33, MMS/VBN.12.A.006,

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MMS/VBN.12.A.007, and MMS/VBN.12.B.014: four teeth; UP/VBN.93.13a and b,

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MMS/VBN.09.D.007a, MMS/VBN.12.A.004, MMS/VBN.12.B.010, MMS/VBN.12.B.015: six

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cervical vertebrae; UP/VBN.93.02, MMS/VBN.93.32, UP/VBN.09.157: three dorsal vertebrae;

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MMS/VBN.93.31a, MMS/VBN.93.32b, MMS/VBN.00.14, MMS/VBN.00.15, MMS.VBN.09.46,

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MMS/VBN.09.54, MMS/VBN.09.159b, MMS/VBN.09.D.003, MMS/VBN.09.D.009,

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MMS/VBN.09.D.010, MMS/VBN.09.D.011, MMS/VBN.12.33, MMS/VBN.12.B.013a,

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MMS.VBN.12.B.013b, MMS/VBN.12.B.018, MMS/VBN.12.C.003, MMS/VBN.12.C.004:

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seventeen caudal vertebrae; MMS/VBN. 93.31b and MMS/VBN.93.32b: two haemal arches;

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MMS/VBN.09.51a and b: two cervical ribs; MMS/VBN.09.D.07b and MMS/VBN.09.D.007c: two

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dorsal ribs; MMS/VBN.09.66: sacral rib; MMS/VBN.09.124D: scapula; MMS/VBN.09.A.018: left

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humerus; MMS/VBN.12.P.06a: right ulna; MMS/VBN.09.D.001: radius; MMS/VBN.09.113,

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UP/VBN.93.09: two metacarpals; MMS/VBN.12.32: ilion; MMS/VBN.09.51c: right ischium;

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MMS/VBN.09.126: right femur; MMS/VBN.02.90: left tibia; MMS/VBN.09.132: fibula.

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The fossil material is labelled and housed in the municipality palaeontological and

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archaeological structures of Velaux, under the care of the research association Palaios, and is

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property of the department CD (Conseil Départemental) 13.

216 Emended diagnosis. Pubic peduncle of the ilium with a posterior concave surface in its distal

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half, surrounded by two sharp ridges. Recovered local autapomorphies from the phylogenetic

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analysis: i) anterior and middle cervical vertebrae without pleurocoels (character #22), ii) ratio

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between the anteroposterior length/height of posterior face of the posterior cervical

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vertebrae higher than 3 (character #29), and iii) prominent ulnar olecraneon process,

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projecting above the proximal articulation (character #61). None of the features of the former

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diagnosis from Garcia et al. (2010) can longer be regarded as diagnostic for Atsinganosaurus

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velauciensis.

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225 DESCRIPTION

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Skull

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Three skull fragments (Fig. 2) have been unearthed: an occipital condyle (MMS/VBN.09.41), a

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right portion of the braincase (MMS/VBN.09.167), and a probable left pterygoid

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(MMS/VBN.09.158a)

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Occipital condyle. MMS/VBN.09.41 (Figure 2E) is a robust occipital condyle with a rounded

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outline. The neck is not preserved, and the foramen for the hypoglossal nerve (XII) can only be

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seen on the right side in dorsolateral view. It is a single opening, as seen in most titanosaurian

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taxa (Paulina Carabajal, 2012; Poropat et al., 2016).

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Braincase. MMS/VBN.09.167 seems to be a right fragment of a braincase, with portions of the

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basioccipital, basisphenoid, prootic, and laterosphenoid (Figure 2A and B). However, this is a

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bones – and all the foramina for the cranial nerves and fenestrae are collapsed. However,

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some structures can be identified: grooves for the trigeminal (V) and facial (VII) nerves, and the

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crista prootica in lateral view; the channel for the internal carotid artery in the basisphenoid;

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and several grooves along the medial surface of the prootic, probably related with brain or

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cranial nerve structures. The grooves for cranial nerves V and VII more closely resemble those

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on the partial braincase MCNA 7439, referred to Lirainosaurus (Díez Díaz et al., 2011), than

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those observed on the specimen FAM 03.064 from Fox-Amphoux-Métisson referred to

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Titanosauria indet. (Díez Díaz et al., 2012b). Besides this, no more detailed comparisons can be

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made due to the poor preservation of the specimen from Velaux.

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Pterygoid. MMS/VBN.09.158a is a fragmentary skull bone that probably belongs to a left

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pterygoid (Figure 2C and D). It is a flat triradiate element, the ends of which are not completely

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preserved. Pterygoids have only been described in the titanosaurs Nemegtosaurus (Nowinski,

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1971), Quaesitosaurus (Kurzanov and Bannikov, 1983), Rapetosaurus (Curry Rogers and

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Forster, 2004), Tapuiasaurus (Zaher et al., 2011, Wilson et al., 2016), and Sarmientosaurus

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(Martínez et al., 2016). MMS/VBN.09.158a shares its general morphology with them, like its

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plate-like morphology (with its three processes coplanar), that seems to be a diagnostic

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character within Titanosauria (Poropat et al., 2016). The lateral surface of MMS/VBN.09.158a

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is slightly convex, and the medial one is flat. The anterodorsal pterygoid wing is the longest of

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the three wings because of its preservation. It narrows distally, and forms an angle of 90° with

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the anteroventral ectopterygoid wing. The anteroventral ectopterygoid wing becomes more

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robust towards its distal end, forming an anterior bulge for the contact with the ectopterygoid.

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In lateral view, at the junction between the three wings, a broken surface probably

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corresponds to the lateral depression for contact with the palatine. The posteroventral

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quadrate wing is not complete and poorly preserved. It forms an angle of ca. 130° with the

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anterodorsal wing. Laterally, a shallow depression on the posteroventral quadrate wing marks

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the contact with the quadrate. No pterygoid remains have been described in other European

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titanosaurians so far.

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Teeth

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Four new teeth have been found (MMS/VBN.12.A.006 and 07, MMS/VBN.12.B.014 and

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MMS/VBN.93.33) (Figure 2F, Table 1). They are similar to those previously described in

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Atsinganosaurus (see Garcia et al., 2010 and Díez Díaz et al., 2013c). They are peg-like, with

269

cylindrical crowns and a tapered tip. The lingual surface is flat, and the labial one convex. The

270

apex is slightly inclined lingually. An apical wear facet is present, with and angle of 60° in

271

relation with the apicobasal axis of the crown. This angle is similar to the ones calculated for

272

most of the titanosaurian teeth found in the Ibero-Armorican Island (see Díez Díaz et al. 2012a,

273

b, 2014). The enamel is smooth, with smooth longitudinal lines. The mesial and distal ridges

274

are more prominent in the distal third of the crown. There are no denticles or carinae present.

275

They clearly differ from other titanosaurian teeth described from the Ibero-Armorican Island

276

(see Díez Díaz et al. 2013c and 2014 for a more detailed comparison). These new teeth have a

277

similar SI (SI mean of the sample: 4.49) as the other teeth ascribed to Atsinganosaurus (SI

278

mean: 4.15; see Díez Díaz et al., 2013c). MMS/VBN.12.A.006 has a more slender and slightly

279

more labiolingually compressed crown than the other preserved teeth of Atsinganosaurus.

280

Cervical vertebrae

281

Six cervical vertebrae have been recovered, belonging to the anterior, middle and posterior

282

sections of the neck. All of them display the same general morphology as those originally

283

described by Garcia et al. (2010) (Figure 3A-C and E, Table 2). The centra are opisthocoelous,

284

with camellate internal texture, characteristic for Titanosauriformes (Upchurch, 1998; Wilson,

285

2002; Wedel, 2003; Upchurch et al., 2004; D'Emic, 2012). The prezygapophyses extend

286

anterior to the anterior tip of the condyle, contrary to some derived lithostrotians (Poropat et

287

al., 2016). Analyzing the changes on the EI we can elucidate a pattern in the cervical series: the

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centra shorten their length through the anterior to middle cervicals, becoming longer again in

289

the posterior ones, being even more transversally compressed than the first ones (although

290

this could be also due to preservation).

291

Anterior cervical vertebra. MMS/VBN.12.A.004, MMS/VBN.12.B.015 and MMS/VBN.09.D.007a

292

(this one found associated with two dorsal ribs) are anterior cervical vertebrae (Figure 3D, F

293

and G). The first one is the best preserved, but the main features are shared by all elements.

294

The left side of MMS/VBN.12.A.004 (Figure 3G) misses the tuberculum of the cervical rib, but

295

this structure is preserved in the right side of the specimen, together with a fragment of the

296

cervical rib (see below for a more detailed description). The centrum is long and has a sub-

297

quadrangular cross-section, especially its posterior half. The posterior ventral surface is flat,

298

whereas the anterior one is concave. The lateral surfaces, which are flat posteriorly and

299

concave anteriorly, do not present pneumatic foramina, contrary to Lohuecotitan (Díez Díaz et

300

al., 2016) and Magyarosaurus (NHMUK R. 4898). None of the specimens preserve the

301

postzygapophyses. The diapophyses and parapophyses are located on the anterior half of the

302

centrum. The parapophysis is located below the centrum. The dorsal surface of the

303

parapophysis is not excavated, but a shallow fossa is present on the lateral surface of the

304

centrum, above the parapophysis, in MMS/VBN.12.B.010 (Fig. 4C and C’). The prezygapophysis

305

is wide and robust, anterodorsally directed, and does not diverge too much from the centrum.

306

The neural spine is not completely preserved in any of them; it seems to be a single, laterally

307

compressed structure with a simple lamination. The lamination is the same that presumably

308

can be found in most sauropod cervical vertebrae: acpl, pcpl, pcdl, prdl in the centra, and podl,

309

sprl and spol in the spine. No acdl, prsl or posl are present. The fossae between these laminae

310

are very shallow with the exception of the spof, which is narrow and deep.

311

Middle to posterior cervical vertebrae. UP/VBN.93.13a and b were found in anatomical

312

connection. Because they are still embedded in the matrix, most of the structures on their

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right side cannot be seen. Both present the same general morphology, also together with the

314

anterior cervicals, but these are smaller and more slender. The cross-section of the centra is

315

more circular. The ventral surfaces of the centra are concave anteriorly and flat posteriorly, as

316

in Ampelosaurus. The diapophyses and parapophyses are better developed laterally, and the

317

parapophyses are slightly ventrally placed with respect to the centra. Both are still located on

318

the anterior half of the centra. The tubercula and capitula are preserved, but not the cervical

319

ribs. The prezygapophyses are only preserved in UP/VBN.93.13b; they are short and wide, and

320

directed anterodorsally. The postzygapophyses are broad, teardrop-shaped structures, whose

321

articulations are directed ventrally and slightly laterally. The single neural spines are higher,

322

and have a triangular outline in lateral view. There is a rugose thickening in the distal half of

323

the neural spine, maybe for tendinous attachment. The laminae and fossae complexes are

324

more developed than on the anterior cervicals: besides the laminae also present in the

325

anterior cervicals, the single cprl and cpol can be seen, together with an accessory lamina that

326

divides vertically a shallow posterior fossa below the pcdl. Shallow fossae are developed on

327

the dorsal surfaces of the parapophyses and below the diapophyses; on the lateral surfaces of

328

the centra, two additional fossae (anterior and posterior – the latter divided by an accessory

329

lamina) are present. The fossae on the neural spines are deeper than in the other European

330

titanosaurs (but not like the ones present in the Argentinean taxon Mendozasaurus, that are

331

even delimited by sharp-lipped laminae [González Riga et al., 2018]), like the triangular pocdf

332

between the pcdl and the podl, the sdf above the podl, and the spof.

333

Posterior cervical vertebra. Garcia et al. (2010) described three posterior cervical vertebrae:

334

UP/VBN.93.12a–c . Besides the new cervical found, we figure these three vertebrae again,

335

detailing the lamina and fossae complexes (Figure 3A-C and E). The new posterior cervical,

336

MMS/VBN.12.B.010 (Figure 4), is the smallest of the sample and the most posterior one, as

337

indicated by its shorter and lower centrum and its higher neural spine. In general terms, this

338

vertebra presents the same features as the other five cervicals. Although there is some

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340

ventral face of the centrum is also anteriorly concave and posteriorly flat. The ribs are missing,

341

but the diapophyses and parapophyses are preserved and ventrally directed. In this specimen,

342

the parapophyses are more anteriorly located on the centrum than the diapophyses, which are

343

located in the middle part of the centrum. The prezygapophyses are not well-preserved, but it

344

can be inferred that they were more anterodorsally directed than on the anterior cervicals.

345

Only the right postzygapophysis is preserved and dorsolaterally directed. There is also a rugose

346

thickening on the distal half of the neural spine, directed posterodorsally from the

347

postzygapophysis. The laminae are thicker than in the other cervicals, and the fossae are

348

slightly shallower than on the middle to posterior cervicals, with the exception of the lateral

349

pneumatic foramina, which are better developed on this vertebra. The posterior cervical

350

vertebra MDE C3-265, referred to Ampelosaurus, also has lateral pneumatic foramina. In

351

addition, the anterior side of the neural spine of MMS/VBN.12 B.010 has two sprls that define

352

a deep and narrow sprf between themselves. The posterior spof is similarly deep and narrow,

353

delimited by the spols. Ampelosaurus (MDE C3-265) also possesses a deep spof; however, this

354

fossa is much wider than in Atsinganosaurus, as is its neural spine overall. The cervicals of

355

Ampelosaurus also present a prsl (Le Loeuff, 2005).

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The conservative pattern of the lamina and fossa complexes within the cervical series is noteworthy. This pattern is not present on the dorsal and sacral vertebrae, and different

358

patterns may occur in the same (right and left features) or in different individuals. This also

359

occurs in the vertebrae of Atsinganosaurus described by Garcia et al. (2010), and in the

360

titanosauriform Giraffatitan brancai (Wedel and Taylor, 2013; VDD pers. obs.).

361

Cervical ribs

362

A fragmentary cervical rib, probably a right one, is associated with MMS/VBN.12 A.004 (Figure

363

3G). The preserved fragment is slender, with the same width along most of its length (ca. 1.6

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cm). The lateral face is flat. However, we cannot infer the section of the specimen because it is

365

still hidden in the rock matrix. The preserved length is ca. 30 cm.

366

Dorsal vertebrae

367

None of the new dorsal vertebrae are completely preserved, but they closely resemble those

368

already described by Garcia et al. (2010) (see also Díez Díaz et al., 2013a, fig. 9C for the

369

laminae and fossae complexes and the comparison of UP/VBN.93.01b with other European

370

titanosaurs) (Figure 5A-C; Table 2). MMS/VBN.93.32 (Figure 5A) is an anterior neural arch

371

lacking the spine, UP/VBN.09.157 (Figure 5B) is a poorly preserved centrum with the base of

372

the neural arch, and UP/VBN.93.02 (Figure 5C) is a fragment of the left half of a middle to

373

posterior dorsal (in which the neural canal is not clearly visible, as it is obliterated). The dorsal

374

centra are opisthocoelous, with lateral eyed-shaped pleurocoels (set within a fossa), as in

375

other European titanosaurian taxa except Paludititan (Csiki et al., 2010; Díez Díaz et al., 2013a,

376

fig. 9). UP/VBN.09.157 likely had a ventral keel, unlike other European taxa. The inner

377

structure of the centra cannot be observed in any of the specimens, although the camellate

378

internal tissue is present in the anterior neural arch MMS/VBN.93.32. In this latter specimen,

379

the prezygapophyses are short and directed anterodorsally, but its posterior surface is

380

completely eroded. The neural canal is small and circular. The prezygapophyses are better

381

developed and laterally directed in Lirainosaurus (MCNA 7445; Díez Díaz et al., 2013a).

382

Although their distal ends are missing, the diapophyses are oriented dorsolaterally. Some

383

laminae can be seen in this specimen: single cprl, the base of the left sprl, pcdl, and podl. The

384

left pocdf and posdf are deep. The main difference between this specimen and Lirainosaurus

385

(MCNA 7445) is the presence of an acdl in the latter. In UP/VBN.93.02, the diapophyses appear

386

to be better developed and more robust. The postzygapophyses are small and their articular

387

surfaces face ventrally. The cpols are single, slender and vertical laminae. A pocdf is also

388

developed between the pcdl, the cpol, and the broken podl, and the posdf is shallower. In this

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specimen, only the base of the neural spine is preserved. In UP/VBN.09.157, a different lamina

390

pattern can be seen: together with the pcdl, an acdl is present and between them a triangular

391

fossa is present. In addition, as no matrix is present between the cpol and the pcdl, we observe

392

that the pocdf was so deep that it reached the inner structure of the neural arch, confirming

393

that these dorsal vertebrae were highly pneumatized. These lamina and fossa complexes are

394

also present in a posterior dorsal of Ampelosaurus (MDE C3-247). As in UP/VBN.93.02, the

395

posterior dorsals of Lirainosaurus are devoid of an acdl. However, the lateral pneumatic

396

foramina of this Iberian titanosaur are smaller. The main differences with the dorsal vertebrae

397

of Lohuecotitan are found on the ventral surface of the centrum, the laminae and fossae

398

complexes, and the development of the diapophyses (Díez Díaz et al., 2016, fig. 2. C-E).

399

Paludititan does not present a podl, but in general, its laminae and fossae complexes are more

400

complex than those of Atsinganosaurus.

401

Dorsal and sacral ribs

402

Two dorsal ribs (Figure 5D-G) were found associated with the anterior cervical vertebra

403

MMS/VBN.09.D.07a. They are flat (plank-like) and slender, although an important level of

404

crushing should be taken into account. One of them (the longest one: MMS/VBN.07.D.07b,

405

preserved length 58.5 cm) shows part of its tuberculum and capitulum separated by a

406

concavity. The preserved length of the other (MMS/VBN.09.D.007c) is 56 cm. No evidences on

407

pneumaticity can be assessed because of their preservation.

408

Only one fragmentary sacral rib (MMS/VBN.09.66) was recovered. It is probably one of first

409

ones from the left side, because of the development of a transverse foramen. In the sacrum

410

described by García et al. (2010), only the first three preserved sacrals present a transverse

411

foramen between the centra and the ribs. This element is anteroposteriorly compressed and

412

its acetabular arm is not completely preserved. Both costovertebral junctions with the

413

diapophysis and the parapophysis are preserved, although their ends are broken off. The

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capitulum is more slender than the tuberculum, which is bifurcated distally. The area between

415

the tuberculum and the capitulum (the transverse foramen sensu Wilson, 2011) is highly

416

concave.

417

Sacrum

418

The sacrum MMS/VBN.02.82 (Figure 6) was already described by Garcia et al. (2010), so here

419

we will point out some details that are not present in the former work.The ventral surfaces of

420

the sacral vertebrae present a ventral keel (Figure 6C). This sacrum is a robust and well-fused

421

specimen, as stated by huge fusion of the centra and neural spines, but also the presence of

422

thickened flat dorsal surfaces in the tuberculum of the sacral ribs. These surfaces are well-

423

differentiated from the rest of the sacral rib (Figure 6A and D). The laminae and fossae

424

complexes do not have the same patterns through all the sacral series, and are not even

425

symmetrical. A supraspinous rod (Figure 6A) runs distally through all the neural spines, as seen

426

in many other derived sauropods (see e.g. Cerda et al., 2015, fig. 7). Indeed, this rod could be a

427

diagnostic feature within Titanosauria (Poropat et al., 2016).

428

Caudal vertebrae

429

Seventeen new caudal vertebrae have been recovered (Figures 7 and 8, Table 2). All of them

430

are procoelous (with some exceptions in the posterior caudal vertebrae, that become slightly

431

amphicelous, like in MMS/VBN.93.32a [Figure 7V-X], UP/VBN.93.03 and UP/VBN.93.04 [Figure

432

8F-G]), a condition typically found in Lithostrotia (e.g. Salgado et al., 1997; Upchurch et al.,

433

2004; D’Emic, 2012). The presence of non-procoelous posterior caudal vertebrae

434

(amphicoelous, opisthocoelous and biconvex) has been found in other lithostrotian

435

titanosaurs, like Rinconsaurus caudamirus (Calvo and González Riga, 2003; VDD, pers. obs.) or

436

Opisthocoelicaudia skarzynskii (Borsuk-Białynicka, 1977). Their neural arches are placed

437

anteriorly on their centra, as in Titanosauriformes (e.g. Salgado et al., 1997; Wilson, 2002;

438

Upchurch et al., 2004), and are vertically oriented as in most lithostrotians (Carballido et al.,

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440

(Upchurch et al., 2004, Carballido et al., 2011).

441

Anterior caudal vertebrae. Six anterior caudal vertebrae are preserved (MMS/VBN.93.31a

442

[Figure 7J-K], MMS/VBN.00.14 [Figure 7A-E], MMS/VBN.00.15 [Figure 7F-I], MMS.VBN.09.46,

443

MMS/VBN.09.54 [Figure 8B], MMS/VBN.12.C.004 [Figure 8A]). The broken surfaces of

444

MMS/VBN.09.54 allow observation of the camellate internal tissue of the centrum. None of

445

them have transverse processes, instead possessing lateral bulges located dorsally on the

446

centrum, close to the junction with the neural arch. This, together with the simple neural

447

spine, indicates a relatively more posterior position along the anterior caudal series, probably

448

close to the middle section of the tail. The centra are strongly procoelous with a well-

449

developed condyle, which is not constricted unlike in Lirainosaurus (Díez Díaz et al., 2013a) and

450

Lohuecotitan (Díez Díaz et al., 2016). In addition, this condyle is located in the middle of the

451

posterior articulation, which is not the case in Normanniasaurus and Paludititan, whose

452

condyles are dorsally displaced on the centra. The centrum of MMS/VBN.12 B.004 is sub-

453

quadrangular in cross-section, as in the caudal vertebrae found in Chera (Spain) and referred

454

to an indeterminate titanosaurian distinct from Lirainosaurus (see Díez Díaz et al., 2015), but

455

unlike other European titanosaurs. However, it is important to highlight that this is the only

456

similarity with the caudals of the second taxon from Chera. Longitudinal ridges are present in

457

the most anterior caudals (Figure 7D and H), and become less developed in the next ones in

458

the series. No longitudinal ridges or midline grooves are developed along the ventral face of

459

the posterior anterior centra (Figure 7Q), this is also the case in Lirainosaurus. The articular

460

surface for the the haemal arches is poorly preserved. MMS/VBN.12 B.004 lacks the right

461

prezygapophysis and the neural spine. The prezygapophyses of both specimens are directed

462

slightly anterodorsally, and the one of MMS/VBN.09.54 is broader. The neural spine is an

463

anteroposteriorly short, transversely-compressed, and slightly posterodorsally-directed

464

lamina. It is proportionally lower than the neural spines of the anterior caudals of

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466

The postzygapophyses are triangular surfaces located posteriorly on the neural spine. They

467

closely resemble those described by Garcia et al. (2010). We consider that MMS/VBN.02.110 is

468

an anterior caudal because of the presence of transverse processes.

469

Anterior to middle caudal vertebrae. Three fragmentary middle caudals have been recovered:

470

MMS/VBN.09.D.009, MMS/VBN.09.D.011, MMS/VBN.12.B.018. Their morphology (procoelous

471

centra, low neural arches, and long and horizontal prezygapophyses) is not particularly

472

noteworthy within Titanosauria. Their ventral surfaces do not present any longitudinal ridges

473

or midline grooves, like in the anterior caudal vertebrae.

474

Posterior caudal vertebrae. Eight posterior caudal vertebrae have been found:

475

MMS/VBN.93.32a (Figure 7V-X), MMS/VBN.09.159.b (Figure 8E), MMS/VBN.09.D.003 (Figure

476

7R-U), MMS/VBN.09.D.010, MMS/VBN.12.B.013a, MMS/VBN.12.B.013b, MMS/VBN.12.C.003

477

(Figure 8C), MMS/VBN.12.33. Only MMS/VBN.12 B.013a and b were found associated. These

478

vertebrae are procoelous (with some exceptions, as seen above), unlike the shorter and

479

amphiplatyan centra on the posterior caudals of Paludititan. Their condyle is less developed

480

than on the anterior caudals, unlike in Lirainosaurus and Lohuecotitan, in which the posterior

481

caudals still have a constricted condyle located slightly dorsally on the posterior articular

482

surface of the centra (Díez Díaz et al., 2013a, fig. 6; Díez Díaz et al., 2016, fig. 3). The centra are

483

longer than the anterior caudals, but shorter dorsoventrally. The ventral surface of

484

MMS/VBN.09.159b is flat, and its articular surface for the haemal arches is prominent as in

485

Lohuecotitan (Díez Díaz et al., 2016). A ridge marks the junction between the neural arch and

486

the centrum, as also observed on the middle and posterior caudal vertebrae of Alamosaurus

487

(Gilmore, 1946), Ampelosaurus (Le Loeuff, 2005), Andesaurus (Mannion and Calvo, 2011),

488

Baurutitan (Kellner et al., 2005), Narambuenatitan (Filippi et al., 2011), and Normanniasaurus

489

(Le Loeuff et al., 2013). The neural spine is only preserved in MMS/VBN.12 B.013a; it is a

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491

caudals. In the other posterior caudals, the neural arch is incipient. The prezygapophyses are

492

long and slender, and almost horizontal. The postzygapophyses are located on the

493

posterodorsal tip of the neural spine, forming a triangular articular surface. These vertebrae

494

are different from the posterior caudals described by Garcia et al. (2010). However, because of

495

its dorsoventral compression and the presence of articulations for the haemal arches,

496

VBN.93.MHNA.99.33 is probably a middle to posterior caudal vertebra. We consider

497

MMS/VBN.93.3-8, described by Garcia et al. (2010), as distal caudal vertebrae because of their

498

typical spool-like morphology and the absence of neural arches. These six caudals were found

499

almost articulated.

500

Haemal arches

501

MMS/VBN.93.31b (Figure 7L-M) and MMS/VBN.93.32b (Figure 8Y-Z) are two haemal arches

502

found associated with the caudal vertebrae MMS/VBN.93.31a and MMS/VBN.93.32a

503

respectively. Both are open Y-shaped, as in most macronarians (Wilson, 2002; Curry Rogers,

504

2005; Mannion and Calvo, 2011; Otero et al., 2012). The haemal canal does not reach the

505

middle of the total length of both arches, contrary to the ones referred to Paludititan. The

506

distal blades are transverselly flattened distally, contrary to Lirainosaurus. Although the

507

proximal articular faces are not completely preserved it is visible that they are not divided in

508

two articular faces, as the ones of Lohuecotitan.

509

Pectoral girdle

510

Scapula. Besides the fragmentary scapulocoracoid (MMS/VBN.02.78a–b, Figure 9A-B) and the

511

scapula (MMS/VBN.93.11, Figure 9C), previously described by Garcia et al. (2010), another

512

fragmentary right scapula (Figure 9D) has been found, which likely belonged to a juvenile

513

individual (MMS/VBN.09.124D). It consists of the proximal third of the scapular blade and part

514

of the acromial blade. Its medial surface is concave (no ridges or prominences present),

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whereas its lateral side is convex, with a rounded and longitudinal ventral ridge. No triangular

516

processes on the ventral margin are present.

517

Forelimb

518

Humerus. MMS/VBN.00.12 (Figure 10A-D) is a right humerus, and MMS/VBN.09.A.018 (Figure

519

10E-H, Table 3) a left one This second one has poorly preserved proximal and distal edges and

520

deltopectoral crest. Their diaphyses are slender and anteroposteriorly compressed. The

521

posterior surface is convex, and the anterior one concave. No bulges or tuberosities are

522

present in the posterior surface of the proximal third of MMS/VBN.09.A.018, contrary to

523

MMS/VBN.00.12, which presents a tuberosity close to the lateral margin of the posterior

524

surface, at approximately the level of the distal tip of the deltopectoral crest. This tuberosity

525

was probably for the insertion of m. latissimus dorsi (Borsuk-Bialynicka, 1977; Otero, 2010;

526

D’Emic, 2012) No other prominences or ridges are visible or present in the anterior and

527

posterior surfaces of these specimens. The distal edge of the deltopectoral crest is located

528

above the middle of the diaphysis, as in Lirainosaurus, Ampelosaurus, and Magyarosaurus (Le

529

Loeuff, 2005; Díez Díaz et al. 2013b; VDD pers. obs.). The deltopectoral crest doubles its

530

thickness distally, and it is slightly deflected medially. The diaphysis of this specimen seems

531

more slender than in other European titanosaurs. A more detailed comparison is not possible

532

due to the preservation of the proximal and distal ends of the specimen. However, the

533

slenderness of the diaphysis (ECC [eccentricity index, sensu Wilson and Carrano, 1999]: 3.76)

534

and the relative development and position of the deltopectoral crest resemble the condition in

535

MMS/VBN.00.12 (ECC: 3.14), described by Garcia et al. (2010) as belonging to Atsinganosaurus

536

(figure 6A). VBN.93.MHNA.99.52 is a fragmentary right humerus (Figure 10I-J) that was not

537

described by Garcia et al. (2010). The anterior surface is not well-preserved, the proximal end

538

is eroded and the distal extremity is lost. The posterior surface is better preserved, but no

539

special features can be seen.

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Ulna. MMS.VBN.12.P.06a is a slender right ulna (Figure 10K-P), Table 3), with a broad proximal

541

end. This end has a triradiate outline (forming an angle of almost 90° between the longest

542

arms, which are not completely preserved), although its articular surface is not preserved. The

543

posterior process is well-developed. The olecranon process is better developed than in

544

Lirainosaurus and the ulna C3-1296 of Ampelosaurus, more closely resembling the condition in

545

C3-1490. The well-developed proximal processes delimit three shallow surfaces that extend

546

along the diaphysis up to the distal extremity, which is only slightly expanded and not

547

completely preserved (the presence of an anteromedial fossa for the reception of the radius

548

cannot be assessed).

549

Radius. MMS/VBN.09.D.001 (Figure 10Q-R) is a fragmentary diaphysis of a radius, and has a

550

cylindrical cross-section. No more features can be described due to its poor preservation.

551

Metacarpals. Only two metacarpals I (MMS/VBN.09.113 and UP/VBN.93.09) have been

552

recovered (Figure 11, Table 4); the second specimen is much smaller, likely belonging to an

553

immature individual. Both specimens are poorly preserved, and their proximal and distal ends

554

are missing. MMS/VBN.09.113 was probably a left metacarpal, as suggested by the position of

555

its articular surface for metacarpal II. The diaphyses are long and anteroposteriorly

556

compressed, as in Bonatitan (Salgado et al., 2015) and Rapetosaurus (Curry Rogers, 2009),

557

contrasting with the metacarpals of Magyarosaurus, which have a more rounded cross-

558

section. Metacarpal I of Epachthosaurus (Martínez et al., 2004) is more robust, and its

559

diaphysis is not compressed. The diaphyses are straight, as in the derived titanosaurs

560

Bonatitan, Epachthosaurus, Rapetosaurus, and Opisthocoelicaudiinae (Apesteguía, 2005) and

561

unlike the bowed morphology in the basal taxa Andesaurus (Mannion and Calvo, 2011),

562

Antarctosaurus (Huene, 1929), Argyrosaurus (Mannion and Otero, 2012), and Malawisaurus

563

(Gomani, 2005). The proximal and distal ends are mediolaterally expanded; the proximal end is

564

also anteroposteriorly compressed, as in other titanosaurs, e.g. Andesaurus and Rapetosaurus.

AC C

EP

TE D

M AN U

SC

RI PT

540

24

ACCEPTED MANUSCRIPT Pelvic girdle

566

Ilium. One fragmentary right ilium is preserved (MMS/VBN.12.32) (Figure 12A-B). It consists of

567

the dorsal part of the acetabulum, ventral fragments of the pre- and postacetabular processes

568

of the iliac blade, and the pubic peduncle. The preacetabular process is slightly horizontal

569

(more than in other titanosaurs) and laterally projected, and has a ventral ridge that ends

570

above the acetabulum, contrary to the ilia of Lirainosaurus and Lohuecotitan, which have a

571

vertical preacetabular lobe. The postacetabular process is vertical. The pubic peduncle

572

(anteroposterior length: 7.8 cm; transversal length: 8.7 cm) is robust, becomes broader

573

towards its distal end, and has a C-shaped cross-section. The posterior surface of the distal half

574

of the peduncle is particularly concave and surrounded by two sharp ridges. This morphology is

575

not known in any other titanosaur, and is consequently considered as an autapomorphy of

576

Atsinganosaurus. The lateral ridge extends through the dorsal edge of the acetabulum and

577

runs through the ventral edge of the preacetabular lobe. There is no triangular hollow at the

578

base of the pubic peduncle, contrary to Lirainosaurus (Díez Díaz et al., 2013b). The acetabulum

579

is not as strongly concave as it is in Paludititan. Both ilia are pneumatized, as in Lirainosaurus

580

(Díez Díaz et al., 2013b), Diamantinasaurus (Poropat et al. 2015) and derived titanosaurs (see

581

Cerda et al., 2012). However, this could be a synapomorphy of a more inclusive clade than just

582

Titanosauria, as Euhelopus also has pneumatized ilia (see Wilson and Upchurch, 2009;

583

Mannion et al., 2013).

584

Ischium. One right ischium (MMS/VBN.09.51c) has been recovered (Figure 12C-E, Table 5). The

585

iliac peduncle is incompletely preserved, its distal edge is missing. The plate-like morphology of

586

this element, and the absence of an emargination along the anterior margin of the ischiadic

587

blade, are common features in titanosaurs (Wilson, 2002; Upchurch et al., 2004; González Riga

588

et al., 2009). The acetabular margin is almost flat, as also observed in Ampelosaurus (Le Loeuff,

589

2005, Fig. 4.17), and it is not well differentiated from the iliac peduncle. This feature is

AC C

EP

TE D

M AN U

SC

RI PT

565

25

ACCEPTED MANUSCRIPT interesting to analyze more carefully, as an acute acetabular margin is a diagnostic feature

591

within Lithostrotia (see D’Emic, 2012). Both Atsinganosaurus and Ampelosaurus are grouped

592

together in our phylogenetic analysis (see below), so maybe we are talking about a diagnostic

593

feature within these French taxa. The iliac peduncle is slender and well developed, contrasting

594

with the wider and more robust peduncles in Ampelosaurus and Paludititan. The pubic

595

peduncle is poorly preserved, but seems continuous with the anteroventral edge of the

596

ischium. The ischia of Ampelosaurus and Paludititan are boomerang-shaped and their pubic

597

peduncle is well differentiated from their distal blade. At the base of the iliac peduncle, a

598

lateral tubercle (with a groove associated, as in Titanosauriformes [Poropat et al., 2016]) is

599

present near the posterior edge of the proximal part of the blade. This lateral ridge could

600

correspond to the bulge interpreted by Borsuck-Białynicka (1977) as the attachment point for

601

m. flexor tibialis internus III (see also Poropat et al., 2015). This lateral tubercle or tuberosity

602

seems to be a diagnostic feature within Titanosauria (Carballido et al., 2017). At about the

603

middle of the ischiadic blade, near its ventral margin, a lateral ridge is present. The ischiadic

604

blade is a straight plate, whose thickness decreases towards its distal edge.

605

Hindlimb

606

Femur. MMS/VBN.09.126 is the diaphysis of a right femur (Figure 13A-B, Table 3). Its proximal

607

and distal extremities are not preserved, but a low and poorly developed fourth trochanter is

608

present posteromedially, as in Lirainosaurus and Ampelosaurus, and contrasting with the more

609

centrally-situated fourth trochanter in Lohuecotitan. The diaphysis seems wider than in the

610

Spanish taxa, but more lateromedially developed than in Ampelosaurus (e.g. C3-87).

611

Tibia. MMS/VBN.02.90 is a left tibia (Figure 13C-H, Table 3). This bone was previously

612

identified as a metacarpal by Garcia et al. (2010), but it is highly similar as MMS/VBN.02.109

613

(although this last specimen is larger [Figure 13K-P]). This bone is slender, with an expanded

614

proximal third and a distal extremity with a triangular outline in distal view. Both articular

AC C

EP

TE D

M AN U

SC

RI PT

590

26

ACCEPTED MANUSCRIPT

surfaces are poorly preserved, but the shallow surface of the anterolaterally-projected cnemial

616

crest can be observed. No “tuberculum fibularis” can be seen in the internal face of the

617

cnemial crest. A second cnemial crest is absent too, as is the case of most somphospondylans

618

and diplodocoids (Mannion et al., 2013). Its proximal end appears compressed as in

619

Lirainosaurus, contrasting with the more rounded ones in Lohuecotitan and Ampelosaurus.

620

Distally, a prominent anteromedial ridge delimits two concave surfaces, as in Lirainosaurus

621

(MCNA 2203).

622

Fibula. MMS/VBN.09.132 is the proximal third of a fibula (Figure 13I-J, Table 3). It is more

623

expanded than the diaphysis and slightly lateromedially compressed, as in Lirainosaurus and

624

Ampelosaurus, and unlike in Lohuecotitan. Its lateral surface is convex, whereas its poorly

625

preserved medial surface is flat to slightly concave. The lateral trochanter is not preserved.

626

Metatarsal. The left metatarsal I (UP/VBN.93.10; Figure 14, Table 4) was only briefly described

627

by Garcia et al. (2010). It is a robust element, with expanded proximal and distal edges. Its

628

shaft is more slender than in other titanosaurs (e.g. Rapetosaurus, Epachthosaurus [Martínez

629

et al., 2014], Bonitasaura [Gallina and Apesteguía, 2015], Notocolossus [González Riga et al.,

630

2016], or Mendozasaurus [González Riga et al., 2018]). Its proximal surface is quadrangular in

631

outline. The proximal and distal medial surfaces are slightly concave for articulation with

632

metacarpal II. The distal articular surface is poorly preserved, but apparently had a comma-

633

shaped outline. In lateral view, a ridge extends from the middle of the shaft down to the

634

posterior edge of the distal articular surface. It also presents a prominent ventrolateral

635

expansion along its distal half, such that the distal end expands further laterally than the

636

proximal end.

AC C

EP

TE D

M AN U

SC

RI PT

615

637 638

HISTOLOGICAL OBSERVATIONS

27

ACCEPTED MANUSCRIPT 639

All Atsinganosaurus sections display a similar bone histology, dominated by heavy remodelling

640

of the primary bone and several cross-cutting generations of secondary osteons (sensu Stein et

641

al., 2010 and Mitchell et al., 2017; Figure 15A-B). No pristine in situ trabecular structures can be identified because the transition

643

between the medullary cavity and the innermost cortex is abrupt and goes from broken

644

trabeculae (sometimes embedded in sediments [Figure 15C]) to crushed, distorted secondary

645

osteons.

SC

RI PT

642

The secondary osteons are mature, rounded to elliptical in shape, and composed of

647

successive layers of alternating bone lamellae (as seen under cross polarized light, type two

648

osteons sensu Ascenzi and Bonucci, 1968; Figure 15A). The elliptical osteons have the long axis

649

preferentially oriented parallel to the periosteal surface in transverse section, a feature also

650

seen in other titanosaurs (e.g. Phuwiangosaurus sirindhornae and Ampelosaurus atacis in Klein

651

et al., 2009 and Klein et al., 2012a respectively). In long bones of A. velauciensis, four to five

652

generations of secondary osteons can be recognized in the innermost cortex, five to six

653

generations in the mid-cortex and four to six generations in the outer cortex (see Table 6

654

below for details – Fig. 15B). No open resorption cavities were observed in the innermost

655

cortex in any of the samples. Instead, the innermost cortex is often characterized by irregular

656

secondary osteons which are found with broken trabeculae. MMS/VBN.09.126 and

657

MMS/VBN.09.A.018 are the best sections showing the broken trabeculae.

TE D

EP

AC C

658

M AN U

646

All samples except MMS/VBN.09.A.018 show some patches of primary tissue. These

659

patches are mostly confined to the outer cortex. However, no unambiguous primary vascular

660

canals can be seen in any of these patches. It is possible that the outermost µm of the cortical

661

samples are missing because of weathering or mechanical preparation.

662 663

Following Klein and Sander (2008) and Stein et al. (2010), the studied specimens match the Histologic Ontogenetic Stage (HOS) 14 because of the complete remodelled type H bone

28

ACCEPTED MANUSCRIPT 664

tissue of the cortices (Fig. 15A, E and F). Dense secondary osteons are clearly visible even

665

macroscopically as purple dots in Fig. 15E. Given the multiple cross-cutting secondary osteon

666

generations throughout the cortex, the Remodelling Stages (RS) (sensu Mitchell et al., 2017)

667

are ranging from RS 13 to 14. Longitudinal sections (Figure 15D-F) were made to complement data from the

RI PT

668

transverse sections, in particular to verify any preferential orientation of the secondary

670

osteons. Their oval shape in transverse section could be either the result of a section plane at a

671

slight angle to the ideal transverse section (Mitchell et al., 2017) or of the 3D geometry of the

672

osteons not correlating to the long bone axis. The osteonal boundaries are more difficult to

673

see, and so are the different cross-cutting generations. The cortices yield a widespread

674

remodelled histology with very elongated secondary osteons meaning they are mainly

675

oriented along the long bone axis (purple lines in Fig. 15F). Some secondary osteons have an

676

ellipsoid appearance, which implies they are oriented oblique to the long bone axis.

M AN U

The histology of a putative cervical rib (MMS/VBN.09.51a and b) is characterized by

TE D

677

SC

669

strong remodelling features, and only a small part of the original ossified tendon matrix is still

679

present (Figure 16). Numerous tensile secondary osteons (sensu Ascenzi and Bonuci, 1968)

680

with smooth cement lines make up the most significant part of the tissue, some of them

681

showing cross-cutting relations. However, interstitially, small areas remain unremodelled and

682

show densely packed collagen fibre bundles, similar to those in the ossified tendons of

683

hadrosaurs (Adams and Organ, 2005; Organ and Adams, 2005) and elongated cervical ribs of

684

other sauropod dinosaurs (Cerda, 2009; Klein et al., 2012b).

685

AC C

EP

678

In a longitudinal section (Figure 16), the longitudinal vascular canals of the secondary

686

osteons are dominant features, and the osteons have longitudinally oriented osteocyte

687

lacunae with faint but numerous branching canaliculi. In between the longitudinally oriented

29

ACCEPTED MANUSCRIPT 688

osteons, fibre bundles with fibrocyte lacunae can be observed. These features complement the

689

cross sectional view and are furthermore reminiscent of ossified tendons.

690

Taking into account the strongly elongated morphology, parallel occurrence in the sediment and ossified tendinous histology of the two described elements, there can be little

692

doubt that they represent the ossified tendons of sauropod cervical ribs.

RI PT

691

693

695

PHYLOGENETIC ANALYSIS

SC

694

The result of this phylogenetic analysis with 29 sauropod taxa yielded a single MPT of 166 steps, with a consistency index (CI) of 0.572 and a retention index (RI) of 0.665 (Figure 17).

697

The general topology is similar to the one obtained by Salgado et al. (2015), but with two main

698

differences: i) the diagnosis of Lithostrotia has been resolved, with Malawisaurus placed in a

699

more derived position than Andesaurus (and therefore within Titanosauria); ii) the derived

700

clade Saltasauridae has been divided, with Opisthocoelicaudiinae regarded as a more basal

701

group than Saltasaurinae (this split can be also seen in the analysis of Sallam et al. 2018).

702

Another notable difference with previous phylogenetic analyses is the recovery of

703

Lognkosauria within Rinconsauria. Similar results were obtained by González Riga et al. (2018),

704

resolving Lognkosauria as the sister taxon of Rinconsauria. The phylogenetic relationships of

705

this clade seem more difficult to solve, as it has been placed as a basal clade within Lithostrotia

706

(Calvo et al., 2007, González Riga et al., 2009), or as more derived lithostrotians (González Riga

707

et al., 2016) related with Aeolosaurini (González Riga and Ortiz, 2014) or with Rinconsauria

708

(Salgado et al., 2015). However, this discussion is beyond the scope of this paper; herein, we

709

focus on the relationships between the European taxa.

710 711

AC C

EP

TE D

M AN U

696

European taxa were almost completely neglected in previous titanosaurian phylogenies: Sallam et al. (2018) include all of the Late Cretaceous European taxa, but before

30

ACCEPTED MANUSCRIPT

this work only few included Lirainosaurus and Ampelosaurus together (see e.g. Powell, 2003;

713

Curry Rogers, 2005), and most of the time separately or scored only from the literature (see

714

e.g. González Riga, 2003; Upchurch et al., 2004; Bonaparte et al., 2006; Calvo et al., 2007;

715

González Riga et al., 2009; Hocknull et al., 2009; Csiki et al., 2010). As previously suggested by

716

Bonaparte et al. (2006), González Riga et al. (2009), Gallina and Apesteguía, (2011), Salgado et

717

al. (2015), and Sallam et al. (2018), the present analysis recovers Lirainosaurus as a member of

718

Lithostrotia, whereas it was regarded as a derived titanosaur more closely related to

719

Saltasauridae by Upchurch et al. (2004), Calvo et al. (2007), Csiki et al. (2010), and Filippi et al.

720

(2011), or even a member of the saltasaurid clade by Hocknull et al. (2009) and Díez Díaz et al.

721

(2013d). In our analysis, Lirainosaurus appears as a lithostrotian closely related to a clade

722

formed by the French titanosaurs Ampelosaurus and Atsinganosaurus. This clade is here

723

named Lirainosaurinae nov. Both French titanosaurs have been included in a few analyses

724

(only together in Sallam et al. (2018)), and their relationships have not been well studied (e.g.

725

Powell, 2003; Curry Rogers, 2005; Sallam et al. 2018). Díez Díaz et al. (2013d) suggested that

726

French titanosaurs were basal lithostrotians and that Lirainosaurus a member of

727

Opisthocoelicaudiinae. However, Díez Díaz (2013) scored these three titanosaurs in two

728

previously published matrices (Bonaparte et al., 2006; González Riga et al., 2009), and in both

729

phylogenetic hypotheses the three taxa appeared closely related. Lohuecotitan and Paludititan

730

are grouped together as basal lithostrotians. The phylogenetic affinities of Paludititan are not

731

well resolved (Csiki et al., 2010), and Lohuecotitan has only been scored in Díez Díaz et al.

732

(2016) and Sallam et al. (2018), so few comments can be made here, besides the lack of

733

affinities of Lirainosaurus with the French taxa. The Early Cretaceous French taxon

734

Normanniasaurus is nested within Titanosauria, but not within Lithostrotia.

AC C

EP

TE D

M AN U

SC

RI PT

712

735 736

DISCUSSION

31

ACCEPTED MANUSCRIPT

After the detailed study and comparison of the specimens published by Garcia et al. (2010) and

738

the ones described in this work, an emended diagnosis of A. velauciensis is suggested. The new

739

diagnosis focuses on the ilium: pubic peduncle of the ilium with a posterior concave surface in

740

its distal half, surrounded by two sharp ridges. Three isolated humeri (the most recurring non-

741

axial bone in the site) have been found, so at least three individuals of Atsinganosaurus are

742

present at Velaux-La-Bastide Neuve. However, besides the holotype, no other remains were

743

found associated or articulated, so their referral to each individual it is not possible. It should

744

be noted that further titanosaurian remains have been found at Velaux-La Bastide Neuve and

745

they present several divergences (especially humeri and an ulna) with the holotype and

746

material referred to Atsinganosaurus velauciensis by Garcia et al. (2010). The remains ascribed

747

to this possible new taxon were most of them found in the same level as the ones belonging to

748

Atsinganosaurus, with the exception of one almost complete sacrum and a humerus, that

749

were recovered from a second level (2 meters above the former one). This new material is

750

currently under study.

751

Estimation of Body Size and Mass for Atsinganosaurus velauciensis

752

As we have recovered several humeri and femora we can hypothesize the body size and mass

753

for Atsinganosaurus. For the body mass and size we have used the equations proposed by

754

Seebacher (2001) for size, and Packard et al. (2009) and Campione and Evans (2012) for mass,

755

in which M(g) = 3.352PerH+F2,125, M(kg) = 214.44L(m)1.46, and logM(g) = 2.754logPerH+F −

756

1.097, where M: body mass, PerH+F: sum of the perimeters of the humerus and femur in mm,

757

L: body length. With the smallest humerus and femur we obtain a size of 6.45 meters, and a

758

mass of 2.46 tonnes (sensu Packard et al., 2009) and 3.2 tonnes (sensu Campione and Evans,

759

2012), whereas with the largest specimens the results are 14.54 meters, and 3.661 tonnes

760

(sensu Packard et al., 2009) and 5.26 tonnes (sensu Campione and Evans, 2012).

AC C

EP

TE D

M AN U

SC

RI PT

737

32

ACCEPTED MANUSCRIPT 761

We tentatively propose a body length of ca. 8-12 meters for the adults of Atsinganosaurus, or as much as 14 meters for the largest individuals, and a body mass of ca.

763

3.5-5 tonnes. Although it is a sauropod of small size, it probably doubled (or even tripled) the

764

length of Lirainosaurus (4 meters and 2-4 tonnes, Díez Díaz et al., 2013b).

765

Ontogeny and Dwarfism

766

In general, all sampled specimens of A. velauciensis show very similar histological features.

767

Clearly, the samples do not represent a growth series and are all of comparable developmental

768

stages. The histology of A. velauciensis is comparable to that of the small European titanosaurs

769

Lirainosaurus astibiae (adult specimen descriptions in Company, 2011, fig. 5) and

770

Magyarosaurus dacus (Stein et al., 2010).

SC

M AN U

771

RI PT

762

Heavy remodelling is the main histological pattern in the long bones of A. velauciensis. This mature histology suggests that these individuals were fully grown. Considering the

773

reduced size of the femur and humeri, the remodelling process would have begun early in the

774

ontogeny of this titanosaur compared to non-titanosaurian sauropods, at a rate that surpassed

775

the apposition rate. This is consistent with the histology of juveniles of the titanosaur

776

Rapetosaurus krausei (Rogers et al., 2016). If the haversian bone deposition rate is assumed to

777

be constant throughout ontogeny (Mitchell and Sander, 2014), the combination of a slow

778

apposition rate with heavy remodelling prior to the final size involves some kind of size

779

reduction and/or insular dwarfism comparable to other titanosaurs in the Cretaceous

780

European archipelago (e.g. Lirainosaurus astibiae, Magyarosaurus dacus; Company, 2011;

781

Stein et al., 2010).

AC C

EP

TE D

772

782 783

Palaeobiogeographical considerations

33

ACCEPTED MANUSCRIPT 784

Our new phylogenetic results shed light on the palaeobiogeographical patterns of the

785

titanosaurian faunas from the Ibero-Armorican Island. With these results we can suggest two

786

different scenarios:

787

1) Csiki-Sava et al. (2015) commented that European titanosaurs do not seem to have a southern influence, but in our analysis we have found that Lohuecotitan and

789

Paludititan are grouped together close to the basal African lithostrotian Malawisaurus.

790

Works on the Cretaceous titanosaurian faunas from Africa (see Gorscak et al. 2014,

791

2017; Lamanna et al., 2017; and works in progress) will help to clarify soon the

792

relationships of these faunas with the Late Cretaceous European ones. Indeed, the

793

titanosaur Mansourasaurus from the Late Cretaceous of Egypt seems to be closely

794

related to Lohuecotitan (Sallam et al., 2018), supporting sauropod dispersal between

795

Europe and Africa in the terminal Cretaceous. Therefore, a Gondwanan influence

796

cannot be discarded; this has been also previously posited for other groups of reptiles

797

(Pereda Suberbiola, 2009).

SC

M AN U

TE D

798

RI PT

788

2) The case of the more derived lithostrotians Lirainosaurus and the French taxa

800

Ampelosaurus and Atsinganosaurus is likely different. This group, here named

801

Lirainosaurinae, could lead to a possible endemicity in the Ibero-Armorican Island, and

802

that is why Lirainosaurus (late Campanian) and the French titanosaurs (late

804

AC C

803

EP

799

Campanian-early Maastrichtian) appear to be closely related. As Pereda et al. (2009)

and Mannion and Upchurch (2011) suggested, Late Cretaceous European dinosaurs

805

could be relictual lineages of Laurasian faunas, and Lirainosaurinae could be a good

806

example of this. It is also possible that the late Maastrichtian taxa found in the

807

Pyrenean region (northern Spain and southern France) and southeastern France (i.e.

808

Vitrolles la Plaine, Valentin et al., 2012) evolved from these titanosaurs known from

809

late Campanian–early Maastrichtian faunas.

34

ACCEPTED MANUSCRIPT 810

These hypotheses represent a solid foundation for future phylogenetic and

811

palaeobiogeographical analyses incorporating the Cretaceous European titanosaurian faunas,

812

following on from palaeobiogeographic analyses primarily focused on titanosaurs from

813

elsewhere (e.g. Gorscak et al. 2016; Poropat et al. 2016).

RI PT

814 CONCLUSIONS

816

In this work we describe new titanosaurian cranial and postcranial remains found in the Upper

817

Cretaceous site of Velaux-La Bastide Neuve (southern France), which are referred to

818

Atsinganosaurus velauciensis. This new material has allowed us to better define the

819

morphological features of this taxon and emend its diagnosis, thereby helping us to better

820

understand the sauropod faunas that inhabited the Ibero-Armorican Island.

M AN U

SC

815

Long bones of Atsinganosaurus velauciensis are heavily remodelled (HOS 14, RS

822

ranging from stage 13 to 14). The sampled specimens of A. velauciensis were fully grown. The

823

small size but mature nature of the specimens might be linked to insular dwarfism, as seen in

824

Magyarosaurus or Lirainosaurus. However, Atsinganosaurus was larger than these two taxa, as

825

shown by its hypothesized body size and mass: ca. 8-12 meters for the adults, or as much as 14

826

meters for the largest individuals, and ca. 3.5-5 tonnes.

EP

AC C

827

TE D

821

A phylogenetic analysis with 29 sauropod taxa was performed, with the European

828

titanosaurs Atsinganosaurus, Ampelosaurus, Lirainosaurus, Lohuecotitan, Paludititan (Late

829

Cretaceous) and Normanniasaurus (Early Cretaceous) all scored for the same analysis for the

830

first time. Atsinganosaurus and Ampelosaurus form a clade closely related to Lirainosaurus

831

within Lithostrotia, whereas Lohuecotitan and Paludititan are grouped together as basal

832

lithostrotians. Lirainosaurinae is defined here for the first time as Lirainosaurus astibiae,

833

Ampelosaurus atacis, their common ancestor, and all of its descendants. Atsinganosaurus

35

ACCEPTED MANUSCRIPT 834

velauciensis appears within this clade, as sister taxon of Ampelosaurus. As for

835

Normanniasaurus, it is nested within Titanosauria but not within Lithostrotia. From a palaeobiogeographical perspective, the phylogenetic results suggest that

837

European titanosaurs belong to at least three distinct lineages and that two lithostrotian

838

lineages were present during the latest Cretaceous in the European archipelago. Although the

839

“African origin” of the latest Cretaceous re-invasion of Europe is not well-supported by other

840

groups of tetrapods (see Mannion and Upchurch, 2011 and references therein), the results

841

obtained in this work and the one published by Sallam et al. (2018) shed some light on one

842

possible dispersal route between North Africa and Europe during the Cenomanian–Campanian.

843

More works on the African titanosaurs are needed to test if these African faunas are closely

844

related with other South American titanosaurian clades, as previously hypothesized by

845

Mannion and Upchurch (2011). On the other hand, Lirainosaurinae could be a relictual lineage

846

of Laurasian sauropod faunas. To assess these hypotheses more inclusive (with more Late

847

Cretaceous Laurasian taxa, together with the African and European ones) phylogenetic and

848

paleobiogeographical should be done.

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The diversity of the titanosaurian faunas from the Late Cretaceous of Europe, and more specifically from the Ibero-Armorican Island, has been an important research issue since

851

the last years of the 19th century (see e.g. Le Loeuff, 1993), always suggesting a higher

852

diversity than previously thought. According to the findings of these last years, especially in

853

Spain, France, and Romania, this diversity has been increased to, at least, seven titanosaurian

854

taxa in the Campanian-Maastrichtian of Europe. However, new findings and reanalyses of

855

previously published material will no doubt increase this further.

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ACKNOWLEDGMENTS

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M. Moreno-Azanza (Universidade Nova de Lisboa, Portugal) helped in the development of the

859

phylogenetic analysis. VDD would like to thank V. Fondevilla (ICP, Spain) for the useful

860

discussions on titanosaurian faunas and stratigraphy. We would like to acknowledge A.

861

Montaufier for the photographs (with financial support of the Lisea-Vinci group), and C. Zafra

862

for editing the figures. We thank J. C. Corral and J. Alonso (Museo de Ciencias Naturales de

863

Álava/Arabako Natur Zientzien Museoa, Vitoria-Gasteiz, Spain), B. Madarieta (Museo Vasco de

864

Historia de la Medicina y de las Ciencias of Leioa, Spain), F. Ortega (Grupo de Biología

865

Evolutiva, Universidad Nacional de Educación a Distancia, Spain), J. Le Loeuff (Musée des

866

Dinosaures d’Espéraza, France), P. Barrett (Natural History Museum, U.K.), and B. González

867

Riga (IANIGLA, CRICyT, Mendoza, Argentina) for access to collections under their care. The Willi

868

Hennig Society sponsors the use of the TNT cladistics software. Research work of XPS was

869

supported by the Ministerio de Economía y Competitividad of Spain (MINECO, project

870

CGL2017-85038-P), the European Regional Development Fund, the Gobierno Vasco/Eusko

871

Jaurlaritza (research group IT-1044-16) and the Universidad del País Vasco (UPV/EHU, research

872

group PPG17/05), and works of BJ by the FRIA grant. BJ-C thanks J. Laval for producing the thin

873

sections for histological purposes, V. Fischer for his useful critics on the long bone histology

874

part, and J. Jentgen for having helped a lot to produce the histological figures. We are greatly

875

indebted to P.M. Mannion (UCL, UK) and S.F. Poropat (Swinburne University of Technology,

876

Hawthorn, Australia), which provided useful comments that helped improving this work. This

877

work has been developed thanks to the collaboration between Palaios (research association in

878

which XV is the president), the University of Poitiers, the Velaux Municipality (J.-P. Maggi and

879

L. Melhi) with its heritage, culture and technical services (M. Calvier, and S. Chauvet), the

880

environment department from CD 13 (M. Bourrelly, T. Tortosa, G. Michel, N. Mouly, and S.

881

Amico), the ‘Service Départemental d’Incendie et de Secours’ (SDIS 13), and numerous

882

volunteers during the field campaigns in 2009 and 2012. This work was supported by the

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Ministry of Education and Communication (research grant VR1013 to Palaios association), the

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Bouches du Rhône department CD 13 proposals MAPADGAC23112010-1 and

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1159 Mannion, P.D., Upchurch, P., Barnes, R.N., Mateus, O. 2013. Osteology of the Late Jurassic

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1183 Matheron, P. 1869. Note sur les reptiles fossiles des dépôts fluvio-lacustres crétacés du basin à

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Dinosaurs. Journal of Vertebrate Paleontology 21(1), 51-60.

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Magyarosaurus dacus (Sauropoda: Titanosauria), PNAS 107, 9258-9263. DOI:

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1283 Upchurch, P., Barrett, P., Dodson, P. 2004. Sauropoda. In: Weishampel, D.B., Dodson, P.,

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Vullo, R., Garcia, G., Godefroit, P., Cincotta, A., Valentin, X. In press. Mistralazhdarcho maggii

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gen. et sp. nov., a new azhdarchid pterosaur from the Upper Cretaceous of southeastern

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France. Journal of Vertebrate Paleontology.

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Wedel, M.J. 2003. The evolution of vertebral pneumaticity in sauropod dinosaurs. Journal of

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Vertebrate Paleontology 23(2), 344-357.

1308 Wedel, M.J., Taylor, M.P. 2013. Caudal Pneumaticity and Pneumatic Hiatuses in the Sauropod

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Dinosaurs Giraffatitan and Apatosaurus. PLoS ONE 8(10), e78213. DOI:

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10.1371/journal.pone.0078213

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Wilson, J.A. 1999. A nomenclature for vertebral laminae in sauropods and other saurischian

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dinosaurs. Journal of Vertebrate Paleontology 19, 639-653.

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Wilson, J.A. 2002. Sauropod dinosaur phylogeny: critique and cladistic analysis. Zoological

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Journal of the Linnean Society 136, 217-276.

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Wilson, J.A. 2006. Anatomical nomenclature of fossil vertebrates: standardized terms or lingua

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biomechanical and systematic perspective on sauropod locomotion. Paleobiology 25, 252-267.

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Wilson, J.A., Upchurch, P. 2003. A revision of Titanosaurus Lydekker (Dinosauria-Sauropoda),

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the first dinosaur genus with a “Gondwanan” distribution. Journal of Systematic Palaeontology

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1, 125-160.

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Wilson, J.A., Upchurch, P. 2009. Redescription and reassessment of the phylogenetic affinities

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of Euhelopus zdanskyi (Dinosauria: Sauropoda) from the Early Cretaceous of China. Journal of

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Systematic Palaeontology 7, 199–239.

1335 Wilson, J.A., D'Emic, M.D., Ikejiri, T., Moacdieh, E.M., Withlock, J.A. 2011. A nomenclature for

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10.1371/journal.pone.0017114

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Wilson, J.A., Pol, D., Carvalho, A.B., Zaher, H. 2016. The skull of the titanosaur Tapuiasaurus

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macedoi (Dinosauria: Sauropoda), a basal titanosaur from the Lower Cretaceous of Brazil.

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Zoological Journal of the Linnean Society 178(3), 611-662. DOI: 10.1111/zoj.12420.

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Zaher, H., Pol, D., Carvalho, A.B., Nascimento, P.M., Riccomini, C., Larson, P., Juárez-Valieri, R.,

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Pires-Domingues, R., da Silva Jr., de Almeida Campos, N.J.D. 2011. A complete skull of an early

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Cretaceous Sauropod and the evolution of advanced Titanosaurians. PLoS ONE 6(2), e16663.

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FIGURE LEGENDS

AC C

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1351

Figure 1. (A) Simplified geological map of the Aix-en-Provence Basin (Bouches-du-Rhône,

1352

France). Arrow indicates the location of the Velaux-La Bastide Neuve site. (B) Map indicating

1353

the repartition of vertebrate specimens collected since 1993 including some important

1354

titanosaurian bones (without the institutional abbreviations) and the concentration of bones

1355

collected in 2009 (a) and 22012 (b).

1356

56

ACCEPTED MANUSCRIPT Figure 2. Cranial remains of the titanosaur Atsinganosaurus velauciensis. Right fragment of a

1358

braincase (MMS/VBN.09.167) in (A) lateral and (B) medial views. Left pterygoid

1359

(MMS/VBN.09.158a) in (C) medial and (D) lateral views. Occipital condyle (MMS/VBN.09.41 ) in

1360

(E) right lateral view. Tooth (MMS/VBN.12.A.006) in (F) labial view. Abbreviations as in the

1361

text.

RI PT

1357

1362

Figure 3. Cervical vertebrae of the titanosaur Atsinganosaurus velauciensis. Posterior cervical

1364

vertebrae, previously described by Garcia et al. (2010), in left lateral view: (A) UP/VBN.93.12a

1365

(B), UP/VBN.93.12b, and (C) UP/VBN.93.12c. (D) Anterior cervical vertebra

1366

(MMS/VBN.12.B.015), with parts of the subsequent centrum ventrally associated to it in left

1367

lateral view. Posterior view of (E) UP/VBN.93.12a and (F) MMS/VBN.12.B.015. (G) Anterior

1368

cervical vertebra (MMS/VBN.12.A.004), with a fragment of the cervical rib, in right lateral view.

1369

Abbreviations as in the text.

M AN U

TE D

1370

SC

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Figure 4. Posterior cervical vertebra (MMS/VBN.12.B.010), and interpretative drawings, of the

1372

titanosaur Atsinganosaurus velauciensis in (A, A’) left lateral, (B, B’) anterior, (C, C’) right

1373

lateral, and (D, D’) posterior views. Abbreviations as in the text.

AC C

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EP

1371

1375

Figure 5. Fragmentary dorsal vertebrae and ribs of the titanosaur Atsinganosaurus

1376

velauciensis. (A) fragment of an anterior dorsal neural arch (MMS/VBN.93.32) in anterior view,

1377

(B) fragmentary dorsal vertebra (UP/VBN.09.157) in right lateral view, and (C) fragmentary

1378

middle to posterior dorsal vertebra (MMS/VB.93.02) in posterolateral view. Dorsal ribs

1379

MMS/VBN.07.D.07b in (D) lateral and (E) medial views, and MMS/VBN.07.D.07a in in (F) lateral

1380

and (G) medial views. Abbreviations as in the text.

57

ACCEPTED MANUSCRIPT 1381

Figure 6. Sacrum (MMS/VBN.02.82) of the titanosaur Atsinganosaurus velauciensis, previously

1383

described by Garcia et al. (2010), in (A) right lateral, (B) anterior, (C) slightly ventrolateral, and

1384

(D) posterior views.

RI PT

1382

1385

Figure 7. Caudal vertebrae and haemal arches of the titanosaur Atsinganosaurus velauciensis.

1387

Anterior caudal vertebra (MMS/VBN. 00.14) in (A) left lateral, (B) anterior, (C) posterior, (D)

1388

ventral, and (E) dorsal views. Anterior caudal vertebra (MMS/VBN. 00.15) in (F) left lateral, (G)

1389

anterior, (H) ventral, and (I) dorsal views. Anterior caudal vertebra (MMS/VBN.93.31a) in (J)

1390

left lateral and (K) anterior views. Haemal arch (MMS/VBN. 93.31b) in (L) anterior and (M)

1391

posterior views. Anterior caudal vertebra (MMS/VBN. 02.110) in (N) left lateral, (O) anterior,

1392

(P) posterior, and (Q) ventral views. Middle to posterior caudal vertebra (MMS/VBN.09.D.003)

1393

in (R) left lateral, (S) anterior, (T) posterior, and (U) ventral views. Posterior (distal) caudal

1394

vertebra (MMS/VBN.93.32a) in (V) right lateral, (W) anterior, and (X) posterior views. Haemal

1395

arch (MMS/VBN.93.32b) in (Y) anterior and (Z) posterior views.

M AN U

TE D

EP

1396

SC

1386

Figure 8. Caudal vertebrae of the titanosaur Atsinganosaurus velauciensis. (A) anterior caudal

1398

vertebra (MMS/VBN.12.C.004) in left lateral view, (B) fragmentary anterior caudal vertebra

1399

(MMS/VBN.09.54) in left lateral view, (C) posterior caudal vertebra (MMS/VBN.12.C.003) in

1400

right lateral view, (D) fragmentary posterior caudal vertebra (MMS/VBN.09.D.010) in left

1401

lateral view, (E) posterior caudal vertebra (MMS/VBN.09.159.b) in right lateral view, (F)

1402

posterior caudal vertebra (UP/VBN.93.03), in left lateral view, (G) posterior caudal vertebra

1403

(UP/VBN.93.04), in right lateral view, (H) posterior caudal vertebra (UP/VBN.93.05), in right

1404

lateral view, (I) fragmentary posterior caudal vertebra (UP/VBN.93.06), in right lateral view (J)

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58

ACCEPTED MANUSCRIPT 1405

posterior caudal vertebra UP/VBN.93.07), in right lateral view, and (K) posterior caudal

1406

vertebra (UP/VBN.93.08), in right lateral view. F-K were previously described by Garcia et al.

1407

(2010).

RI PT

1408 Figure 9. Scapular girdle remains of the titanosaur Atsinganosaurus velauciensis. Fragmentary

1410

left scapulocoracoid (MMS/VBN.02.78a–b) in (A) lateral and (B) medial views. (C) Left scapula

1411

(MMS/VBN.93.11) in medial view. (D) Right juvenile scapula (MMS/VBN.09.124D) in lateral

1412

view.

SC

1409

M AN U

1413

Figure 10. Forelimb remains of the titanosaur Atsinganosaurus velauciensis. Right humerus

1415

(MMS/VBN.00.12), previously described by Garcia et al. (2010), in (A) anterior, (B) medial, (C)

1416

posterior, and (D) lateral views. Left humerus (MMS/VBN.09.A.018) in (E) anterior, (F) medial,

1417

(G) posterior, and (H) lateral views. Right humerus (VBN.93.MHNA.99.52) in (I) anterior and (J)

1418

posterior views. Right ulna (MMS.VBN.12.P.06a) in (K) proximal (medial towards top), (L)

1419

medial, (M) posterior, (N) lateral, (O) distal (lateral towards top), and (P) anterior views.

1420

Fragmentary radius (MMS/VBN.09.D.001) in (Q) anterior/posterior? and (R)

1421

posterior/anterior? views.

EP

AC C

1422

TE D

1414

1423

Figure 11. Metacarpal remains of the titanosaur Atsinganosaurus velauciensis. Left metacarpal

1424

I (MMS/VBN.09.113) in (A) dorsal, (B) posterior, (C) medial, and (D) lateral views. Left

1425

metacarpal I (UP/VBN.93.09) in (E) dorsal, (F) posterior, (G) medial, and (H) lateral views.

1426

59

ACCEPTED MANUSCRIPT 1427

Figure 12. Pelvic girdle of the titanosaur Atsinganosaurus velauciensis. Fragment of a right

1428

ilium (MMS/VBN.12.32) in (A) lateral and (B) ventromedial views. Right ischium

1429

(MMS/VBN.09.51c) in (C) lateral,(D), posterior, and (E) medial views. Abbreviations as in the

1430

text.

RI PT

1431

Figure 13. Hind limb remains of the titanosaur Atsinganosaurus velauciensis. Diaphysis of a

1433

right femur (MMS/VBN.09.126) in (A) anterior and (B) posterior views. Left tibia

1434

(MMS/VBN.02.90) in (C) proximal (lateral towards bottom), (D) lateral, (E) anterior, (F) medial,

1435

(G) distal (medial towards top), and (H) posterior views. Proximal third of a fibula

1436

(MMS/VBN.09.132) in (I) lateral and (J) medial views. Left tibia (MMS/VBN.02.109) in (K)

1437

proximal (lateral towards bottom), (L) lateral, (M) anterior, (N) medial, (O) distal (medial

1438

towards top), and (P) posterior views.

TE D

1439

M AN U

SC

1432

Figure 14. Left metatarsal I (MMS/VBN.93.10), previously described by Garcia et al. (2010), of

1441

the titanosaur Atsinganosaurus velauciensis in (A) dorsal, (B) distal, (C) medial, (D) proximal, (E)

1442

ventral (dorsal toward bottom), and (F) lateral (dorsal towards top) views.

AC C

1443

EP

1440

1444

Figure 15. Micro- and macrohistology of the titanosaur Atsinganosaurus velauciensis. A-C and

1445

E: transverse sections. D and F: longitudinal sections. (A) heavy remodelling of the cortex

1446

(MMS/VBN.09.A.018). (B) zoom with multiple secondary osteon generations indicated by

1447

numbers (MMS/VBN.09.A.018). (C) broken trabeculae trapped in sediments at the base of the

1448

core (MMS/VBN.09.A.018). (D) longitudinal section of MMS/VBN.09.126. (E-F) macrohistology

1449

of MMS/VBN.09.126 in radial and longitudinal section respectively. Scale bars: A-B = 0.5 mm,

1450

C-D = 1 mm, E-F = 1 cm.

60

ACCEPTED MANUSCRIPT 1451 Figure 16. Neck rib histology of the titanosaur Atsinganosaurus velauciensis. (A) overview of

1453

the two ribs in their storage unit, with inset illustrating the sectioning planes. The arrow in A,

1454

D, and E indicates the longitudinal axis. (B) composite image (plane polarized light and cross

1455

polars) with an overview of the histology of the sauropod cervical ribs in cross section. Note

1456

the patches of longitudinally running collagen fibre bundles. (C) composite image (in plane

1457

polarized light and cross polars) of the secondary osteons and fibre bundles in cross section at

1458

high magnification. Note the cross cutting relationships of some of the secondary osteons. (D)

1459

overview (plane polarized light) of the histology of the cervical ribs in longitudinal section. (E)

1460

detail of D. Note the strong longitudinal orientation of the osteons and osteocyte lacunae, as

1461

well as the fibre bundles with fibrocytes. Abbreviations: cl, cementing line; fb, fibre bundles;

1462

so, secondary osteon.

M AN U

SC

RI PT

1452

TE D

1463

Figure 17. Phylogenetic hypothesis. Only one MPT of 166 steps was obtained from the Salgado

1465

et al. (2015) data matrix, with a consistency index (CI) of 0.572 and a retention index (RI) of

1466

0.665. The European taxa are highlighted in the cladogram. The obtained nodes are (1)

1467

Titanosauriformes, (2) Titanosauria, (3) Lithostrotia, (4) Opisthocoelicaudiinae, (5)

1468

Saltasaurinae, (6) Aeolosaurinae, (7) Rinconsauria, (8) Lognkosauria, and (9) Lirainosaurinae.

AC C

1469

EP

1464

1470

TABLE LEGENDS

1471

Table 1. Measurements (in mm) of the teeth of the titanosaur Atsinganosaurus velauciensis.

1472

Abbreviations: Ø m-d: maximum mesiodistal width; Ø lb-ln: maximum labiolingual width; SI:

1473

slenderness index (Upchurch, 1998): length of the tooth crown divided by its maximum

61

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mesiodistal width; CI: compression index (Díez Díaz et al., 2013c): maximum labiolingual width

1475

divided by the maximum mesiodistal width of the crown.

1476 Table 2. Measurements (in mm) of the vertebrae of the titanosaur Atsinganosaurus

1478

velauciensis. Abbreviations: A, anterior; M, middle; P, posterior; D, distal; EI (Elongation index)

1479

(Upchurch, 1998): anteroposterior length of the centrum (without the condyle) divided by the

1480

midline width of the cotyle.

RI PT

1477

SC

1481

Table 3. Measurements (in mm) of the fore and hindlimb remains of the titanosaur

1483

Atsinganosaurus velauciensis. Abbreviations: Max. width Prox. end: maximum width of the

1484

proximal end; Max. width distal end: maximum width of the distal end; Min. AP Width:

1485

minimum anteroposterior width; Min. Cir. Diaph.: minimum circumference of the diaphysis;

1486

Min. Transv. Width: minimum transversal width; ECC (eccentricity index) (Wilson and Carrano,

1487

1999): mid-shaft mediolateral width divided by the anteroposterior width.

TE D

1488

M AN U

1482

Table 4. Measurements (in mm) of the metacarpal and metatarsal remains of the titanosaur

1490

Atsinganosaurus velauciensis. Abbreviations: AP, anteroposterior; ML, mediolateral.

1491

EP

1489

Table 5. Measurements (in mm) of the ischium of the titanosaur Atsinganosaurus velauciensis.

1493

Abbreviations: PP, pubic peduncle.

1494 1495

AC C

1492

Table 6. Histological data summary of Atsinganosaurus velauciensis.

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AC C

EP

TE D

M AN U

SC

RI PT

MMS/VBN.12.A.006 MMS/VBN.12.B.14 MMS/VBN.12.A.07 MMS/VBN.93.33

Crown length Ø m-d Ø lb-ln SI CI 190 33 23 5.76 0.69 180 45 4 160 37 33 4.32 0.89 150 39 3.85 -

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Centrum length Centrum length Vertebral Centrum height Centrum width Neural arch Neural spine (w/condyle) (wo/condyle) Heigth (posterior) (posterior) heigth heigth 352.5 330 195 220 230 185 255 280 -

333.5 270 175 195 200 155 235 252 220

240 300 310 220 260 185 192

74 51 85 90 60 82 63 50

69 44 85 90 50 72 61 34

1270.7 -

1017.1 -

-

130

75

86 91 83 85 102 90 94 121 123 97 97 125 113 90 99 76 75 71

60 77 67 74 70 74 103 84 98 102 83 86 109 92 77 74 86 68 70 59

107 143 104 133 85 74 66 71 54 64 54 60 44

62 39 35 65 53 56 48 47 45 29 59 31 38 40 34 24

28 90 95 36 51 58 62 50 46 54 48 61 45 26 30 21

AC C

EP

M AN U

CAUDALS MMS/VBN.93.31a (A) MMS/VBN.00.14 (A) MMS/VBN.00.15 (A) MMS/VBN.09.46 (A) MMS/VBN.09.54 (A) MMS/VBN.12.C.004 (A) MMS/VBN.09.D.011 (A-M?) MMS/VBN.12.B.018 (A-M?) MMS/VBN.09.D.009 (M?) MMS/VBN.12.B.013a (P) MMS/VBN.12.B.013b (P) MMS/VBN.09.D.03 (P) MMS/VBN.09.D.010 (P) MMS/VBN.09.159.b (P) MMS/VBN.12.C.003 (P) MMS/VBN.12.33 (P) UP/VBN.93.3 (P-D) UP/VBN.93.4 (P-D) UP/VBN.93.5 (P-D) UP/VBN.93.6 (D) UP/VBN.93.7 (D) UP/VBN.93.8 (D)

TE D

MMS/VBN.02.99 UP/VBN.09.157

120 200 210 118 100 78 90

3.91 3.98 2.29 2.22 3.10 3.26 4.13 6.47

-

275.7 -

-

57 70 40 68 41 36 48 23 25 35 33 30 19 24 16

51 32 22 50 17 14 21 7 21 14 9 0 7 3

2.14 0.86 0.71 2.06 1.37 1.28 1.65 1.66 1.87 2.02 1.92 1.26 1.64 2.62 2.33 2.81

SC

DORSALS

171 25 2050 147 185 102 126

RI PT

CERVICALS MMS/VBN.12.A.004 (A) MMS/VBN.12.B.015 (A) MMS/VBN.09.D.007a (A) UP/VBN.93.13a (M) UP/VBN.93.13b (M) MMS/VBN.12.B.10 (P) UP/VBN.93.12a (P) UP/VBN.93.12b (P) UP/VBN.93.12c (P)

EI

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Min. Cir. Diaph.

Max. width Prox.end

Max. width distal end

21 17

3.14 3.76

23.31 16.94

-

-

57.96

30.22

1.92

22.58

272

57

29

1.97

-

709

90.42

57.95

562

112

43

TIBIAE MMS/VBN.02.90 MMS/VBN.02.109

322 530

50.14 81.85

21.2 38.66

FIBULA MMS/VBN.09.132

221

47

390

RADIUS MMS/VBN.09.D.01

29

AC C

FEMORA MMS/VBN.00.12 MMS/VBN.09.126

SC

ULNA MMS/VBN.12.P.06a

M AN U

66 64

EP

555 480

RI PT

ECC

55.16

43.75

-

-

1.56 2.60

45.67 40.67

-

-

2.37 2.12

37.3 63.22

106.61 64.23

72 38.7

-

-

-

TE D

Preserved length Min. Transv. Width Min. AP Width HUMERI MMS/VBN.00.12 MMS/VBN.09.A.018

1.62

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AC C

EP

TE D

M AN U

SC

RI PT

Length AP width diaphisis LM width diaphisis AP width Prox. Art. LM width Prox. Art. AP width Dist. Art. LM width Dist. Art. MMS/VBN.93.09 87 13 17 22 32 MMS/VBN.09.113 180 14 27 23 60 27 43 UP/VBN.93.10 120 46 27 71 31 60 60

AC C

EP

TE D

M AN U

SC

RI PT

MANUSCRIPT Preserved length ACCEPTED PP articular surface Distal edge width MMS/VBN.09.51c 345 105

Preserved lentgh (mm) ±570 470 555

ACCEPTED MANUSCRIPT Bone tissue type 2ry osteon generations in the inner,mid,outer cortex respectively

Core location Posterior side, above the mid-shaft Posterior side, in the mid-shaft Anterior side, in the mid-shaft

H H H

5,6,4 5,5,6 4,5,4

AC C

EP

TE D

M AN U

SC

RI PT

A. velauciensis sample Bone MMS/VBN.09.126 Right femur MMS/VBN.09.A.018 Left humerus MMS/VBN.00.12 Right humerus

HOS,RS 14,13+ 14.14 14.13

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