This is the accepted version of the article: Matamales Andreu, Rafel; Roig Munar, Francesc X.; Oms, O.; [et al.]. «A captorhinid-dominated assemblage from the palaeoequatorial Permian of Menorca (Balearic Islands, western Mediterranean)». Earth and Environmental Science Transactions of the Royal Society of Edinburgh, Vol. 112, Issue 2 (June 2021), p. 125-145. DOI 10.1017/S1755691021000268 This version is available at https://ddd.uab.cat/record/250385 under the terms of the license A captorhinid-dominated assemblage from the palaeoequatorial Permian of Menorca (Balearic Islands, western Mediterranean) Rafel Matamales-Andreu1,2*, Francesc Xavier Roig-Munar3, Oriol Oms4, Àngel Galobart1,5 & Josep Fortuny1 1 Institut Català de Paleontologia Miquel Crusafont, Universitat Autònoma de Barcelona, Edifici ICTA-ICP, c/ Columnes s/n, Campus de la UAB, 08193 Cerdanyola del Vallès, Barcelona, Spain. 2 Museu Balear de Ciències Naturals, ctra. Palma-Port de Sóller km 30, 07100 Sóller, Mallorca, Illes Balears, Spain. 3 C/ Carritxaret 18-6, 07749 es Migjorn Gran, Menorca, Illes Balears, Spain. 4 Departament de Geologia, Universitat Autònoma de Barcelona, avda. de l’Eix Central s/n, Campus de la UAB, 08193 Cerdanyola del Vallès, Barcelona, Spain. 5 Museu de la Conca Dellà, c/ del Museu 4, 25650 Isona i Conca Dellà, Lleida, Spain. *Corresponding author. E-mail address: rafel.matamales@icp.cat. Abstract Moradisaurine captorhinid eureptiles were a successful group of high-fibre herbivores that lived in the arid low latitudes of Pangaea during the Permian. Here we describe a palaeoassemblage from the Permian of Menorca (Balearic Islands, western Mediterranean), consisting of ichnites of small captorhinomorph eureptiles, probably moradisaurines (Hyloidichnus) and parareptiles (cf. Erpetopus), and bones of two different taxa of moradisaurines. The smallest of the two is not diagnostic beyond Moradisaurinae incertae sedis. The largest one, on the other hand, shows characters that are not present in any other known species of moradisaurine (densely ornamented maxillar teeth), and it is therefore described as Balearosaurus bombardensis gen. et sp. nov. Other remains found in the same outcrop are identified as cf. Balearosaurus bombardensis gen. et sp. nov., as they could also belong to the newly-described taxon. This species is sister to the moradisaurine from the lower Permian of the neighbouring island of Mallorca, and is also closely related to the North American genus Rothianiscus. This makes it possible to suggest the hypothesis that the Variscan mountains, which separated North America from southern Europe during the Permian, were not a very important palaeobiogeographical barrier to the dispersion of moradisaurines. In fact, mapping all moradisaurine occurrences known so far, it is shown that their distribution area encompassed both sides of the Variscan mountains, essentially being restricted to the arid belt of palaeoequatorial Pangaea, where they probably outcompeted other herbivorous clades until they died out in the late Permian. Key Words: Captorhinidae, Moradisaurinae, Hyloidichnus, palaeobiogeography, central Pangaea Captorhinids were a clade of small to medium-sized early eureptiles that became widespread on Laurasia and Gondwana during the Permian. The earliest known member of the group, of small size and with a single-rowed dentition well suited for insectivory, lived in North America during the late Carboniferous (Müller & Reisz 2005; Reisz et al. 2016). Captorhinids radiated during the early Permian, maintaining small forms with a single row of teeth that likely fed on insects or even on smaller tetrapods (e.g., Brocklehurst 2017; Modesto et al. 2018 and references therein), which coexisted with other small to medium-sized forms that developed other food processing styles. Some of those species were omnivorous, with teeth arranged in a single row or with several rows of teeth oblique to the jaw margins (Modesto et al. 2007; LeBlanc & Reisz 2015; Brocklehurst 2017; Reisz et al. 2020), whereas others were high-fibre herbivores, always with multiple rows of teeth arranged more or less parallel to the jaw margins (Dodick & Modesto 1995; Reisz & Sues 2000; Modesto et al. 2014, 2019; LeBlanc et al. 2015; Brocklehurst 2017). This last group has been classified in a subfamily of their own, the Moradisaurinae Ricqlès & Taquet, 1982. Moradisaurines showed a wide range of sizes, from very small species with a skull length of about 25 mm (Olson 1970), to medium-sized species with a skull length of about 450 mm (Ricqlès & Taquet 1982; Modesto et al. 2019). All of them possessed tooth plates with several tooth rows on the dentary and on the maxilla, well suited for high-fibre herbivory (e.g., Dodick & Modesto 1995; Reisz & Sues 2000; LeBlanc et al. 2015). In fact, some representatives of both small and medium-sized forms have been inferred to be able to produce a propalinal motion of the lower jaw during food processing (Dodick & Modesto 1995; Modesto et al. 2007, 2014, 2019), which enabled them to efficiently grind and shred the plant material on which they fed. The number of rows and teeth per row were variable among the different species and throughout ontogeny (e.g., LeBlanc & Reisz 2015; Jung & Sumida 2017; Modesto et al. 2019). In the largest forms, the limb bones became distinctly more robust (e.g., Modesto et al. 2019), but not as much as theoretically expected (Romano & Rubidge 2019). In order to reduce the mechanical stress on the limb bones during locomotion, those herbivorous large forms probably moved more slowly (Romano & Rubidge 2019), which did not compromise their ability to obtain plant food, contrarily to smaller captorhinids, which needed to catch their prey. Ichnites attributed to captorhinomorphs that could be produced by moradisaurines, corresponding to the ichnogenus Hyloidichnus Gilmore, 1927, first appear in Sakmarian rocks (lower Permian) of North America (Lucas et al. 2013; Schneider, 2020), slightly earlier than the oldest known moradisaurines, which belong to the genus Captorhinikos Olson, 1954, reported from the Artinskian to the middle Kungurian (lower Permian) of North and South America (Cisneros et al. 2020a and references therein). The genus Captorhinikos is currently considered the most basal member and the first high-fibre herbivore of the clade (Brocklehurst 2017; Modesto et al. 2019). Larger herbivorous species started to appear shortly after, represented by the genera Labidosaurikos Stovall, 1950 (Kungurian, lower Permian: Dodick & Modesto 1995), Kahneria Olson, 1962a (Kungurian/Roadian?, lower/middle Permian: Olson 1962a) and Rothianiscus Kuhn, 1961 (Kungurian/Roadian?, lower/middle Permian: Olson 1962a), together with other undetermined specimens from southern North America (Kungurian, lower Permian: Modesto et al. 2016) and Mallorca (Artinskian–Kungurian?, lower Permian: Liebrecht et al. 2017; Matamales-Andreu et al. 2019). This also coincided with an increase in morphological disparity (Brocklehurst 2017), which may have played a part in the ecological success of the group, contributing to the shift to eureptile dominance in the post-Artinskian ichnoassemblages of both Europe and North America (Marchetti et al. 2015a, 2019a). There, the ichnogenus Hyloidichnus becomes abundant, and in rare cases, it is accompanied by another ichnogenus purportedly produced by large moradisaurines, Merifontichnus Gand et al., 2000 (Gand & Durand 2006; Marchetti 2016; Citton et al. 2019; Santi et al. 2020). In the middle–late Permian, moradisaurines appear represented by small-sized species in eastern Europe (Gecatogomphius Vjushkov & Chudinov, 1957, middle Permian: Ivakhnenko 2008), central-east Asia (Gansurhinus Reisz et al., 2011, middle–upper Permian: Reisz et al. 2011) and North Africa (Acrodenta Dutuit, 1976, and other unidentified moradisaurines, upper? Permian: Jalil & Dutuit 1996; Hmich et al. 2006), and the largest known species, in central Africa (Moradisaurus Taquet, 1969, middle– upper? Permian: Olroyd & Sidor 2017; Modesto et al. 2019). The most recent ichnites attributed to moradisaurines belong to the ichnogenus Hyloidichnus and were found in upper Permian rocks of North Africa (Voigt et al. 2010). As evidenced by some of the works cited above, the record of body fossils of moradisaurine captorhinid eureptiles in southern Europe was hitherto restricted to the island of Mallorca (Balearic Islands, western Mediterranean). Liebrecht et al. (2017) described a fragment of maxilla and parts of the palate of a large moradisaurine, which confirmed the presence of this clade on the island, previously inferred from tracks (Calafat et al. 1986, 1986–1987; Calafat 1988; Gand et al. 2010; Matamales-Andreu et al. 2019). Both the bones and the tracks were found in the Port des Canonge Unit, the age of which is at present unclear and under study, preliminarily dated as lower Permian (Artinskian or Kungurian) (Matamales-Andreu et al. 2019). Nevertheless, from the Permian beds of the neighbouring island of Menorca, some authors (Pretus & Obrador 1987; Carmona 2004) had also reported large bones of unidentified tetrapods, which had not been studied in detail so far. The first report of vertebrate remains on Menorca was published by Pretus & Obrador (1987), illustrating a large scapula found ex situ. That and other bones, herein revised, were the object of the preliminary work of Carmona (2004), who suggested that two of the fossil vertebrae belonged to a large and a small species of indeterminate seymouriamorphs. However, it is worth noting that Carmona (2004) did not consider all the bones that had been collected until then, because some of them had yet to be prepared. The present work resumes the study of tetrapod bone remains from the Permian of Cala del Pilar–Pla de Mar section (Menorca, Balearic Islands, western Mediterranean), re-assigning all of them to moradisaurine captorhinid eureptiles. This includes the detailed description of all the material present in old collections except for the scapula figured by Pretus & Obrador (1987), which is currently housed in a private collection and preparation required to properly study it has not been possible. Moreover, new ichnological material found at the outcrop is also studied. Unfortunately, new prospection/excavation campaigns have not been carried out due to administrative setbacks. Nevertheless, this study aims to shed light on the hitherto poorly described tetrapod fossils of this site, characterising a new locality of Permian palaeoequatorial faunas. 1. Geological and geographical context Menorca is the northeasternmost island of the Balearic Archipelago, located at the western Mediterranean. Even as an extension towards the NE of the Betic Orogen, Menorca is quite different from the rest of the Balearic Islands in structural and stratigraphic terms (Bourrouilh 1973; Vera et al. 2004; Sàbat et al. 2018). Geologically, the island is neatly divided into two main regions: Migjorn, at the S, where a post-orogenic upper Miocene cover is largely dominant; and Tramuntana, at the N, with older materials that broadly span from the Lochkovian (Lower Devonian) to the Rupelian (lower Oligocene) (Bourrouilh 1973, 1983; Vera et al. 2004; Martin- Closas & Ramos 2005) (Fig. 1A). The Permian red-beds studied in the present paper, framed between two erosive surfaces, lay within the latter structural unit. They are unconformably disposed over the underlying Devonian or Carboniferous rocks, and the top of their sequence is eroded and overlain by the Lower–Middle Triassic Buntsandstein facies (Gómez-Gras 1987, 1992, 1993; Rosell et al. 1988, 1989a, 1989b; Bercovici et al. 2009; Linol et al. 2009). Those beds were first attributed to the upper Permian by Bourrouilh (1973, 1983) and were subsequently studied by Pomar-Gomà (1979), Obrador (1983), Martí et al. (1985), Rodríguez-Perea et al. (1987), Arribas et al. (1990), Brandes & Tiedt (1991), Gómez-Gras (1987, 1992, 1993), Rosell et al. (1988, 1989a, 1989b), Broutin et al. (1992), Gómez-Gras & Alonso-Zarza (2003), Bercovici et al. (2009), Linol et al. (2009) and Borruel-Abadía et al. (2019). Despite of all these detailed works, the precise palaeogeographic position of Menorca before the Alpine orogeny is still a matter of discussion. During the late Carboniferous–early Permian, the extensional collapse of the Variscan orogen in Iberia and neighbouring regions opened many rift basins, which were filled with continental sediments until the Middle Triassic (López-Gómez et al. 2019a). Some authors (Gómez-Gras 1992, 1993; Sàbat et al. 2018) have argued that the Menorcan sections have a sedimentary evolution that is somewhat reminiscent to that of the basins of the SW of the Catalan Coastal Ranges, in the eastern margin of the Iberian Peninsula. However, the palaeocurrent directions of the Permian and Triassic of Menorca point generally towards the SW (Linol et al. 2009), whereas in the Iberian Peninsula the trend is towards the SE (López-Gómez & Arche 1987, 1992; Arche & López-Gómez 1992), and therefore it is unlikely that they were part of a same fluvial system or (sub)basin. The most probable scenario with the data available today is that the Menorcan basin was relatively independent from the other basins of Iberia, including that of the neighbouring island of Mallorca. In any case, the Menorcan basin was probably located very close to the equator throughout the Permian, approximately in a latitude of 4º N (Scotese 2014), at the western margin of the Palaeotethys ocean (Bercovici et al. 2009; Linol et al. 2009). The climate was tropical, alternating arid and hot seasons with rainy seasons (Gómez-Gras & Alonso-Zarza 2003; Bercovici et al. 2009; Roscher et al. 2011). Gómez-Gras (1987) described three lithostratigraphic units for the Permian of Menorca (informally named P1, P2 and P3), which were revised by Rosell et al. (1988, 1989a, 1989b), Gómez-Gras (1992, 1993), Bercovici et al. (2009) and Linol et al. (2009). For the present paper, one stratigraphic section has been logged in detail at the cliffs between Cala del Pilar and Pla de Mar (Fig. 1B–C; Supplementary Material 1), encompassing the three lithostratigraphic units. 1.1. Palaeoenvironment and climatic conditions The palaeoenvironments of the Permian recorded in Cala del Pilar–Pla de Mar section changed through time, responding to the evolution of the basin and its climatic conditions. A review of the three main lithostratigraphic units, based on the works of Gómez-Gras (1987, 1992, 1993), Rosell et al. (1988, 1989a, 1989b), Gómez-Gras & Alonso-Zarza (2003), Bercovici et al. (2009), Linol et al. (2009) and new data collected for the present study, is offered here: In the studied section, the P1 unit consists of 4–6 m of crudely bedded, coarse breccias with intercalated sandstones, overlaying the angular, erosive boundary with the Carboniferous Culm facies. In the first stages of rifting, when the subsidence rates are high, alluvial/colluvial fans transverse to the main axis of the basin usually develop near the footwall scarp (e.g., Speksnijder 1985; Miall 2006; Franzel et al. 2020 and references therein). The P1 unit is here interpreted as one of such deposits, and the formation of calcareous mature palaeosols on top of each of the breccia beds (Gómez-Gras & Alonso-Zarza 2003; Bercovici et al. 2009) attests that the depositional events that formed this unit were multiple, separated in time and under a climate with periods of very low precipitation (Gómez-Gras & Alonso-Zarza 2003). Apart from rhizocretions, no fossils have been reported from the P1 unit so far. In the studied section, the P2 unit consists of about 150 m of massive lutites with sporadic intercalations of sandstones with climbing ripples and, rarely, microbreccias of reworked pedogenic calcretes. This unit represents a playa lake palaeoenvironment (as defined by Briere 2000) in which lutites from overbank flows were deposited (Bercovici et al. 2009). Throughout the sequence, there is an alternation of 1–12 m-thick lutitic packs with 0.25–1.5 m-thick intervals that are more resistant to the erosion, with immature palaeosols and/or mud cracks. The former correspond to the deposition of fine sediments during high water table periods, whereas the latter reflect intervals of desiccation of the playa lakes and subsequent formation of mud cracks and incipient palaeosols. Appearing between those, there are sandstone and microbreccia beds with geometries ranging from lenticular (channelled flow) to tabular (unconfined flow), representing crevasse splays and sheetfloods that reworked the floodplains in sporadic heavy rain events (Gómez-Gras & Alonso-Zarza 2003). The fossil content of this unit consists of rhizocretions developed in different types of palaeosols (Bercovici et al. 2009), and bones and bone fragments that have been observed in a bed of reworked pedogenic calcrete fragments. The studied section also comprises the lower 170 m of the P3 unit, consisting of sandstones intercalated with lutites. The bases of the sandstone elements are usually erosive, with a lag of abundant reworked pedogenic calcretes from the floodplains (Gómez-Gras & Alonso- Zarza 2003). Sandstones are organised in two main sequence types: the first, with lateral accreting surfaces and a general upwards decrease of grain size, representing meandering channels, and the second, consisting mostly of tabular beds with horizontal, low-angle cross stratification or climbing ripple lamination, representing sheetflood deposits. Lutites are mostly massive and with a pervasive development of calcareous palaeosols (Bercovici et al. 2009). This unit represents a floodplain (playa, as per Briere 2000) with abundant vegetation under a seasonal climate. It was traversed by meandering rivers and, during the rainy seasons, unconfined sheetfloods covered the floodplain. One of the meandering channels, observed at m 301.5–303.5 of the studied section, corresponds to sandstone and breccia beds with abundant lignite lenses and plant debris. This channel was probably abandoned as an oxbow lake, where local reducing conditions favoured precipitation of copper minerals (Crespí & Merino 1998; Llull & Perelló 2013). Other areas of the floodplain were swamped or with a high water table for long time intervals, developing alfisols (Bercovici et al. 2009), which have been recognised in several beds of this unit. The most abundant fossils of the P3 unit are rhizocretions (Bercovici et al. 2009) and ichnofossils of the Scoyenia ichnofacies, including tetrapod tracks. Bones and bone fragments are also locally abundant as part of reworked pedogenic calcrete breccias. The uppermost part of the P3 unit, cropping out NW of Pla de Mar at Penyals d’Alforinet, has not been considered in the present study because it is separated from the lower part by a very thick covered interval, probably faulted and, moreover, no tetrapod fossils have been found there so far. It was studied in great detail by Bercovici et al. (2009) and Linol et al. (2009), and the palaeoenvironments there recorded are similar to those of the rest of the P3 unit. 2. Material and methods 2.1. Collection number abbreviations FMNH: Field Museum of Natural History, Chicago, Illinois, United States of America. IPS: Institut Català de Paleontologia Miquel Crusafont (formerly Institut de Paleontologia de Sabadell), Sabadell, Barcelona, Spain. MBCN: Museu Balear de Ciències Naturals, Sóller, Mallorca, Balearic Islands, Spain. MNHN: Muséum National d’Histoire Naturelle, Paris, France. MT: Macar de sa Teula, field code for the rock with the ichnites. It was left in the field (GPS coordinates: 40° 3'9"N 3°58'24"E). 2.2. ZooBank registration of new names New taxon names have been registered in ZooBank (http://zoobank.org) in order to comply with the rules of the International Code of Zoological Nomenclature for electronic publications (article 8.5.3). The LSID for this publication is: urn:lsid:zoobank.org:pub:8153E0E1-9B66-4C55-89B9- A246195DCD02. 2.3. Stratigraphy and sedimentology For the stratigraphic and sedimentological study, one section has been logged in situ, bed by bed, to a minimum resolution of 1 cm of bed thickness (in 1:25 scale), using a tape measure in well- exposed outcrops and a Jacobs staff for lutite, semi-covered and covered intervals. This section, named Cala del Pilar–Pla de Mar, is here presented in Supplementary Material 1 (in 1:40 scale), and a synthetic version is in Figure 1C (in 1:1160 scale). The recognised sedimentary lithofacies have been classified according to Miall (1985, 2006), Postma (1990), Mack et al. (1993), Gómez- Gras & Alonso-Zarza (2003), Bercovici et al. (2009) and Linol et al. (2009) (Supplementary Material 1). 2.4. Provenance and 3D modelling of tetrapod ichnofossils The tetrapod ichnites studied in the present work (MT01) were all preserved as natural casts on the surface of an ex situ rock found on the beach of Macar de sa Teula. The rock seemed freshly detached from its original bed, which was determined on the outcrop that had to be the one from m 174–179.5 (Fig. 1C), because both the bed and the ex situ rock had approximately the same thickness and consisted in very fine sandstones (somewhat silty) with abundant invertebrate burrows and common gleyed patches, unlike other nearby beds. Therefore, its position has been indicated in Figure 1C with a question mark. A photogrammetric 3D model of the ichnites was created (see ‘3. Systematic palaeoichnology’) and then the rock was left at the outcrop. Photogrammetry is a technique that has recently become widespread in ichnological studies (e.g., Falkingham 2012; Citton et al. 2016; Mujal et al. 2016a, 2020), making it possible to collect and save information that would otherwise be lost to erosion in the case of big, unmovable rock surfaces. Moreover, it provides an alternative to the confection of artificial casts, which are sometimes hard to make in open environments that are difficult to reach. The present study has broadly followed the same methodology as Mujal et al. (2016a, 2020 and references therein), using the open-source software MeshLab v2016.12 (http://meshlab.sourceforge.net/) and ParaView 5.5.0-RC4 64-bit (http://www.paraview.org) to process the meshes. However, to create the mesh, the licensed software Agisoft Photoscan standard v1.1.4. (www.agisoft.com) has been used instead. In order to produce the 3D model, 89 pictures of the surface of MT01 were taken from different angles and distances using a digital camera (Panasonic Lumix DMC-TZ27). Then, they were aligned, and the dense point cloud and the mesh were created. After that, a false- colour height map and contour lines were superimposed on the 3D model, and finally it was drawn on a vector-based graphics design software and measured using the open-source software ImageJ 1.52d (https://imagej.nih.gov/ij/), following the criteria of Leonardi (1987) and Hasiotis et al. (2007) (Table 1). The ichnites selected for study correspond to the category “1” of footprint preservation scale by Marchetti et al. (2019b), that is, relatively poorly-preserved ichnites missing some diagnostic structures (i.e., some digits). The other ichnites present on the slab scored a “0”, that is, their preservation was very poor (Marchetti et al. 2019b), so they could not be studied. The 3D models herein studied are archived and freely available in MorphoSource (https://www.morphosource.org/) with the following DOI: MT01-1 and MT01-2 (https://doi.org/10.17602/M2/M367858), MT01-10 (https://doi.org/10.17602/M2/M367864) and MT01-13 (https://doi.org/10.17602/M2/M367870). 2.5. Phylogenetic analysis The phylogenetic analysis was performed using a modified version (Supplementary Material 2) of the matrix of Cisneros et al. (2020a), mainly with changes introduced by Modesto et al. (2019) and Brocklehurst (2020). All character state changes for Captorhinikos chozaensis were applied following Modesto et al. (2019), except for their character ‘72’ (here character ‘73’) as there was no state 2 (see character list in Modesto et al. 2019). Character states for Moradisaurus were also recoded following Modesto et al. (2019). The rest of character state changes listed by Modesto et al. (2019) had already been applied in the matrix of Cisneros et al. (2020a). MBCN15730 (the moradisaurine from Mallorca) and Kahneria were added to the matrix with the character state codes of Brocklehurst (2020), modifying the following: character ‘10’ of the matrix used by Brocklehurst (2020) was redefined into two characters by Cisneros et al. (2020a), so they are now in both cases character ‘10’ with state 1 and character ‘11’ with state 1. Character ‘42’ of MBCN15730 (character ‘41’ in Brocklehurst 2020) was changed from 1 to ?, as the ventral side of the palatine is not visible on the specimen. Balearosaurus bombardensis gen. et sp. nov. and the other indeterminate small moradisaurine from Menorca studied in the present work have been coded first-hand. For the final analysis, both the indeterminate small moradisaurine from Menorca and MAP PV664 (Moradisaurinae indet.) from Brazil (Cisneros et al. 2020a) were removed because of their large amount of missing data, which caused significant polytomies in the Moradisaurinae. Phylogenetic analysis was run using PAUP* v.4.0 (Swofford 2003) as a branch- and-bound search with parsimony as the optimality criterion, unordered and unweighted characters and with branches collapsing when their maximum length was zero. Then, a strict consensus tree was computed, and bootstrap support values were calculated with 1000 repetitions, not showing values under 50. 3. Systematic palaeoichnology Ichnogenus Hyloidichnus Gilmore, 1927 Hyloidichnus isp. (Fig. 2A–D; Table 1) Studied material. MT01-1, MT01-2, MT01-3, MT01-4, natural cast of a partial trackway with a right manus pes set, a left pes imprint and a right pes imprint. MT01-5, natural cast of an isolated left manus imprint. MT01-10, natural cast of a left ?pes imprint. Most of the other footprints of the same surface (MT01-6, MT01-7, MT01-8, MT01-9, MT01-11, MT01-12) may also belong to this ichnogenus given their similar size and general shape but their preservation is too incomplete. All of them were found on an ex situ boulder at Macar de sa Teula, attributable to the m 174–179.5 of Cala del Pilar–Pla de Mar section, P3 Unit, indeterminate Permian, Menorca, Balearic Islands, western Mediterranean. Description. Pes imprints semiplantigrade, pentadactyl, probably slightly longer (26.4 mm) than wide. The most deeply imprinted parts are digits I and II (medial functional prevalence of the autopodia). The digit imprints radiate from the sole and are relatively slender and straight, with some tips ending in pointed claw traces. The relative length of the preserved digit imprints can be ordered as follows (MT01-1): I