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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Earth Sci.</journal-id>
<journal-title>Frontiers in Earth Science</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Earth Sci.</abbrev-journal-title>
<issn pub-type="epub">2296-6463</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="publisher-id">672229</article-id>
<article-id pub-id-type="doi">10.3389/feart.2021.672229</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Earth Science</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>Changes in Cave Sedimentation Mechanisms During the Late Quaternary: An Example From the Lower Cerova&#x10d;ka Cave, Croatia</article-title>
<alt-title alt-title-type="left-running-head">Kure&#x10d;i&#x107; et&#x20;al.</alt-title>
<alt-title alt-title-type="right-running-head">Cave Sediments in Dinaric Karst</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname>Kure&#x10d;i&#x107;</surname>
<given-names>Tomislav</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1246924/overview"/>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Bo&#x10d;i&#x107;</surname>
<given-names>Neven</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1041421/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Wacha</surname>
<given-names>Lara</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1279605/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Bakra&#x10d;</surname>
<given-names>Koraljka</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1279585/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Grizelj</surname>
<given-names>Anita</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1281074/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Tresi&#x107; Pavi&#x10d;i&#x107;</surname>
<given-names>Dinko</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>L&#xfc;thgens</surname>
<given-names>Christopher</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Sironi&#x107;</surname>
<given-names>Andreja</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Radovi&#x107;</surname>
<given-names>Sini&#x161;a</given-names>
</name>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1279776/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Redovnikovi&#x107;</surname>
<given-names>Loris</given-names>
</name>
<xref ref-type="aff" rid="aff7">
<sup>7</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Fiebig</surname>
<given-names>Markus</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
</contrib-group>
<aff id="aff1">
<label>
<sup>1</sup>
</label>Department of Geology, Croatian Geological Survey, <addr-line>Zagreb</addr-line>, <country>Croatia</country>
</aff>
<aff id="aff2">
<label>
<sup>2</sup>
</label>Department of Geography, Division of Physical Geography, Faculty of Science, University of Zagreb, <addr-line>Zagreb</addr-line>, <country>Croatia</country>
</aff>
<aff id="aff3">
<label>
<sup>3</sup>
</label>Kaducej d.o.o., <addr-line>Split</addr-line>, <country>Croatia</country>
</aff>
<aff id="aff4">
<label>
<sup>4</sup>
</label>Institute of Applied Geology, University of Natural Resources and Life Sciences (BOKU), <addr-line>Vienna</addr-line>, <country>Austria</country>
</aff>
<aff id="aff5">
<label>
<sup>5</sup>
</label>Laboratory for Low-level Radioactivities, Division of Experimental Physics, Ru&#x111;er Bo&#x161;kovi&#x107; Institute, <addr-line>Zagreb</addr-line>, <country>Croatia</country>
</aff>
<aff id="aff6">
<label>
<sup>6</sup>
</label>Institute for Quaternary Palaeontology and Geology, Croatian Academy of Sciences and Arts, <addr-line>Zagreb</addr-line>, <country>Croatia</country>
</aff>
<aff id="aff7">
<label>
<sup>7</sup>
</label>Department of Applied Geodesy, Faculty of Geodesy, University of Zagreb, <addr-line>Zagreb</addr-line>, <country>Croatia</country>
</aff>
<author-notes>
<fn fn-type="edited-by">
<p>
<bold>Edited by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/636507/overview">Aurel Per&#x015F;oiu</ext-link>, Romanian Academy, Romania</p>
</fn>
<fn fn-type="edited-by">
<p>
<bold>Reviewed by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/268617/overview">Andrea Zerboni</ext-link>, University of Milan, Italy</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/751101/overview">Christos Pennos</ext-link>, University of Bergen, Norway</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Neven Bo&#x10d;i&#x107;, <email>nbocic@gmail.com</email>
</corresp>
<fn fn-type="other">
<p>This article was submitted to Quaternary Science, Geomorphology and Paleoenvironment, a section of the journal Frontiers in Earth Science</p>
</fn>
</author-notes>
<pub-date pub-type="epub">
<day>30</day>
<month>06</month>
<year>2021</year>
</pub-date>
<pub-date pub-type="collection">
<year>2021</year>
</pub-date>
<volume>9</volume>
<elocation-id>672229</elocation-id>
<history>
<date date-type="received">
<day>25</day>
<month>02</month>
<year>2021</year>
</date>
<date date-type="accepted">
<day>15</day>
<month>06</month>
<year>2021</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2021 Kure&#x10d;i&#x107;, Bo&#x10d;i&#x107;, Wacha, Bakra&#x10d;, Grizelj, Tresi&#x107; Pavi&#x10d;i&#x107;, L&#xfc;thgens, Sironi&#x107;, Radovi&#x107;, Redovnikovi&#x107; and Fiebig.</copyright-statement>
<copyright-year>2021</copyright-year>
<copyright-holder>Kure&#x10d;i&#x107;, Bo&#x10d;i&#x107;, Wacha, Bakra&#x10d;, Grizelj, Tresi&#x107; Pavi&#x10d;i&#x107;, L&#xfc;thgens, Sironi&#x107;, Radovi&#x107;, Redovnikovi&#x107; and Fiebig</copyright-holder>
<license xlink:href="http://creativecommons.org/licenses/by/4.0/">
<p>This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these&#x20;terms.</p>
</license>
</permissions>
<abstract>
<p>During archeological excavations in the Lower Cerova&#x10d;ka Cave (Mt. Velebit, Croatia), the test trench penetrated to a depth of 1.8&#xa0;m. An undisturbed sequence of sediments was exposed. Considering that caves represent highly efficient sediment traps it was possible to recognize changes in the depositional mechanisms during the Pleistocene&#x2013;Holocene period. Using the multiproxy approach, the mineralogical, petrographic, and biostratigraphic characterization of the cave sediments was performed. Facies analysis revealed several stages in the development of the clastic filling of cave channels. Allochthonous origin of the sediment was assumed. Sedimentation took place under various conditions from pronounced cold and dry climate during Pleistocene stages in the base of the profile, to humid periods with anthropogenic influence during the Holocene at the very top of the profile. Although traditionally these sediments were believed to be of a Pleistocene age, here for the first time a stratigraphic calibration of the profile has been performed based on luminescence dating of detrital cave sediments and radiometric dating of speleothems.</p>
</abstract>
<kwd-group>
<kwd>cave sediments</kwd>
<kwd>facies analysis</kwd>
<kwd>provenance</kwd>
<kwd>numerical dating</kwd>
<kwd>palynofacies</kwd>
<kwd>
<italic>Ursus spelaeus</italic>
</kwd>
<kwd>Dinaric karst</kwd>
</kwd-group>
</article-meta>
</front>
<body>
<sec id="s1">
<title>Introduction</title>
<p>Situated in the locus typicus of the Dinaric karst (<xref ref-type="bibr" rid="B147">Zupan Hajna, 2019</xref>) within the NE slopes of Mt. Crnopac (SE part of the Velebit massif in Croatia) (<xref ref-type="fig" rid="F1">Figures 1A,B</xref>), the Cerova&#x10d;ke Caves represent a network of subhorizontal hydrologically inactive cave channels (<xref ref-type="fig" rid="F2">Figures 2A,B</xref>) in today&#x2019;s vadose zone. There are three Cerova&#x10d;ke caves, namely Lower, Middle and Upper Cerova&#x10d;ka Cave (LCC, MCC and UCC). LCC was discovered in 1913 (<xref ref-type="bibr" rid="B75">Malez, 1956</xref>, <xref ref-type="bibr" rid="B74">1958</xref>) during the construction of the railroad. The caves have been the focus of research for many speleologists and other geoscientists ever since. Because of the scientific interest, as well as exploitation interest related to the geo-heritage and tourist potential of the cave, intensive cave surveying was conducted, combined with paleontological and archaeological excavations. That research gave insight into the rich cave history, as evidenced by findings of large Pleistocene fossil mammals (<xref ref-type="bibr" rid="B78">Malez, 1960a</xref>; <xref ref-type="bibr" rid="B76">1965a</xref>). Consequently, excavation campaigns resulted in the first available data of cave channel sediment infill and provenance of cave detrital sediments (e.g., <xref ref-type="bibr" rid="B55">Ivanovi&#x107; et&#x20;al., 1976</xref>). First interpretations suggest that these sediments represent products of host rock weathering, deposited after the caves lost their ponor (swallow hole) function during the uplift of the mountain and lowering of the Gra&#x10d;ac karst polje level (<xref ref-type="bibr" rid="B77">Malez, 1965b</xref>).</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>
<bold>(A)</bold> Geographic position of the Cerova&#x10d;ke Caves, <bold>(B)</bold> Elevation map of the surrounding area, legend: 1&#x2014;surface streams with ponors, 2&#x2014;cave chanells of Lower and Upper Cerova&#x10d;ka Cave, 3&#x2014;entrance positions of Lower (LCC) and Upper (UCC) Cerova&#x10d;ka Cave, <bold>(C)</bold> Geological map of the surrounding area, sources: Geological map of Croatia 1:300.000 (<xref ref-type="bibr" rid="B23">Croatian Geological Survey, 2009</xref>), Basic geological map of Croatia 1:100.000, sheet Obrovac (<xref ref-type="bibr" rid="B54">Ivanovi&#x107; et&#x20;al., 1973</xref>), Basic geological map of Croatia 1:100.000, sheet Udbina (<xref ref-type="bibr" rid="B121">&#x160;u&#x161;njar et&#x20;al., 1973</xref>), legend: 1&#x2014;clastic rocks (C, P), 2&#x2014;carbonate rocks (T<sub>2</sub>), 3&#x2014;clastic-pyroclastic rocks (T<sub>3</sub>), 4&#x2014;dolomites (T<sub>3</sub>), 5&#x2014;limestones and dolomites (J<sub>1</sub>), 6&#x2014;thick layered limestones and dolomites (J<sub>2</sub>), 7&#x2014;limestones and dolomites (J<sub>3</sub>), 8&#x2014;carbonate (Jelar) breccia (Pg, Ng), 9&#x2014;alluvial deposits (Q), 10&#x2014;Terra Rossa (Q), 11&#x2014;faults, LF&#x2014;Lika fault.</p>
</caption>
<graphic xlink:href="feart-09-672229-g001.tif"/>
</fig>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>
<bold>(A)</bold> Simplified plan view of the Upper and Lower Cerova&#x10d;ka Cave, <bold>(B)</bold> plan view of the entrance part of the Lower Cerova&#x10d;ka Cave with the marked position of the researched test trench (cave survey according <xref ref-type="bibr" rid="B11">Bo&#x10d;i&#x107; et&#x20;al., 2016</xref>), <bold>(C)</bold> selected cross-sections (1&#x2013;4), and <bold>(D)</bold> cross-section of the cave channel at the location of the test trench.</p>
</caption>
<graphic xlink:href="feart-09-672229-g002.tif"/>
</fig>
<p>In recent years, the interest in revitalizing the tourist potential of the LCC intensified. Following requirements prescribed by the Conservation Department in Zadar (Croatia), new archaeological research in the LCC was conducted during 2019. Excavations included the area of the cave with archaeological potential, endangered by construction works along the new visitor pathway. The main archaeological excavation area was placed along the route of the new pathway, spanning 120&#xa0;m from entrance. Three distinctive phases of human occupation were determined within the excavation sites of the LCC, above the geological record (<xref ref-type="bibr" rid="B128">Tresi&#x107; Pavi&#x10d;i&#x107;, 2020</xref>). The latest phase is attributed to the modern period, from the discovery of the cave in 1913 until today, and includes various features such as existing pathway, trenches for electrical cables and archaeological and geological test trenches from previous excavations. The medieval phase within the cave was represented by a small number of finds dated to the 13th century (<xref ref-type="bibr" rid="B128">Tresi&#x107; Pavi&#x10d;i&#x107;, 2020</xref>) when the cave was used sporadically, probably as a shelter. The earliest and archeologically most significant phase of human occupation represented in the excavated area, corresponds to features and finds from the Late Bronze Age period which in the area of Lika roughly corresponds to the period from the 14th to 10th century BC (<xref ref-type="bibr" rid="B10">Ble&#x10d;i&#x107;-Kavur, 2014</xref>; <xref ref-type="bibr" rid="B6">Bakari&#x107;, 2017</xref>). The data collected suggest that the cave was used for food storage and as a temporary dwelling in specific circumstances such as extreme weather conditions during the Late Bronze Age. The archaeological remains are numerous and well documented. However, there has been a significant lack of any new geological research within the cave since the seventies.</p>
<p>The sediment profile (DC-SP) investigated within our research is situated within a test trench placed 120&#xa0;m from the cave entrance at the end of archaeological excavation area (<xref ref-type="fig" rid="F2">Figure&#x20;2B</xref>). Since the test trench penetrated to a depth of 1.8&#xa0;m, an undisturbed sequence of sediments was exposed. At the site, the Late Bronze Age and Modern Period features were found within the investigated profile (<xref ref-type="fig" rid="F3">Figure&#x20;3A</xref>). However, the majority of the profile represents geological strata of unknown origin and age. The aim of this study, therefore, is to determine the provenance of sediments, and the type and degree of changes in the environment during the time of deposition of clastic cave sediments within the main channel of the LCC. A multiproxy research approach was applied to the sediment including detailed sedimentological and mineralogical analysis. The lithofacies analysis of the detrital cave sediments was used to answer questions regarding the deposition mechanisms in specific conditions during the Pleistocene. Mineralogical analyzes are applied to get insight into the provenance of the cave sediments. Macropaleontological analysis was performed for a detailed determination of the excavated fossil bones as well as palynological analysis to determine the palynofacies. To establish the time frame and stratigraphic calibration of the investigated profile, luminescence dating of detrital cave sediments was performed and supported with radiometric dating of speleothems found within the sediment sequence. Furthermore, a comparison with available data on similar (spatio-temporal) sedimentary profiles will be&#x20;given.</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>Sedimentary log and photo of the investigated profile DC-SP within the archaeological excavation site in the Lower Cerova&#x10d;ka Cave <bold>(A)</bold> Sedimentary log with indicated main structural and lithological features, <bold>(B)</bold> photo of profile and indicated position of sampling spots (on the left side&#x2014;bulk analysis of described intervals; on the right side&#x2014;high-resolution granulometric analyses).</p>
</caption>
<graphic xlink:href="feart-09-672229-g003.tif"/>
</fig>
</sec>
<sec id="s2">
<title>Geological and Geomorphological Setting</title>
<p>Velebit Mt. is a part of the Dinaric mountain system and the longest mountain range in Croatia (<xref ref-type="fig" rid="F1">Figure&#x20;1A</xref>). Cerova&#x10d;ke Caves are located on the northern slope of its extreme southeastern part, Crnopac (<xref ref-type="fig" rid="F1">Figure&#x20;1B</xref>). To the north of Crnopac lies the Gra&#x10d;ac karst polje. In the structural-geological sense, the area of the Gra&#x10d;ac polje forms an anticline with Paleozoic clastites in their core. Around them Mesozoic sediments spread periclinally (<xref ref-type="bibr" rid="B116">Soka&#x10d; et&#x20;al., 1976</xref>; <xref ref-type="bibr" rid="B121">&#x160;u&#x161;njar et&#x20;al., 1973</xref>; <xref ref-type="bibr" rid="B54">Ivanovi&#x107; et&#x20;al., 1973</xref>, <xref ref-type="bibr" rid="B55">1976</xref>). Triassic dolomites and clastites and Jurassic dolomites predominate at the surface. The youngest are Quaternary Terra Rossa and alluvial deposits recorded at the bottom of the polje (see <xref ref-type="fig" rid="F1">Figure&#x20;1C</xref> for details). This lithology causes the bottom of the Gra&#x10d;ac polje to act as a hydrogeological barrier. A surface drainage network has developed on its surface with a general drainage direction to the south. The main stream is the Otu&#x10d;a River, which forms a ponor zone in the southern, deepest part of the field (<xref ref-type="fig" rid="F1">Figures 1B,C</xref>). The Otu&#x10d;a drainage system superficially drains an area of about 90&#xa0;km<sup>2</sup> as well as the underground karst water that converges to the polje from the surrounding hills. The lowest point of the field is at an elevation of 544&#xa0;m. South of the Gra&#x10d;ac polje rises the Crnopac massif (1,404&#xa0;m), separated by the Lika fault (<xref ref-type="fig" rid="F1">Figures 1B,C</xref>). Crnopac is a part of the main ridge and tectonic unit Velebit. Its structure is dominated by Jurassic and Cretaceous carbonate rocks separated by paleo-relief boundaries from overlaying Paleogene carbonate breccias (<xref ref-type="bibr" rid="B54">Ivanovi&#x107; et&#x20;al., 1973</xref>, <xref ref-type="bibr" rid="B55">1976</xref>) known as Jelar breccia (<xref ref-type="bibr" rid="B3">Bahun, 1963</xref>, <xref ref-type="bibr" rid="B4">1974</xref>). Areas built up of Jelar breccias like the Northern Velebit are intensively karstified, with a large number of dolines and deep caves, including Lukina jama, the deepest cave in the Dinarides (<xref ref-type="bibr" rid="B13">Bo&#x10d;i&#x107; et&#x20;al., 2019</xref>). Similar to the Northern Velebit, the Crnopac area is also extremely karstified. The area is characterized by large, steep, and numerous dolines whose maximum density reaches 93 dolines per km<sup>2</sup> (<xref ref-type="bibr" rid="B81">Markovi&#x107; et&#x20;al., 2016</xref>). More than 200 caves have been explored in the area, the largest of which is the Crnopac Cave System (CCS) (<xref ref-type="bibr" rid="B7">Bari&#x161;i&#x107;, 2017</xref>), which is the longest cave in the Dinarides and 67th longest cave in the world, measuring 53.3&#xa0;km in length (<xref ref-type="bibr" rid="B21">Caver Bob, 2021</xref>; <xref ref-type="bibr" rid="B24">Croatian Mountaineering Association, 2021</xref>).</p>
<p>Sinking waters from the Gra&#x10d;ac polje flow underground through the Crnopac massif toward the south, to the valleys of the Krupa and Zrmanja rivers. These allogenic flows influence the formation of cave systems. Due to the uplifting of the Crnopac massif cave channels form at several levels. The speleogenesis of the Crnopac massif is also influenced by autogenous water, which has a vertical circulation through a deep unsaturated zone (<xref ref-type="bibr" rid="B64">Kuhta and Stroj, 2005</xref>).</p>
<p>This area has the climate type Cfb (temperate humid with warm summer) (<xref ref-type="bibr" rid="B34">Filip&#x10d;i&#x107;, 1998</xref>). Basic climatological characteristics of the area are visible through the basic data of the Gra&#x10d;ac meteorological station for the period 2004&#x2013;2014: (i) the average annual air temperature is 9.9&#xb0;C and the mean annual precipitation is 1,960&#xa0;mm and (ii) the warmest month is July (19.9&#xb0;C), but the highest mean monthly precipitation is in December (283&#xa0;mm) (<xref ref-type="bibr" rid="B26">Czuppon et&#x20;al., 2018</xref>).</p>
<p>All three known caves at the investigated site (UCC 4,035&#xa0;m, LCC 4,048&#xa0;m, MCC, 390&#xa0;m long) are located in the ponor (input) zone of the Crnopac karst system above the level of the karst polje, i.e.,&#x20;the currently active ponors. All three caves are formed in Paleogene carbonate (Jelar) breccias (<xref ref-type="fig" rid="F1">Figures&#x20;1B,C</xref>).</p>
<p>The LCC is a predominantly horizontal branchwork cave (sensu <xref ref-type="bibr" rid="B95">Palmer, 1991</xref>). The entrance altitude is 630&#xa0;m, i.e.,&#x20;about 80&#xa0;m higher than the active ponors at the edge of the karst polje. The cave can be morphologically divided into two parts. In the northern part, the channels run mainly in NW-SE direction, following the main fold and thrust belt direction of the External Dinarides (<xref ref-type="bibr" rid="B123">Tari, 2002</xref>; <xref ref-type="bibr" rid="B110">Schmid et&#x20;al., 2008</xref>; <xref ref-type="bibr" rid="B57">Korbar, 2009</xref>). Here the channels are relatively narrower and rarely exceed 5&#xa0;m. In the southern part of the cave, which extends toward the SW, the channels are much wider and often exceed 10&#xa0;m in width (<xref ref-type="fig" rid="F2">Figure&#x20;2A</xref>). The formation of the cave is most likely related to the function of the karst conduit of sinking waters from the Gra&#x10d;ac karst polje. The investigated test trench is located in the main channel at a distance of about 120&#xa0;m from the entrance, measures about 3&#x20;&#xd7; 3&#xa0;m in plan and is 1.8&#xa0;m deep (<xref ref-type="fig" rid="F2">Figure&#x20;2B</xref>).</p>
</sec>
<sec sec-type="materials|methods" id="s3">
<title>Materials and Methods</title>
<p>The cave survey was the starting point to obtain data on the morphology of the cave. The part of the cave open for visitors (about 700&#x20;m long) was surveyed at a scale of 1: 200, the rest of the cave at a scale of 1: 500. The survey was made in the UIS-5-4-BC mapping grade (<xref ref-type="bibr" rid="B43">H&#xe4;uselmann, 2011</xref>). A standard procedure was used to determine the relative position of survey points by measuring the distance, azimuth and inclination angle. The Leica hand laser distometer and Suunto clino-compas were used. The starting point outside the cave was stabilized with a GNSS receiver. Additional data on the morphology of the investigated part of the cave were obtained by laser scanning. The first laser scanning of LCC was performed in the period from January 15 to 17, 2016. At that time, two geodetic bases were established, one in front of and the second inside of the cave. The Faro Focus3D X 330 laser scanner, the Topcon HiPer SR GNSS receiver and two total stations (TOPCON GTS 105N and Cygnus 2LS) were used for the geodetic survey of the LCC. The laser scanning was performed again on June 13th and 14th, 2019. but this time strong lighting was used and panoramic 360&#xb0; photographs were collected during the scan to obtain a colored point cloud. Point clouds obtained by the photogrammetric method during archaeological research are connected to the new colored point cloud and presented within this paper as 3D supplement (<xref ref-type="sec" rid="s10">Supplementary Material S1</xref>). Leica Cyclone 3DR software was used to visualize the obtained data and to create a characteristic profile.</p>
<p>Archaeological excavations were carried out with hand tools following stratigraphic principles, and standard archaeological field records were kept. A detailed catalog of methods and archaeological findings is given by <xref ref-type="bibr" rid="B129">Tresi&#x107; Pavi&#x10d;i&#x107; and Burmaz (2020)</xref> and <xref ref-type="bibr" rid="B128">Tresi&#x107; Pavi&#x10d;i&#x107; (2020)</xref>. Sedimentological field data and sampling were acquired within the archaeological test trench.</p>
<p>For a detailed sedimentological analysis individual layers and lithofacies units were recognized below the archaeological layer (<xref ref-type="fig" rid="F3">Figure&#x20;3A</xref>). The nomenclature for the established lithofacies units was based on <xref ref-type="bibr" rid="B16">Bosch and White (2004)</xref>. All layers were sampled (<xref ref-type="fig" rid="F3">Figure&#x20;3B</xref>). The grain-size of the sediment was determined on five bulk samples from each observed lithological unit using the areometric method (<xref ref-type="fig" rid="F3">Figure&#x20;3B</xref>; Samples DC-SP 2, 3, 5, 6, 7) while high-resolution grain-size (in 10&#xa0;cm resolution) was determined using the laser diffraction method. A total of 14 samples were analyzed with a Shimadzu Laser Diffraction Particle Size Analyzer SALD-2300 to determine the detailed dynamics of vertical changes in the particle size distribution (<xref ref-type="fig" rid="F3">Figure&#x20;3B</xref>; Samples DC-SP 35&#x2013;165&#xa0;cm). 0.1&#xa0;g of a dry representative sample was isolated for the analysis. The samples were treated with a 4% solution of tetra-sodium diphosphate decahydrate (Na<sub>4</sub>P<sub>2</sub>O<sub>7</sub>&#xb7;10H<sub>2</sub>O) and deionized water against coagulation and dispersed for at least 6&#xa0;h on a shaker. Each measurement was repeated five times and an average value was used for the grain-size distribution. The sediment was classified according to <xref ref-type="bibr" rid="B127">Trefethen (1950)</xref>.</p>
<p>To get insight in the composition of the sediment and determine the provenance of the material, the modal (heavy and light minerals) and XRPD analyses were performed. For the separation of heavy and light minerals, the 0.09&#x2013;0.16&#xa0;mm fraction of five samples was used (<xref ref-type="fig" rid="F3">Figure&#x20;3B</xref>; Samples DC-SP 2, 3, 5, 6, 7). Samples were treated with 10% HCl to remove the carbonates, and washed with H<sub>2</sub>0 in an ultrasonic bath. The grains were separated using sodium polytungstate (<italic>&#x3c1;</italic> &#x3d; 2.8&#xa0;g&#xa0;cm<sup>&#x2212;3</sup>). Thin slides were prepared from the separated material, and the composition was determined by counting up to 300 grains per sample using a Leitz Orthoplan polarizing microscope (<xref ref-type="bibr" rid="B151">Mange and Maurer, 1992</xref>). Typical mineral groups were isolated and their characteristics and relative proportions in the samples were described. Due to the low content of transparent heavy minerals (THM) within the heavy mineral fraction (HMF), real percentages and statistical analysis are not&#x20;shown.</p>
<p>The mineral composition of seven cave sediment samples and a bone fragment were determined by X-ray powder diffraction (XRPD) (<xref ref-type="fig" rid="F3">Figure&#x20;3B</xref>; Samples DC-SP 1-bone, 1-7-sediment). The samples were grinded, sieved through a 0.063&#xa0;mm sieve and the &#x3c;2&#xa0;&#xb5;m fraction was separated using the centrifuge method (<xref ref-type="bibr" rid="B63">Krumm, 1994</xref>). Oriented mounts from &#x3c;2&#xa0;&#xb5;m fraction were prepared. Oriented samples were treated with following treatments: a) air drying, b) saturation with K<sup>&#x2b;</sup> c) saturation with Mg<sup>2&#x2b;</sup> d) Mg<sup>2&#x2b;</sup> saturation and ethylene-glycol solvation, e) K<sup>&#x2b;</sup> saturation and ethylene-glycol solvation, f) Mg<sup>2&#x2b;</sup> saturation and glycerol solvation, g) K<sup>&#x2b;</sup> saturation and DMSO solvation, h) heating more than &#xbd; hour to 400 and 550&#xb0;C, i) treating with HCl (18%, 24&#xa0;h) (<xref ref-type="bibr" rid="B137">Weaver, 1967</xref>; <xref ref-type="bibr" rid="B118">Starkey et&#x20;al., 1984</xref>; <xref ref-type="bibr" rid="B89">Moore and Reynolds, 1997</xref>) and XRD patterns were recorded. The measurements were performed using the Philips vertical goniometer (type X`Pert) equipped with a Cu tube under the following experimental conditions: 45&#xa0;kV, 40&#xa0;mA, PW 3018/00 PIXcel detector, primary beam divergence 1/4&#xb0;, continuous scan (step 0.02&#xb0;2&#x3b8;/s). The interpretation of XRPD was obtained using <xref ref-type="bibr" rid="B45">HIGH SCORE PLUS (2016)</xref> calculation and <xref ref-type="bibr" rid="B97">PDF-4 / Minerals (2020)</xref> databases. The semi-quantitative analysis was performed using the procedure described by <xref ref-type="bibr" rid="B111">Schultz (1964)</xref>.</p>
<p>Palynological analyses were carried out on four samples collected from the lower and upper part of the section (<xref ref-type="fig" rid="F3">Figure&#x20;3B</xref>; Samples DC-SP 1, 2, 7, 8). Standard palynological processing techniques were used to extract the organic matter (e.g., <xref ref-type="bibr" rid="B90">Moore et&#x20;al., 1991</xref>; <xref ref-type="bibr" rid="B144">Wood et&#x20;al., 1996</xref>). The samples were treated with 4% solution of tetra-sodium diphosphate decahydrate (Na<sub>4</sub>P<sub>2</sub>O<sub>7</sub>&#xb7;10H<sub>2</sub>O) against coagulation, cold HCl (15%) and HF (40%), removing carbonates and silica, respectively. Heavy liquid (ZnCl<sub>2</sub>, <italic>&#x3c1;</italic> &#x3e; 2.1&#x20;kg/l) was used to separate the organic matter from the undissolved inorganic components. The organic residue was sieved through a 10&#xa0;&#xb5;m mesh. For palynofacies analysis slides were mounted in glycerin and, for palynomorphs analysis in&#x20;silicon oil. Microscopic analyses were performed using the Olympus BH-2 and Leica DM2500 microscope (Croatian geological survey). Photomicrographs were taken using an AmScopeTM camera adapter connected to the AmScope v.3.7 camera software and Leica MC190 HD camera connected to the Leica LAS EZ software. The palynofacies analyses were performed according to the classifications proposed by <xref ref-type="bibr" rid="B130">Tyson (1995)</xref> and <xref ref-type="bibr" rid="B112">Sebag et&#x20;al. (2006)</xref>. Three categories of organic matter (OM) were used: (1) phytoclasts: opaque phytoclasts (OP) and ligno-cellulosic debris (LcD), which can be preserved as cuticles and membranes (CM), transparent (TLC), altered (ALC), amorphous (AP) or gelified particles (GP), (2) Amorphous organic matter (AOM) and (3) palynomorphs. Minimum 500 particles of OM were counted per sample. Results were plotted in OM percentage abundance diagram and diagram presenting the relation between preserved/transformed phytoclasts and AOM to characterize the palaeoenvironment.</p>
<p>Macropaleontological analyses were performed on faunal remains collected during the research. The material was dry sieved on site using a mesh size of 6&#x20;&#xd7; 6 mm, bagged and named. In the laboratory the faunal remains were washed and dried and a detailed palaeontological analysis was conducted at the Institute for Quaternary Palaeontology and Geology in Zagreb. During the anatomical and taxonomical analysis, the fossil remains were compared with the fossil and recent comparative collection stored at the Institute. This was followed by a detailed taphonomic study. All bone and teeth fragments were carefully examined with a hand lens (&#xd7;10 magnification) looking for any bone modifications that could indicate butchery, gnawing, and other taphonomic traces as direct indicators of different agencies responsible for the accumulation and preservation of the skeletal material. Due to a relatively modest number of identified remains (873), taxonomic representation and element frequency were quantified using NISP (Number of Identified Specimens; <xref ref-type="bibr" rid="B73">Lyman, 1994</xref>).</p>
<p>The luminescence dating method was applied on two cave sediment samples to establish a chronological framework of the deposits (<xref ref-type="fig" rid="F3">Figure&#x20;3B</xref>; Samples DC-SP 3 and 7). The samples were taken using stainless steel cylinders driven into the freshly cleaned sediment and sealed light tight after sampling. Additional samples for radionuclide determination were taken in the direct surroundings of the luminescence samples. During sample preparation, the ends of the cores were removed, because of potential light exposure during sampling. Since detrital cave sediments as water-lain sediments are known to be prone to incomplete bleaching (insufficient light exposure of the sediment during transport and before burial), the obtained ages are often overestimated. In luminescence dating, reliable methods for the detection and correction of the effects of incomplete bleaching are available. However, a basic restriction is that measurements have to be conducted on subsamples (aliquots) containing only small numbers of grains, ideally down to the single grain level. For that reason, single quartz and potassium-rich feldspar grains (usually between 63&#x2013;300&#xa0;&#xb5;m) were extracted from the collected samples. Sample preparation and measurements were conducted at the Vienna Laboratory for Luminescence dating (VLL) using standard methods (<xref ref-type="bibr" rid="B72">L&#xfc;thgens et&#x20;al., 2017</xref>; <xref ref-type="bibr" rid="B102">Rades et&#x20;al., 2018</xref>). After sample preparation, no significant amount of coarse grains could be extracted from sample DC-SP 7 (VLL-0496-L), while a minimal number amount of coarse grains could be retrieved from sample DC-SP 3 (VLL-0495-L). All subsequent analyses could therefore only be conducted for the latter sample. In contrast to potassium-rich feldspar, it is known that only a small fraction of quartz grains (usually &#x3c;10%, but frequently also down to only few percent) does emit a luminescence signal suitable for dating (e.g., <xref ref-type="bibr" rid="B71">L&#xfc;thgens et&#x20;al., 2011</xref>). Given the very small amount of grains available for measurements and previous results showing rather low quartz luminescence sensitivity in the broader area (e.g., <xref ref-type="bibr" rid="B145">Zhang et&#x20;al., 2018</xref>), single grain measurements on potassium-rich feldspar as the only dosimeter was the method of choice in this&#x20;study.</p>
<p>A single grain, post infrared, infrared stimulated single aliquot regenerative dose protocol (SG pIRIR<sub>225</sub> SAR, e.g., <xref ref-type="bibr" rid="B103">Reimann et&#x20;al., 2012</xref>; <xref ref-type="bibr" rid="B38">Garcia et&#x20;al., 2019</xref> but modified to include the pIRIR225 signal) was applied for the determination of the equivalent dose. Measurements were conducted at the VLL on a RIS&#xd8; DA-20 luminescence reader system (<xref ref-type="bibr" rid="B18">B&#xf8;tter-Jensen et&#x20;al., 2000</xref>, <xref ref-type="bibr" rid="B17">2003</xref>) equipped with an infrared laser (830&#xa0;nm) for stimulation of the single-grain luminescence signals, which were detected through a LOT/Oriel D410/30 interference filter. For laboratory dosing, the system is equipped with a <sup>90</sup>Sr/<sup>90</sup>Y beta source delivering a dose of about 0.1&#xa0;Gy/s. Dose recovery experiments were conducted for both luminescence signals measured in the pIRIR<sub>225</sub> dose protocol [stimulated at 50&#xb0;C (IR<sub>50</sub>) and at 225&#xb0;C (pIRIR<sub>225</sub>)]. The results showed agreement with unity within the error (rejection criteria: recycling/recuperation in percent of the natural signal/test dose error &#x3d; 30/30/10%), proving the suitability of the protocol. Whenever using feldspar as a dosimeter, the effects of anomalous fading (athermal signal loss over time, <xref ref-type="bibr" rid="B142">Wintle 1973</xref>) must be considered. Fading experiments were conducted using the approach of <xref ref-type="bibr" rid="B2">Auclair et&#x20;al. (2003)</xref> but modified to also include the pIRIR<sub>225</sub> signal.</p>
<p>Naturally occurring radionuclides contributing to the doserate (decay chains of <sup>238</sup>U and <sup>232</sup>Th, and <sup>40</sup>K) were measured using low-level, high-resolution gamma spectrometry on a Baltic Scientific Instruments high purity Germanium (HPGe) p-type detector (&#x223c;52% efficiency) after storage of the sample of more than 4 weeks. The sample were found to be in secondary secular equilibrium. The overall doserates and age calculations were conducted using the software ADELE (<xref ref-type="bibr" rid="B65">Kulig, 2005</xref>).</p>
<p>Radiocarbon dating method was applied on a speleothem and bone found in the sediment succession. Radiocarbon dating was performed by accelerator mass spectrometry (AMS). Samples were prepared into graphite targets at the Ru&#x111;er Bo&#x161;kovi&#x107; Institute (RBI, Croatia). The bone sample of <italic>Ursus spelaeus</italic> (DC-SP-2, LCC, sample ID number Z-7351) was precleaned using acid-base-acid wash and collagen extraction (<xref ref-type="bibr" rid="B69">Longin 1971</xref>). However, the amount of collagen in the bone was below 0.1%, which indicated that the carbon in the collagen was too degraded for radiocarbon dating (<xref ref-type="bibr" rid="B82">Marom et&#x20;al., 2013</xref>). The speleothem sample (DC-SP-4/1, LCC, ID number Z-7352) was cut, and about 200&#xa0;mg of powder were scraped off the surface. The powder was hydrolyzed to CO<sub>2</sub> in a vacuum rig using 4% HCl. An aliquot of the obtained CO<sub>2</sub> was sealed in a pyrex tube for <sup>13</sup>C composition analysis on the isotope ratio mass spectrometer (IRMS). Another aliquot of the CO<sub>2</sub> in reaction with zinc was reduced to graphite for radiocarbon AMS analysis (<xref ref-type="bibr" rid="B58">Krajcar Broni&#x107; et&#x20;al., 2010</xref>; <xref ref-type="bibr" rid="B115">Sironi&#x107; et&#x20;al., 2013</xref>). The sample <sup>14</sup>C/<sup>13</sup>C ratio was measured on a 0.5&#xa0;MeV AMS and <sup>13</sup>C/<sup>13</sup>C ratio (<italic>&#x3b4;</italic>
<sup>13</sup>C) on isotope ratio mass spectrometer (IRMS), at the Center for Applied Isotope Studies, University of Georgia (CAIS, United&#x20;States). <italic>&#x3b4;</italic>
<sup>13</sup>C values are expressed in per mil relative to VPDB. Measured <sup>14</sup>C/<sup>13</sup>C ratios were corrected for isotope fractionation using the corresponding <italic>&#x3b4;</italic>
<sup>13</sup>C values measured by IRMS and normalized to &#x2013;25&#x2030; VPDB and presented as <italic>F</italic>
<sup>14</sup>C and the <sup>14</sup>C age before present (BP) (<xref ref-type="bibr" rid="B119">Stuiver and Polach, 1977</xref>; <xref ref-type="bibr" rid="B105">Reimer et&#x20;al., 2004</xref>). Radiocarbon age was rounded of digits in accordance with the recommendations given by <xref ref-type="bibr" rid="B119">Stuiver and Polach (1977)</xref>. The radiocarbon age was calibrated using the OxCal v 4.2.4 software (<xref ref-type="bibr" rid="B19">Bronk Ramsey 2009</xref>, <xref ref-type="bibr" rid="B20">2016</xref>) and IntCal20 calibration curves (<xref ref-type="bibr" rid="B104">Reimer et&#x20;al., 2020</xref>). Speleothem radiocarbon date was presented without reservoir correction (dead carbon fraction, <italic>DCF</italic> &#x3d; 0), with <italic>DCF</italic> of 15% which is generally used for Dinaric secondary carbonates (<xref ref-type="bibr" rid="B47">Horvatin&#x10d;i&#x107; et&#x20;al., 2003</xref>), and also with <italic>DCF</italic> of 12.5% determined at the Modri&#x10d; cave near the LCC location (<xref ref-type="bibr" rid="B107">Rudzka et&#x20;al., 2012</xref>), since <italic>DCF</italic> can vary with location (<xref ref-type="bibr" rid="B153">Srdo&#x10d; et&#x20;al., 1986</xref>; <xref ref-type="bibr" rid="B59">Krajcar Broni&#x107; et&#x20;al., 1986</xref>, <xref ref-type="bibr" rid="B60">1992</xref>; <xref ref-type="bibr" rid="B114">Sironi&#x107; et&#x20;al., 2020</xref>) and time (<xref ref-type="bibr" rid="B48">Hua et&#x20;al., 2017</xref>; <xref ref-type="bibr" rid="B5">Bajo et&#x20;al., 2017</xref>; <xref ref-type="bibr" rid="B124">Therre et&#x20;al., 2020</xref>). Reservoir corrections were reported according to <xref ref-type="bibr" rid="B117">Soulet et&#x20;al. (2016)</xref>:<disp-formula id="equ1">
<mml:math id="m1">
<mml:mrow>
<mml:mi>D</mml:mi>
<mml:mi>C</mml:mi>
<mml:mi>F</mml:mi>
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<mml:mn>1</mml:mn>
<mml:mo>&#x2212;</mml:mo>
<mml:msup>
<mml:mi>F</mml:mi>
<mml:mrow>
<mml:mn>14</mml:mn>
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<mml:mo>%</mml:mo>
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</mml:mrow>
</mml:math>
</disp-formula>
<disp-formula id="equ2">
<mml:math id="m2">
<mml:mrow>
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<mml:mi>R</mml:mi>
<mml:mrow>
<mml:mi>S</mml:mi>
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</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>8033</mml:mn>
<mml:mo>&#x2217;</mml:mo>
<mml:mi mathvariant="normal">In</mml:mi>
<mml:mrow>
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<mml:mrow>
<mml:mn>14</mml:mn>
</mml:mrow>
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<mml:mi>R</mml:mi>
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</mml:math>
</disp-formula>where <italic>F</italic>
<sup>14</sup>
<italic>R</italic>
<sub>
<italic>s-atm</italic>
</sub> is ratio of measured fraction <sup>14</sup>C in speleothem and fraction <sup>14</sup>C in contemporary atmosphere and <italic>R</italic>
<sub>
<italic>S-atm</italic>
</sub> is reservoir offset for correction to reservoir effect (reservoir age). Reservoir age is given without rounding.</p>
</sec>
<sec sec-type="results" id="s4">
<title>Results</title>
<sec id="s4-1">
<title>Cave Morphology</title>
<p>The entrance part of the LCC consists of a main channel and several smaller branches. Morphologically, the channel consists of three parts. The first part, 70&#xa0;m long, is straight and has a Dinaric orientation (NW&#x2013;SE). This is followed by two successive bends and a third straight section about 50&#xa0;m long. The entire channel runs almost parallel to the hill slope at the surface. The present cave entrance is a 1.6 &#xd7; 1&#xa0;m door. The entrance was naturally probably much lower but it was artificially slightly modified. The main channel is 6&#x2013;8&#xa0;m high, although in some places it is much higher (over 15&#xa0;m). The width of the channel is generally in the range of 4&#x2013;7&#xa0;m. The area cross-sections (<xref ref-type="fig" rid="F2">Figure&#x20;2C</xref>) are generally 20&#x2013;35&#xa0;m<sup>2</sup> but may be larger in some places, especially where the ceiling is higher due to some fractures. The depth of the allogenic sediment in the bottom of the cave channel is not known, so the full dimensions and shapes of the cross sections are not completely known. Three sets of fractures were recorded within the channel, which significantly influence its shape and formation. The first part of the channel is dominated by a set of fractures with Dinaric orientation (&#x223c;130&#xb0;&#x2013;310&#xb0;), the middle part by a set of fractures with meridional orientation (&#x223c;0&#xb0;&#x2013;180&#xb0;), and the last part is the most influential by the set of fractures with orientation of &#x223c;100&#xb0;&#x2013;280&#xb0;. The host-rock is not stratified, so there is no visible influence of bedding planes on the cave morphology. Numerous speleogens were recorded behind the channel walls: scallops, elongated domes, solution pockets, pendants, wall rills, etc. Flowstones appear only about 80&#xa0;m from the entrance, mostly in the form of wide stalagmites and wall flowstones. Due to low temperatures in winter and occurrence of ice on the cave walls, the cryofracture weathering of flowstones is pronounced in this part. The floor in the almost entire length of the channel is built of sediment and in the upper part it is mostly covered by archaeological layer. At the site of the test trench, the channel is slightly larger. It is 12&#xa0;m high, 6.6&#xa0;m wide, and the cross-sectional area is about 45&#xa0;m<sup>2</sup>. This is most likely caused by the intersection of the two sets of fractures (<xref ref-type="fig" rid="F2">Figure&#x20;2D</xref>, <xref ref-type="sec" rid="s10">Supplementary Material S1</xref>). The genesis of the whole cave, including this entrance channel, is related to the denudation effect of the sinking waters of the Gra&#x10d;ac karst polje. However, its mechanism is not yet completely clear. Morphological traces (cross-sectional shapes and speleogens indicating saturated conditions) of speleogenesis indicate that the channel was formed mainly under saturated conditions. Erosion traces of water flow in the vadose zone were not recorded because, if present, they are located in the lower parts of the channel covered with sediment.</p>
</sec>
<sec id="s4-2">
<title>Sediment Characteristics and Facies</title>
<p>Within the cave sediment infill found in the passage of the LCC, eight intervals were recognized and described. Based on similar lithological and structural features they were grouped into three lithofacies units and the top archaeological layer. A detailed description of the profile and the individual lithofacies units is given in <xref ref-type="table" rid="T1">Table&#x20;1</xref> and <xref ref-type="fig" rid="F3">Figure&#x20;3A</xref>. According to the results of particle size analysis by the sedimentation method (shown by cumulative granulometric curves, <xref ref-type="fig" rid="F4">Figure&#x20;4A</xref>) it can be seen that all described intervals consist of clayey silt to silt with a small amount of very fine sand particles (&#x3c;9% of sand). According to Trask&#x2019;s sorting coefficient (S<sub>0</sub>), all samples show poor to very poor sorting (1.802&#x2013;3.067), while the asymmetry coefficient (Sk &#x3c; 1) shows that grains smaller than the median (average Md value is 0.0154) predominate in the samples. Samples DC-SP 2, 3 and 5 are classified as very poorly sorted clayey silt, while samples DC-SP 6 and 7 are classified as poorly sorted silt. Furthermore, the results of the high-resolution particle size analysis using the laser diffractometer show a decrease in the amount of the clay-sized fraction from bottom to top of the section (<xref ref-type="fig" rid="F4">Figure&#x20;4B</xref>), the trend comparable to the results of areometric particle size analysis (<xref ref-type="fig" rid="F4">Figure&#x20;4A</xref>).</p>
<table-wrap id="T1" position="float">
<label>TABLE 1</label>
<caption>
<p>Sedimentological field description of DC-SP profile in the Lower Cerova&#x10d;ka Cave with described intervals and lithofacies.</p>
</caption>
<table>
<thead valign="top">
<tr>
<th align="left">Sediment intervals within the profile DC-SP (cm) Lithology&#x2014;short field description</th>
<th align="center">Lithofacies described within the profile DC-SP</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="left">
<bold>DC-SP 1 (0&#x2013;10)</bold> Centimeter to decimeter blocks of limestones and broken speleothems with clayey to silty matrix</td>
<td align="left">
<bold>Breakdown facies (Bd)</bold>&#x2014;within the test trench it appears in two stratigraphic horizons which are laterally interrupted. The lower boundary is not visible within the profile DC-SP. Laterally within the test trench, when visible, it is sharp and uneven. Bd facies is built of very poorly sorted angular clasts. Clasts vary in diameter from centimeter to decimeter blocks of limestones and broken speleothems with the chaotic clast supported arrangement (<xref ref-type="fig" rid="F1">Figures 1A</xref>, <xref ref-type="fig" rid="F3">3A</xref>). Clasts are often colored with black coatings (black coating can be seen also on the flowstone on today&#x2019;s surface of the cave&#x2014;black coated speleothems). Matrix is clayey to silty. The Bd facies is best visible on the western and southern vertical surfaces of the excavation site, while on the eastern side it is completely absent. The upper boundary of the Bd facies is sharp and uneven. The thickness of the Bd deposits is highly variable laterally. Based on the archaeological photo documentation and field description, the maximum thickness of Bd facies reaches up to 50&#xa0;cm</td>
</tr>
<tr>
<td align="left">
<bold>DC-SP 2 (10&#x2013;60)</bold> clayey silt to silty clay (carbonate-free sediment) with fragments of speleothems. Numerous findings of well-preserved bones and teeth, belonging to a large vertebrate (27&#xa0;cm from the bottom of the profile)</td>
<td rowspan="3" align="left">
<bold>Diamicton facies (Di)</bold>&#x2014;represents the filling of a depression formed on the upper surface of the Bd facies, as can be seen, form the disconformity between Bd and Di facies (<xref ref-type="fig" rid="F3">Figures 3A</xref>, <xref ref-type="fig" rid="F11">11A</xref>). The lower boundary of the facies is partly unclear. The impression is that the sediments of the Di facies in the transition zone intertwine with underlying Bd facies. The same sediments which built the majority of the Di facies also built a matrix of the Bd facies. Di facies is built of clayey silt with no visible gradation through the vertical profile (<xref ref-type="fig" rid="F4">Figures 4A,B</xref>). Although on the described profile these facies appear massive, laterally, unevenly scattered speleothem (seem to be collapsed from the ceiling into the clastic sediment) and limestone fragments can be observed (<xref ref-type="fig" rid="F3">Figure&#x20;3A</xref>) resulting in unsorted or poorly sorted sediment. There are no clearly arranged sedimentary textures, the larger clasts appear to "float" in the clayey silt. Numerous osteological remains of large vertebrates can be found on this horizon (<xref ref-type="fig" rid="F3">Figures 3A</xref>,<xref ref-type="fig" rid="F3">B</xref>, <xref ref-type="fig" rid="F11">11A,D</xref>). An unnatural position of the bones is visible on the excavated part of the skeleton. This can be the result of taphonomic processes, but also a sign of re-deposition of the skeleton. The upper boundary of the Di facies represents the lateral continuation of the upper boundary of the Bd facies. It is marked with a thin dashed horizontal zone with fragments of speleothems (<xref ref-type="fig" rid="F3">Figures 3A</xref>, <xref ref-type="fig" rid="F11">11C</xref>) (platy habitus, perhaps a flowstone deposited on the underlying sediment)</td>
</tr>
<tr>
<td align="left">
<bold>DC-SP 3 (60&#x2013;95)</bold> clayey silt, probably contains a smaller amount of the sandy component (carbonate-free sediment). Fragments of speleothems are visible in places</td>
</tr>
<tr>
<td align="left">
<bold>DC-SP 4 (95&#x2013;98)</bold> Horizontally oriented speleothem fragments - laterally discontinuous layer covered with a thin layer (3&#xa0;cm) of light brown clay that disappears laterally</td>
</tr>
<tr>
<td align="left">
<bold>DC-SP 5 (98&#x2013;108)</bold> clayey silt (carbonate-free sediment)</td>
<td rowspan="3" align="left">
<bold>Slackwater facies (Sw)&#x2014;Facies of grayish-yellow laminated silt</bold>: it is visible on all sides of the test trench. The lower boundary of the Sw facies is sharp and clearly marked. At the bottom, 10&#xa0;cm of homogeneous silt sharply turns into an interval of horizontally laminated sediment (mm laminae) (<xref ref-type="fig" rid="F3">Figures 3A,B</xref>). Lamination is marked by vertical alterations of the silty laminae and silty-sandy laminae. Occasionally thin layers occurred (up to 1&#xa0;cm). The thickness of the laminated interval varies laterally - the laminated interval is thinnest at about 1&#x20;m from the side of the cave wall with laminae and layers dipping toward the middle of the cave channel. Therefore, lamination partly follows the inherited morphology in the underlaying homogeneous silt and it showing a channel-like form with a maximum height of up to 10&#xa0;cm, but erosional discordance has not been observed. Laminae follow the shape of the "channel". Toward the top of the profile, there is a transition toward the zone with wavy lamination (probably a post-sedimentary deformation of the sediment&#x2014;convolution). Small cracks with vertical displacement between layers were also observed (micro faults). The increase in the amount of sand in the laminated horizon is visible from the particle size distribution curves (samples DC-SP 105 to DC-SP 135, <xref ref-type="fig" rid="F4">Figure&#x20;4B</xref>). The upper 40&#xa0;cm of the Sw facies represent silty massive sediment with a decreased amount of sand (<xref ref-type="fig" rid="F4">Figures 4B</xref>, <xref ref-type="fig" rid="F11">11B</xref>) and show a finning upwards trend. The upper boundary is marked with uneven and sharp disconformity to the late Bronze age and Modern period archaeological strata (<xref ref-type="fig" rid="F11">Figure&#x20;11A</xref>)</td>
</tr>
<tr>
<td align="left">
<bold>DC-SP 6 (108&#x2013;130)</bold> laminated clayey to sandy silt with intercalations of mm laminae and thin layers (carbonate-free sediment)</td>
</tr>
<tr>
<td align="left">
<bold>DC-SP 7 (130&#x2013;170)</bold> Homogeneous clayey-silt to silty-clay sediment (carbonate-free sediment)</td>
</tr>
<tr>
<td colspan="2" align="left">
<bold>DC-SP 8 (170&#x2013;195)</bold> archaeological strata with pottery fragments. Iapodes, late Bronze age</td>
</tr>
</tbody>
</table>
</table-wrap>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>Granulometric composition of samples from the profile DC-SP. <bold>(A)</bold> Granulometric analysis by sedimentation method: cumulative granulometric curves, <bold>(B)</bold> distribution curves of individual fractions (clay, silt, and sand) through the investigated profile.</p>
</caption>
<graphic xlink:href="feart-09-672229-g004.tif"/>
</fig>
</sec>
<sec id="s4-3">
<title>Mineralogical Composition of the Sediment</title>
<p>The results of the modal analysis of the sediment samples are given in <xref ref-type="table" rid="T2">Table&#x20;2</xref>. Within all samples the LMF predominates, represented by grains of monocrystalline quartz (84&#x2013;92%) which is mostly represented by angular and slightly rounded grains of uniform and undulose extinction. In addition to this dominant group, euhedral quartz grains can be found (<xref ref-type="fig" rid="F5">Figure&#x20;5A</xref>). Sporadic occurrences of well-rounded and spherical quartz grains were recorded, as well. The amount of rock fragments ranges from 4 to 8%. Among them, the most common are chert particles. Rare tuffitic particles were found, as well as schist rock fragments. Feldspars are represented mainly in the form of potassium feldspars, and their total amount is up to 9%. Feldspars are most often anhedral (<xref ref-type="fig" rid="F5">Figure&#x20;5B</xref>) to subhedral. Mica (muscovite) appears only sporadically (&#x3c;1%) in the form of transparent plates with a rounded outline (<xref ref-type="fig" rid="F5">Figure&#x20;5C</xref>). The LMF is quite uniform throughout the profile (<xref ref-type="table" rid="T2">Table&#x20;2</xref>). A slight decrease in the number of quartz grains toward the top of the profile was observed, and in connection with that, a slight increase in the number of feldspars and lithic particles. The mineral composition of all analyzed samples is uniform. Among the HMF, the amount of opaque minerals is high, about 90%. Completely opaque black grains, often well rounded, are observed. Chromite grains, slightly reddish-brown colored, are present in all analyzed samples and in some samples pyrite (<xref ref-type="fig" rid="F5">Figure&#x20;5D</xref>). The THM are very sparse in the samples. Among the THM, the pyroxene predominates. They appear in the form of anhedral to stubby prismatic grains, are green in color and the typical &#x201c;hacksaw&#x201d; terminations are often visible (<xref ref-type="fig" rid="F5">Figures 5F,G</xref>). According to the extinction angle, they are classified in the group of clinopyroxene. The second most common translucent heavy mineral is zircon. Zircons, mainly short-prismatic or anhedral (slightly rounded) are present in all samples. Euhedral grains are rare (<xref ref-type="fig" rid="F5">Figure&#x20;5G</xref>). Tourmaline is present in roughly the same proportion as zircon. It appears in the form of subhedral grains. It is rounded in some places. Pleochroism in brown to greenish color is visible in places. Other observed varieties belong to a group of hemimorphic grains with multicolored poles (<xref ref-type="fig" rid="F5">Figures 5E,H</xref>). Rutile is rare but still present in all samples, appearing in rounded forms with a slightly prismatic habitus. Their color is usually reddish-brown or dark red. Garnets are rare, occur in the form of weakly rounded grains or angular grains/shards with sharp edges. Colorless garnets predominate. Slightly pink garnets are also present (<xref ref-type="fig" rid="F5">Figure&#x20;5E</xref>). Among other THM, grains from the epidote-zoisite group rarely occur. The epidote is greenish, semi-rounded, in the form of irregular grains while mineral grains classified as zoisite/clinozoisite look fresh and show an anomalous blue interference color. Rare occurrences of biotite and greenish anhedral amphiboles are also present.</p>
<table-wrap id="T2" position="float">
<label>TABLE 2</label>
<caption>
<p>Mineral composition of silty cave sediment from profile DC-SP in the Lower Cerova&#x10d;ka Cave.</p>
</caption>
<table>
<thead>
<tr>
<th colspan="11" align="center">
<bold>Light mineral fraction composition (fraction 0.09&#x2013;0.16&#xa0;mm) shown in %</bold>
</th>
</tr>
<tr>
<td align="left">Sample</td>
<td colspan="2" align="center">Quartz (monocrystalline)</td>
<td colspan="2" align="left">Feldspars (kfs&#x2b;Pl)</td>
<td colspan="4" align="center">Lithic particles (chert and other)</td>
<td colspan="2" align="center">Muscovite</td>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="left">DC-SP 2</td>
<td colspan="2" align="center">92</td>
<td colspan="2" align="center">2</td>
<td colspan="4" align="center">6</td>
<td colspan="2" align="left"/>
</tr>
<tr>
<td align="left">DC-SP 3</td>
<td colspan="2" align="center">92</td>
<td colspan="2" align="center">3</td>
<td colspan="4" align="center">5</td>
<td colspan="2" align="center">&#x2b;</td>
</tr>
<tr>
<td align="left">DC-SP 5</td>
<td colspan="2" align="center">88</td>
<td colspan="2" align="center">8</td>
<td colspan="4" align="center">4</td>
<td colspan="2" align="left"/>
</tr>
<tr>
<td align="left">DC-SP 6</td>
<td colspan="2" align="center">87</td>
<td colspan="2" align="center">9</td>
<td colspan="4" align="center">4</td>
<td colspan="2" align="left"/>
</tr>
<tr>
<td align="left">DC-SP 7</td>
<td colspan="2" align="center">84</td>
<td colspan="2" align="center">8</td>
<td colspan="4" align="center">8</td>
<td colspan="2" align="center">&#x2b;</td>
</tr>
<tr>
<td colspan="11" align="center">
<bold>XRPD analysis (bulk samples) shown in %</bold>
</td>
</tr>
<tr>
<td align="left"/>
<td align="center">
<bold>Qtz</bold>
</td>
<td align="center">
<bold>Pl</bold>
</td>
<td align="center">
<bold>14&#xa0;&#xc5;</bold>
</td>
<td align="center">
<bold>10&#xa0;&#xc5;</bold>
</td>
<td align="center">
<bold>9&#xa0;&#xc5;</bold>
</td>
<td align="center">
<bold>7&#xa0;&#xc5;</bold>
</td>
<td align="center">
<bold>Gbs</bold>
</td>
<td align="center">
<bold>Hem</bold>
</td>
<td align="center">
<bold>HA</bold>
</td>
<td align="center">
<bold>Clays</bold>
</td>
</tr>
<tr>
<td align="left">DC-SP 1 bone</td>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">100</td>
<td align="left"/>
</tr>
<tr>
<td align="left">DC-SP 1</td>
<td align="center">12</td>
<td align="left"/>
<td align="center">&#x2b;</td>
<td align="center">&#x2b;</td>
<td align="center">&#x2b;</td>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">39</td>
<td align="center">49</td>
</tr>
<tr>
<td align="left">DC-SP 2</td>
<td align="center">35</td>
<td align="left"/>
<td align="center">&#x2b;</td>
<td align="center">&#x2b;</td>
<td align="center">&#x2b;</td>
<td align="center">&#x2b;</td>
<td align="center">?</td>
<td align="center">&#x2a;</td>
<td align="left"/>
<td align="center">65</td>
</tr>
<tr>
<td align="left">DC-SP 3</td>
<td align="center">36</td>
<td align="left"/>
<td align="center">&#x2b;</td>
<td align="center">&#x2b;</td>
<td align="center">&#x2b;</td>
<td align="center">&#x2b;</td>
<td align="center">&#x2a;</td>
<td align="center">&#x2a;</td>
<td align="left"/>
<td align="center">64</td>
</tr>
<tr>
<td align="left">DC-SP 4/2</td>
<td align="center">30</td>
<td align="center">6</td>
<td align="center">&#x2b;</td>
<td align="center">&#x2b;</td>
<td align="left"/>
<td align="center">&#x2b;</td>
<td align="center">?</td>
<td align="center">?</td>
<td align="left"/>
<td align="center">64</td>
</tr>
<tr>
<td align="left">DC-SP 5</td>
<td align="center">31</td>
<td align="center">4</td>
<td align="center">&#x2b;</td>
<td align="center">&#x2b;</td>
<td align="left"/>
<td align="center">&#x2b;</td>
<td align="center">&#x2a;</td>
<td align="center">?</td>
<td align="left"/>
<td align="center">65</td>
</tr>
<tr>
<td align="left">DC-SP 6</td>
<td align="center">32</td>
<td align="center">7</td>
<td align="center">&#x2b;</td>
<td align="center">&#x2b;</td>
<td align="left"/>
<td align="center">&#x2b;</td>
<td align="center">?</td>
<td align="center">?</td>
<td align="left"/>
<td align="center">61</td>
</tr>
<tr>
<td align="left">DC-SP 7</td>
<td align="center">34</td>
<td align="center">6</td>
<td align="center">&#x2b;</td>
<td align="center">&#x2b;</td>
<td align="left"/>
<td align="center">&#x2b;</td>
<td align="left"/>
<td align="center">?</td>
<td align="left"/>
<td align="center">60</td>
</tr>
<tr>
<td colspan="11" align="center">
<bold>XRPD analysis (fraction &#x3c; 2&#xa0;&#xb5;m) shown by the relative abundance</bold>
</td>
</tr>
<tr>
<td align="left"/>
<td align="center">
<bold>L.c. Vrm</bold>
</td>
<td align="center">
<bold>Vrm</bold>
</td>
<td align="center">
<bold>Ill/Ms</bold>
</td>
<td align="center">
<bold>Tlc-Prl</bold>
</td>
<td align="center">
<bold>Kln</bold>
</td>
<td align="center">
<bold>KlnD</bold>
</td>
<td align="center">
<bold>Chl</bold>
</td>
<td align="center">
<bold>Qtz</bold>
</td>
<td align="center">
<bold>Chl-V</bold>
</td>
<td align="center">
<bold>I-S</bold>
</td>
</tr>
<tr>
<td align="left">DC-SP 2</td>
<td align="center">&#x2a;</td>
<td align="center">XX</td>
<td align="center">X</td>
<td align="center">&#x2a;</td>
<td align="center">X</td>
<td align="center">&#x2a;</td>
<td align="center">XX</td>
<td align="center">&#x2013;</td>
<td align="center">X</td>
<td align="center">&#x2a;</td>
</tr>
<tr>
<td align="left">DC-SP 3</td>
<td align="center">&#x2a;</td>
<td align="center">XX</td>
<td align="center">X</td>
<td align="center">&#x2a;</td>
<td align="center">XX</td>
<td align="center">&#x2a;</td>
<td align="center">X</td>
<td align="center">&#x2a;</td>
<td align="center">X</td>
<td align="left"/>
</tr>
<tr>
<td align="left">DC-SP 4/2</td>
<td align="center">X</td>
<td align="center">X</td>
<td align="center">X</td>
<td align="center">&#x2a;</td>
<td align="center">XX</td>
<td align="left"/>
<td align="center">X</td>
<td align="center">&#x2a;</td>
<td align="center">X</td>
<td align="left"/>
</tr>
<tr>
<td align="left">DC-SP 5</td>
<td align="center">&#x2a;</td>
<td align="center">XX</td>
<td align="center">X</td>
<td align="center">&#x2a;</td>
<td align="center">XX</td>
<td align="center">&#x2a;</td>
<td align="center">X</td>
<td align="center">&#x2a;</td>
<td align="center">X</td>
<td align="left"/>
</tr>
<tr>
<td align="left">DC-SP 6</td>
<td align="center">&#x2a;</td>
<td align="center">X</td>
<td align="center">X</td>
<td align="left"/>
<td align="center">XX</td>
<td align="center">&#x2a;</td>
<td align="center">X</td>
<td align="center">&#x2a;</td>
<td align="center">X</td>
<td align="center">&#x2a;</td>
</tr>
<tr>
<td align="left">DC-SP 7</td>
<td align="center">X</td>
<td align="center">X</td>
<td align="center">X</td>
<td align="left"/>
<td align="center">XX</td>
<td align="center">&#x2a;</td>
<td align="center">X</td>
<td align="center">&#x2a;</td>
<td align="center">X</td>
<td align="center">&#x2a;</td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn>
<p>Data is obtained by modal analysis of Light mineral fraction (performed on fraction 0.09&#x2013;0.16&#xa0;mm), and by Quantitative XRPD analysis. Quantitative mineral composition of bulk samples and semi-quantitative mineral composition of the &#x3c;2&#xa0;&#xb5;m fractionis are shown. <underline>Abbreviation codes:</underline> Qtz&#x2014;quartz, Pl&#x2014;plagioclase, Gbs&#x2014;gibbsite, Hem&#x2014;hematite, HA&#x2014;hydroxylapatite, 14, 10, 9, 7&#xa0;&#xc5;&#x2014;type of clay minerals present in bulk sample marked with &#x2b;, ?&#x2014;mineral is probably present in the sample but cannot be confirmed with certainty because of low content and/or overlapping of diffraction maximums. L.c. Vrm&#x2014;Low-charge vermiculite or high-charge smectite, Vrm&#x2014;vermiculite, Ill/Ms&#x2014;illite/muscovite, Tlc-Prl&#x2014;talc-pyrophillite group, Kln &#x3d; Kaolinite which does not intercalate with DMSO, KlnD&#x2014;kaolinite which forms intercalation compounds with DMSO, Chl&#x2014;chlorite, Chl-V&#x2014;chlorite-vermiculite mixed-layerd clay mineral, I-S&#x2014;illite-smectite mixed-layerd clay mineral, XXX&#x2014;dominant (&#x3e;50%), XX&#x2014;abundant (20&#x2013;50%), X&#x2014;subordinate (1&#x2013;20%), &#x2a;&#x2014;traces (&#x3c;1%).</p>
</fn>
</table-wrap-foot>
</table-wrap>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption>
<p>Overview of selected mineral grains from the light and heavy mineral fraction of the DC-SP profile (photo without analyzer). <bold>(A)</bold> Weakly rounded allotriomorphic and hypidiomorphic quartz grains (Q) from sample DC-SP 2, <bold>(B)</bold> Feldspar (F) from sample DC-SP 2, <bold>(C)</bold> muscovite grains (ms) from sample DC-SP 7, <bold>(D)</bold> rounded opaque minerals (op), chromite (cr), and pyrite (py) from sample DC-SP 2, <bold>(E)</bold> opaque minerals (op), tourmaline (tu), and garnet (grt) from sample DC-SP 6, <bold>(F)</bold> pyroxenes (px) from sample DC-SP 6, <bold>(G)</bold> zircon (zrn), and pyroxene (px) from sample DC-SP 2, and <bold>(H)</bold> opaque minerals (op) and tourmaline (tu) from sample DC-SP 3.</p>
</caption>
<graphic xlink:href="feart-09-672229-g005.tif"/>
</fig>
<p>The results of the XRPD method are shown in <xref ref-type="table" rid="T2">Table&#x20;2</xref>. Sample DC-SP 1 is extremely heterogenous. It consists of bone fragments, and sandy silt size sediments. The analysis was performed on both parts. Sediment sample DC-SP 1 (silt), in addition to clay minerals, contains a significant amount of hydroxylapatite (HA) and quartz (<xref ref-type="table" rid="T2">Table&#x20;2</xref>). Quantities of fractions &#x3c;2&#xa0;&#x3bc;m were too small for clay analysis, so the analysis was performed on a fraction &#x3c;0.063&#xa0;mm. In that fraction quartz, vermiculite, illite/muscovite, talc-pyrophyllite, kaolinite and a small amount of chlorite are present. Bone fragment sample consists only of HA. The main mineral phases in all other analyzed samples are clay minerals and quartz (<xref ref-type="table" rid="T2">Table&#x20;2</xref>). Samples DC-SP 4 to DC-SP 7 contain a smaller amount of plagioclase. Some of the samples (<xref ref-type="table" rid="T2">Table&#x20;2</xref>) contain a very small amount of gibbsite and hematite, but due to the low content cannot be confirmed with certainty in all samples. Mineral composition of &#x3c;2&#xa0;&#x3bc;m fraction of all analyzed samples is similar. In the analyzed samples, among clay minerals, vermiculite, illite/muscovite, kaolinite, and a lesser amount of chlorite and chlorite-vermiculite regularly appear. In some samples, small quantities of low-charge vermiculite or high-charge smectite, talc-pyrophyllite, kaolinite which forms intercalation compounds with DMSO and illite-smectite are also present. Samples DC-SP 3 and DC-SP 5 probably contain secondary chlorite (the 14&#xc5; diffraction maximum disappeared after heating to 550&#xb0;C).</p>
</sec>
<sec id="s4-4">
<title>Palynofacies</title>
<p>Palynofacies of all studied samples beside the oldest one (DC-SP 1) are dominated by phytoclasts. Sporomorphs occur in a small amount and therefore there is no standard palynological diagram. Instead of that, only organic matter abundance is presented in the diagram (<xref ref-type="fig" rid="F6">Figure&#x20;6</xref>). In the oldest analyzed sample, DC-SP 1, the palynofacies is dominated by bacterial amorphous organic matter (AOM) particles (<xref ref-type="fig" rid="F7">Figure&#x20;7A</xref>), and non-opaque phytoclasts, mostly amorphous particles, which indicate an increased input of terrigenous material. Only a few Pinaceae pollen (<xref ref-type="fig" rid="F7">Figure&#x20;7C</xref>) and Fungi spores occur. Microscopic charcoal remains (around 100 microns in size; <xref ref-type="fig" rid="F7">Figure&#x20;7B</xref>) point to the influence of fire (<xref ref-type="bibr" rid="B141">Whitlock and Larsen, 2002</xref>). Palynofacies from the sample DC-SP 2 is dominated by opaque phytoclasts, mostly corroded charcoal, while non-opaque phytoclasts decreased. Sporomorphs from conifer Pinaceae (<xref ref-type="fig" rid="F7">Figure&#x20;7D</xref>) family as well as herbs of Asteraceae (<xref ref-type="fig" rid="F7">Figure&#x20;7D</xref>) and Cichoriaceae family (<xref ref-type="fig" rid="F7">Figure&#x20;7E</xref>) dominate in the same ratio (6%). They point to a cold and dry climate, probably to a glacial stage. In sample DC-SP 7 palynofacies is still dominated by the opaque phytoclasts, mostly corroded charcoal. Beside phytoclasts there are a lot of particles resembling cyanobacteria, maybe degraded cyanobacteria (<xref ref-type="fig" rid="F7">Figures 7F,G</xref>) that lived in the cave. Palynofacies from the youngest sample DC-SP 8 is dominated by the phytoclasts, mostly non-opaque phytoclasts&#x2014;brown wood and amorphous particles. Rare findings of the palynomorph <italic>Pseudoschizaea</italic> (<xref ref-type="fig" rid="F7">Figure&#x20;7I</xref>), probably related to Zygnemataceae, indicate the runoff due to periods of enhanced soil erosion outside the cave (<xref ref-type="bibr" rid="B68">Leroy et&#x20;al., 2007</xref>). The presence of spores from the genus <italic>Glomus</italic> suggests erosion from a forested upstream slope (<xref ref-type="bibr" rid="B132">van Geel, 2001</xref>), possibly due to fires, themselves evidenced by an increase in microcharcoal particles. Aquatic pollen (<italic>Typha</italic>) and grasses (Graminae) were also present in the similar ratio (ca. 3%). At the same time rare <italic>Polygonum persicaria</italic> (<xref ref-type="fig" rid="F7">Figure&#x20;7H</xref>) points to anthropogenic influence.</p>
<fig id="F6" position="float">
<label>FIGURE 6</label>
<caption>
<p>Organic matter (OM) percentage abundance diagram for the DC-SP profile in the Lower Cerova&#x10d;ka Cave. Diagram was made with the Tilia software (<xref ref-type="bibr" rid="B41">Grimm, 1991</xref>).</p>
</caption>
<graphic xlink:href="feart-09-672229-g006.tif"/>
</fig>
<fig id="F7" position="float">
<label>FIGURE 7</label>
<caption>
<p>Palynofacies from the profile DC-SP in the Lower Cerova&#x10d;ka Cave <bold>(A,B)</bold> DC-SP 1, <bold>(C,D)</bold> DC-SP 2, <bold>(E,F)</bold> DC-SP 7, and <bold>(G,H)</bold> DC-SP 8.</p>
</caption>
<graphic xlink:href="feart-09-672229-g007.tif"/>
</fig>
</sec>
<sec id="s4-5">
<title>Paleontological and Taphonomic Analysis</title>
<p>The vertebrate remains from the Pleistocene deposits of the test trench (specifically 873 fragments) were recovered at a depth of &#x223c;1.2&#xa0;m, within a 30&#xa0;cm thick layer (<xref ref-type="fig" rid="F3">Figure&#x20;3A</xref>). Of these, 230 bones and teeth are identified to the genus <italic>Ursus</italic> (26.4%). The vertebrate remains are therefore documented and presented within <xref ref-type="fig" rid="F8">Figure&#x20;8</xref>. Based on morphological and metrical characteristics, all bear remains from LCC are attributed to cave bear (<italic>U. spelaeus</italic>), making this species the only mammalian taxon identified within the analyzed faunal assemblage from Pleistocene deposits. The vast majority of the remains, however, remained taxonomically undetermined. Based on their relative size and robustness, many of these remains could also come from a cave bear. However, given the mention of rare findings of other large carnivores and herbivores in previous studies (<xref ref-type="bibr" rid="B77">Malez, 1965b</xref>; <xref ref-type="bibr" rid="B96">Paunovi&#x107; et&#x20;al., 1999</xref>), this assumption should be considered with caution and the possibility of the existence of other taxa in this assemblage should not be ruled out. Although most of the remains could not be aged precisely, information of the relative age at death shows predominance of adult bears (81.7%), while the rest belongs to juveniles (<xref ref-type="fig" rid="F8">Figure&#x20;8</xref>). A single bone is attributed to a fetal or newborn animal.</p>
<fig id="F8" position="float">
<label>FIGURE 8</label>
<caption>
<p>Body part representation (NISP) of <italic>Ursus spelaeus</italic> at the profile DC-SP in the Lower Cerova&#x10d;ka Cave, presented separately for two main age categories. A single fetal/neonatal bone has been excluded.</p>
</caption>
<graphic xlink:href="feart-09-672229-g008.tif"/>
</fig>
<p>In order to study the body part representation of bears in the LCC, data for both cave bear and taxonomically indeterminate remains of the similar body size are combined. All major parts of the body are present (<xref ref-type="fig" rid="F8">Figure&#x20;8</xref>) suggesting deposition of complete bear carcasses within the cave. However, a closer examination of the differential representation of different body parts revealed the following: the most abundant class are trunk elements (32.2%), closely followed by the elements of the head (teeth included; 29.1%) and feet bones (25.2%). Relative to them, larger bones of the appendicular skeleton are under-represented within the analyzed assemblage. Thus, the upper elements of the fore limbs (<italic>scapula, humerus, radius, ulna</italic>) and hind limbs (<italic>pelvis, femur, tibia, fibula</italic>) are represented by only 6.1 and 7.4%, respectively.</p>
<p>With the exception of a few more complete bones, the skeletal material is fragmented. Recent breaks are present but most breakages are dry and attributable to natural processes typical of cave environment (e.g., trampling by other animals, sediment pressure). Looking at the bone surface modifications the material is relatively well preserved. The average bone color varies between pale white to yellowish white. Just a few fragments display small areas of dark brownish coloration, suggesting light staining probably due to exposure to minerals in the sediment. Besides fragmentation, the most common taphonomic modification is very light weathering (fine line fractures and spalling of bone surface), while chemical etching is evidenced on several fragments. In addition, only a few bones were gnawed by large carnivores (e.g., cave lion or hyena) and there is no evidence of modification by hominins.</p>
</sec>
<sec id="s4-6">
<title>Luminescence Dating</title>
<p>Using the rejection criteria determined in dose recovery experiments, 43 equivalent dose values were accepted for the IR<sub>50</sub> signal, and 33 for the pIRIR<sub>225</sub> signal, respectively. Dose distributions for both signals are positively skewed and show overdispersion values of 56&#x20;&#xb1; 7% (IR<sub>50</sub>) and 42&#x20;&#xb1; 7% (pIRIR<sub>225</sub>), which in combination can be interpreted as an indication for incomplete bleaching being significant in the sample. Therefore, average equivalent doses for both signals were calculated using a bootstrapped three-parameter minimum age model (<xref ref-type="bibr" rid="B37">Galbraith et&#x20;al., 1999</xref>; <xref ref-type="bibr" rid="B25">Cunningham and Wallinga, 2012</xref>), with sigma<sub>b</sub> of 0.3&#x20;&#xb1; 0.2 as a threshold value, based on the overdispersion values from dose recovery experiments and assigned with an uncertainty to account for the lack of a well-bleached natural reference sample. The g-values of 5.6&#x20;&#xb1; 0.8 for the IR<sub>50</sub> and 0.6&#x20;&#xb1; 0.9 for the pIRIR<sub>225</sub> signal were obtained after fading corrections. Fading correction was conducted using the approach of <xref ref-type="bibr" rid="B51">Huntley and Lamothe (2001)</xref> and calculated using the R-Luminescence package of <xref ref-type="bibr" rid="B61">Kreutzer et&#x20;al. (2012)</xref>. Equivalent dose values and resulting ages as well as all luminescence results are summarized in <xref ref-type="table" rid="T3">Table&#x20;3</xref>.</p>
<table-wrap id="T3" position="float">
<label>TABLE 3</label>
<caption>
<p>Results from radionuclide analysis and luminescence dating of detrital cave sediments from profile DC-SP in the Lower Cerova&#x10d;ka Cave.</p>
</caption>
<table>
<thead valign="top">
<tr>
<th align="left">Sample lab code</th>
<th align="center">Sample field code</th>
<th align="center">
<sup>238</sup>U (Bq/kg)</th>
<th align="center">
<sup>232</sup>Th (Bq/kg)</th>
<th align="left">
<sup>40</sup>K (Bq/kg)</th>
<th align="center">Depth below land surface (m)</th>
<th align="center">Overall doserate Fs (Gy/ka)<xref ref-type="table-fn" rid="Tfn1">
<sup>a</sup>
</xref>
</th>
<th align="center">IR50 SG (n)<xref ref-type="table-fn" rid="Tfn2">
<sup>b</sup>
</xref>
</th>
<th align="center">pIRIR225 SG (n)<xref ref-type="table-fn" rid="Tfn2">
<sup>b</sup>
</xref>
</th>
<th align="center">&#x3c3;b<xref ref-type="table-fn" rid="Tfn3">
<sup>c</sup>
</xref> IR50 (%)</th>
<th align="center">&#x3c3;b<xref ref-type="table-fn" rid="Tfn3">
<sup>c</sup>
</xref> pIRIR225 (%)</th>
<th align="center">IR50&#x20;D<sub>e</sub> (Gy)<xref ref-type="table-fn" rid="Tfn4">
<sup>d</sup>
</xref>
</th>
<th align="center">pIRIR225&#x20;D<sub>e</sub> (Gy)<xref ref-type="table-fn" rid="Tfn4">
<sup>d</sup>
</xref>
</th>
<th align="center">IR50 age (ka) faded<xref ref-type="table-fn" rid="Tfn5">
<sup>e</sup>
</xref>
</th>
<th align="center">IR50 age (ka) fading corr<xref ref-type="table-fn" rid="Tfn6">
<sup>f</sup>
</xref>
</th>
<th align="center">pIRIR225 age (ka) faded<xref ref-type="table-fn" rid="Tfn5">
<sup>e</sup>
</xref>
</th>
<th align="center">pIRIR225 age (ka) fading corr<xref ref-type="table-fn" rid="Tfn6">
<sup>f</sup>
</xref>
</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="left">VLL-0495-L</td>
<td align="center">DC-SP 3</td>
<td align="char" char="plusmn">75.33&#x20;&#xb1; 5.42</td>
<td align="char" char="plusmn">94.92&#x20;&#xb1; 5.32</td>
<td align="char" char="plusmn">506.00&#x20;&#xb1; 30.36</td>
<td align="center">&#x223c;60&#x20;m</td>
<td align="char" char="plusmn">4.41&#x20;&#xb1; 0.48</td>
<td align="char" char=".">43</td>
<td align="char" char=".">33</td>
<td align="char" char="plusmn">56&#x20;&#xb1; 7</td>
<td align="char" char="plusmn">42&#x20;&#xb1; 7</td>
<td align="char" char="plusmn">136.5&#x20;&#xb1; 24.4</td>
<td align="char" char="plusmn">237.0&#x20;&#xb1; 16.3</td>
<td align="char" char="plusmn">30.9&#x20;&#xb1; 6.5</td>
<td align="char" char="plusmn">60.8&#x20;&#xb1; 20.6</td>
<td align="char" char="plusmn">
<bold>53.7</bold>&#x20;&#xb1; <bold>6.9</bold>
</td>
<td align="char" char="plusmn">56.7&#x20;&#xb1; 8.2</td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn id="Tfn1">
<label>a</label>
<p>Cosmic doserate determined according to <xref ref-type="bibr" rid="B100">Prescott and Stephan (1982)</xref> and <xref ref-type="bibr" rid="B99">Prescott and Hutton (1994)</xref>, taking the geographical position of the sampling spot (longitude, latitude, and altitude), the depth below surface, as well as the average density of the sediment overburden into account. An uncertainty of 10% was assigned to the calculated cosmic doserate. External and internal doserate calculated using the conversion factors of <xref ref-type="bibr" rid="B1">Adamiec and Aitken (1998)</xref> and the <italic>&#xdf;</italic>-attenuation factors of <xref ref-type="bibr" rid="B84">Mejdahl (1979)</xref>, including an alpha attenuation factor of 0.08 &#xb1;0.01 and an internal K content of 12.5 &#xb1;0.5% (<xref ref-type="bibr" rid="B50">Huntley and Baril 1997</xref>) and an estimated average water content of 30&#x20;&#xb1; 10% throughout burial time. Error was propagated to the overall doserate calculation.</p>
</fn>
<fn id="Tfn2">
<label>b</label>
<p>Number of grains passing all rejection criteria.</p>
</fn>
<fn id="Tfn3">
<label>c</label>
<p>Overdispersion calculated using the CAM (<xref ref-type="bibr" rid="B37">Galbraith et&#x20;al., 1999</xref>).</p>
</fn>
<fn id="Tfn4">
<label>d</label>
<p>Calculated using the bootstrapped MAM-3 (<xref ref-type="bibr" rid="B37">Galbraith et&#x20;al., 1999</xref>; <xref ref-type="bibr" rid="B25">Cunningham and Wallinga 2012</xref>).</p>
</fn>
<fn id="Tfn5">
<label>e</label>
<p>Calculated using the software ADELE (<xref ref-type="bibr" rid="B65">Kulig, 2005</xref>).</p>
</fn>
<fn id="Tfn6">
<label>f</label>
<p>Corrected for fading according to the method of <xref ref-type="bibr" rid="B51">Huntley and Lamothe (2001)</xref> using the R Luminescence package (<xref ref-type="bibr" rid="B61">Kreutzer et&#x20;al., 2012</xref>).</p>
</fn>
</table-wrap-foot>
</table-wrap>
<p>The different characteristics of the two luminescence signals measured with the pIRIR<sub>225</sub> dose protocol can be used to assess the reliability of the determined ages. The IR<sub>50</sub> and pIRIR<sub>225</sub> signals are known to exhibit different fading rates, as was confirmed by the fading measurements in this study, and different bleaching rates, with the IR<sub>50</sub> signal bleaching much faster than the pIRIR<sub>225</sub> signal (e.g., <xref ref-type="bibr" rid="B91">Murray et&#x20;al., 2012</xref>; <xref ref-type="bibr" rid="B8">Bickel et&#x20;al., 2015a</xref>, <xref ref-type="bibr" rid="B9">2015b</xref>). If incomplete bleaching is significant in a sample, the success of the correction of the effect of incomplete bleaching using the statistical approach of the bootstrapped MAM can be assessed by comparing the fading corrected ages for both signals. If the apparent age of the IR<sub>50</sub> is significantly younger than that of the pIRIR<sub>225</sub> signal, incomplete bleaching was not successfully corrected for. If, however, the fading corrected ages for the two signals are in agreement within error limits, like is the case here, this is a strong argument for a successful correction of the effects of incomplete bleaching. Although fading correction was applied also for the pIRIR<sub>225</sub> signal for comparative reasons, the fading rate is negligible within error and because of that the pIRIR<sub>225</sub> based age not corrected for fading of 53.7&#x20;&#xb1; 6.9 ka can be regarded as the most reliable depositional age for the sample (marked in bold in <xref ref-type="table" rid="T3">Table&#x20;3</xref>). In addition, it is important to note that the luminescence age is in stratigraphic order with the radiocarbon age obtained from a flowstone sample (Chapter 4.6.2), further corroborating the high reliability of the age determination.</p>
</sec>
<sec id="s4-7">
<title>Radiocarbon Dating</title>
<p>The speleothem sample (Z-7352, graphite number A2160 (RBI), ID number UGAMS&#x23; 49576 (CAIS)&#x2014;<xref ref-type="fig" rid="F9">Figures 9A&#x2013;C</xref>) had <italic>F</italic>
<sup>14</sup>C &#x3d; 0.1148&#x20;&#xb1; 0.0006 (17,390&#x20;&#xb1; 40 BP) and <italic>&#x3b4;</italic>
<sup>13</sup>C -5.3&#x20;&#xb1; 0.1&#x2030;. <italic>F</italic>
<sup>14</sup>C and radiocarbon dates without and with <italic>DCF</italic> of 12.5 and 15%, along with their calibrated dates are presented in <xref ref-type="table" rid="T4">Table&#x20;4</xref>. Compared calibration curves for both 12.5 and 15% <italic>DCF</italic> and both for using the reservoir function in OxCal and calibrating raw <sup>14</sup>C dates are presented in <xref ref-type="fig" rid="F9">Figure&#x20;9D</xref>. Here should be pointed out that there is a large difference between conventional radiocarbon dated (expressed as BP) and calibrated calendar dates (expressed as cal AD and cal BC) in this part of the radiocarbon calibration curve, resulting in difference of about 2,500&#x20;years between the conventional and calibrated age. The true age of material with the obtained age of 16 ka BP is therefore &#x223c;19.5 ka old (<xref ref-type="table" rid="T4">Table&#x20;4</xref>).</p>
<fig id="F9" position="float">
<label>FIGURE 9</label>
<caption>
<p>Sampled flowstone (<sup>14</sup>C) from the DC-SP profile in the Lower Cerova&#x10d;ka Cave <bold>(A)</bold> Bottom view, <bold>(B)</bold> top view, <bold>(C)</bold> cross-section with indicated sampling line, <bold>(D)</bold> calibration curves for <sup>14</sup>C date without <italic>DCF</italic> correction (in gray), and for 12.5% (&#x201c;Reservoir 1,073,&#x201d; in green) and 15% (&#x201c;Reservoir 1,305,&#x201d; in red) <italic>DCF.</italic>
</p>
</caption>
<graphic xlink:href="feart-09-672229-g009.tif"/>
</fig>
<table-wrap id="T4" position="float">
<label>TABLE 4</label>
<caption>
<p>
<italic>F</italic>
<sup>14</sup>C and radiocarbon dates and calibrated dates for dead carbon fraction of 0, 12.5 and 15%, <italic>R</italic>
<sub>
<italic>S-atm</italic>
</sub>&#x2014;reservoir offset for correction to reservoir effect using the OxCal v 4.2.4 software (<xref ref-type="bibr" rid="B19">Bronk Ramsey 2009</xref>, 2016).</p>
</caption>
<table>
<thead valign="top">
<tr>
<th rowspan="2" align="left">
<italic>DCF</italic> (%)</th>
<th rowspan="2" align="center">
<italic>F</italic>
<sup>14</sup>C</th>
<th rowspan="2" align="center">
<italic>F</italic>
<sup>14</sup>
<italic>R</italic>
<sub>
<italic>s-atm</italic>
</sub>
</th>
<th rowspan="2" align="center">
<sup>14</sup>C date (BP)</th>
<th rowspan="2" align="center">
<italic>R</italic>
<sub>
<italic>S-atm</italic>
</sub> (BP)</th>
<th colspan="2" align="center">Calibrated date (95.4%)</th>
</tr>
<tr>
<th align="center">Span</th>
<th align="center">Median</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="left">0</td>
<td align="char" char="plusmn">0.1148&#x20;&#xb1; 0.0006</td>
<td align="char" char=".">1</td>
<td align="char" char="plusmn">17,390&#x20;&#xb1; 40</td>
<td align="center">&#x2013;</td>
<td align="center">19,050&#x2013;18,940&#xa0;cal BC</td>
<td align="center">19,002&#xa0;cal BC</td>
</tr>
<tr>
<td align="left">12.5</td>
<td align="left"/>
<td align="char" char=".">0.875</td>
<td align="char" char="plusmn">16,315&#x20;&#xb1; 40<xref ref-type="table-fn" rid="Tfn7">
<sup>a</sup>
</xref>
</td>
<td align="char" char=".">1,073</td>
<td align="center">18,189&#x2013;17,811&#xa0;cal BC</td>
<td align="center">18,000&#xa0;cal BC</td>
</tr>
<tr>
<td align="left">15</td>
<td align="left"/>
<td align="char" char=".">0.85</td>
<td align="char" char="plusmn">16,080&#x20;&#xb1; 40<xref ref-type="table-fn" rid="Tfn7">
<sup>a</sup>
</xref>
</td>
<td align="char" char=".">1,305</td>
<td align="center">17,949&#x2013;17,562&#xa0;cal BC</td>
<td align="center">17,758&#xa0;cal BC</td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn id="Tfn7">
<label>a</label>
<p>Dates presented only for orientation, not used directly in the calibration&#x20;curve.</p>
</fn>
<fn>
<p>Radiocarbon dates were calibrated using IntCal20 calibration curve (<xref ref-type="bibr" rid="B104">Reimer et&#x20;al., 2020</xref>) and calibrated date spans are given with 95.4% confidence (<italic>k</italic>&#x20;&#x3d; 2).</p>
</fn>
</table-wrap-foot>
</table-wrap>
</sec>
</sec>
<sec sec-type="discussion" id="s5">
<title>Discussion</title>
<sec id="s5-1">
<title>Mineral Composition and Provenance of Cave Sediments</title>
<p>The investigated sediments represent the clastic filling of cave channels. Earlier research assumed that the clastic filling of cave channels is an accumulation of <italic>in situ</italic> products of weathering of the host rock (Malez, 1965). According to mineralogical analysis presented within this paper the cave sediment is mainly allochthonous clastic detritus but a part of it is autochthonous chemogenic and collapse material. The overall mixture of cave detrital sediments depends greatly on the weathering products in the source area, transported and deposited by episodic events in different facies types (depending on flow dynamics) inside the cave (<xref ref-type="bibr" rid="B53">Georgiadis et&#x20;al., 2019</xref>). Therefore, our results are compared to the geological units in the river Otu&#x10d;a catchment area (<xref ref-type="fig" rid="F1">Figures&#x20;1B,C</xref>).</p>
<p>The results of the LMF and XRD analysis (<xref ref-type="table" rid="T2">Table&#x20;2</xref>) shows that the main components of the analyzed cave sediments are quartz and clay minerals. The sample DC-SP 1 additionally contains bone fragments and significant amounts of hydroxyapatite (HA) (<xref ref-type="table" rid="T2">Table&#x20;2</xref>). HA is the main constituent of mammalian bones and teeth and is often recognized within cave sediments, like e.g., in the Modri&#x10d; Cave (<xref ref-type="bibr" rid="B86">Miko et&#x20;al., 2001</xref>). Also, the relationship between the habitation of bats and HA formation in caves has been found in limestone caves worldwide (Hill and Forti, 1997). HA is usually formed as a crust that coats speleothems and bedrock substrate surfaces within or near bat habitats, while powdery forms of HA could be found under bat guano deposits (<xref ref-type="bibr" rid="B22">Chang et&#x20;al., 2010</xref> and references therein). Hence, it is possible that beside the tiny bone fragments in the fine-grained part of the sample DC-SP 1, a part of the HA may also have originated from the <italic>in situ</italic> bat guano, as indicated by the dark color of the sediment. In samples DC-SP 4 to DC-SP 7 small amount of plagioclase are also present (<xref ref-type="table" rid="T2">Table&#x20;2</xref>). Their preservation in the samples and the absence of gibbsite and hematite indicates that these samples were subjected to less intensive pre-burial weathering compared to samples DC-SP 2 and DC-SP 3. The clay minerals contained in the analyzed cave sediments (<xref ref-type="table" rid="T2">Table&#x20;2</xref>) are similar in composition to the Terra Rossa type paleosols developed on the carbonate rock in the Adriatic region (<xref ref-type="bibr" rid="B29">Durn et&#x20;al., 2007</xref>, <xref ref-type="bibr" rid="B31">2018</xref>). In the wider Mediterranean area, the mineral composition of Terra Rossa type soils and palaeosols may be very variable (<xref ref-type="bibr" rid="B28">Durn, 2003</xref>). This variable composition is a consequence of the polygenetic nature of Terra Rossa which can form exclusively from the insoluble residue of limestone and dolomite but much more often encompasses a range of parent materials that arrived on the carbonate terrain by different transport mechanisms (<xref ref-type="bibr" rid="B28">Durn, 2003</xref>). Thus, in Istrian Terra Rossa, the dominant mineral phases in the clay fraction are kaolinite, illitic material, Fe-oxides and XRD amorphous inorganic compounds, while vermiculite, low-charge-vermiculite or high-charge smectite, chlorite, mixed-layer clay minerals and quartz are present in smaller quantities (<xref ref-type="bibr" rid="B28">Durn, 2003</xref>). Terra Rossa soils from Western Herzegovina have a similar composition where the dominant mineral phases in the clay minerals fraction are kaolinite, Fe-oxides and XRD amorphous inorganic compounds, while vermiculite, smectite, illitic material, chlorite&#x2013;vermiculite and quartz are present in a subordinate amount (<xref ref-type="bibr" rid="B30">Durn et&#x20;al., 2014</xref>). However, even though cave sediments show similarities to Terra Rossa type soils, they cannot be classified as soils (<xref ref-type="bibr" rid="B146">Zupan Hajna et&#x20;al., 2020</xref>). Cave sediments reveal a good, multi-proxy record of cave and surface environmental conditions in the time of their deposition (<xref ref-type="bibr" rid="B14">Bos&#xe1;k, 2002</xref>). Therefore, the red clayey-silty sediments found in the LCC can, to some extent, be considered as redeposited Terra Rossa. Despite the similarities, cave sediments appear to have suffered less advanced stages of weathering compared to Terra Rossa. <xref ref-type="bibr" rid="B52">Iacoviello and Martini (2012)</xref> came to the same conclusion comparing the clay mineral composition of cave sediments and Terra Rossa soils in the karst massif of Montagnola Senese in Italy. The source area of the investigated sediment could be in the Gra&#x10d;ac karst polje in the close vicinity of the entrance to the LCC. In the catchment area of the Otu&#x10d;a river (<xref ref-type="fig" rid="F1">Figure&#x20;1B</xref>), approximately 3.5&#xa0;km upstream of today&#x2019;s ponors close to the cave entrance, the river flows through the area covered with Terra Rossa type sediment, as can be seen from the geological map (<xref ref-type="fig" rid="F1">Figure&#x20;1C</xref>, unit 10; <xref ref-type="bibr" rid="B54">Ivanovi&#x107; et&#x20;al., 1973</xref>). Beside kaolinite, vermiculite, illite/muscovite, chlorite and mix-layered clay minerals, samples DC-SP 2 to DC-SP 6 contain minerals from the talc-pyrophillite group (<xref ref-type="table" rid="T2">Table&#x20;2</xref>). Talc-pyrophyllite usually occurs as a minor component in soils, which could be inherited from the parent rock, but they can also form as a result of weathering processes (<xref ref-type="bibr" rid="B138">Weaver, 1989</xref>). According to <xref ref-type="bibr" rid="B133">Velde and Meunier (2010)</xref> talc can be formed directly from pyroxenes. Other secondary minerals that can be formed from pyroxene are vermiculite, smectite, kaolinite or hematite. The analyzed samples contain a small amount of pyroxene group minerals (<xref ref-type="table" rid="T2">Table&#x20;2</xref>) which could have been the parent material for the talc-pyrophyllite group of minerals. Hematite is present only in traces (<xref ref-type="table" rid="T2">Table&#x20;2</xref>), very likely derived from the Terra Rossa. The mineral assemblage determined by the XRD within the analyzed DC-SP samples is comparable to detrital cave sediments within Dinaric karst (<xref ref-type="bibr" rid="B15">Bos&#xe1;k et&#x20;al., 2012</xref>; <xref ref-type="bibr" rid="B148">Zupan Hajna et&#x20;al., 2021</xref>), and e.g., cave sediments from northwestern Oltenia in Romania (<xref ref-type="bibr" rid="B40">Ghenciu, 2017</xref>). When comparing cave sediment compositions, it should be noted that the composition of these sediments depends on the clastic source rocks, and factors such as weathering and/or pedogenesis.</p>
<p>To answer the question about the clastic source rocks and source areas, results of LMF and HMF analysis (<xref ref-type="table" rid="T2">Table&#x20;2</xref>; <xref ref-type="fig" rid="F5">Figure&#x20;5</xref>) were compared to the main lithological units in today&#x2019;s catchment area of the Otu&#x10d;a river and Gra&#x10d;ac karst polje (<xref ref-type="fig" rid="F1">Figures 1B,C</xref>). Underground passages of the LCC are developed in the Tertiary carbonate breccia host rock (<xref ref-type="bibr" rid="B54">Ivanovi&#x107; et&#x20;al., 1973</xref>) (<xref ref-type="fig" rid="F1">Figure&#x20;1C</xref>, unit 8), known as Jelar breccia (<xref ref-type="bibr" rid="B3">Bahun, 1963</xref>, <xref ref-type="bibr" rid="B4">1974</xref>) which is locally composed of various lithic fragments, most commonly related to the lithological composition of underlying rocks. Therefore, the breccia is mainly composed of lithic fragments of Jurassic, Cretaceous, and younger Paleogene carbonate rocks (<xref ref-type="bibr" rid="B55">Ivanovi&#x107; et&#x20;al., 1976</xref>). In the investigated sediment, it was not possible to recognize this carbonate source area, except within the clearly <italic>in situ</italic> formed Bd facies which contains angular boulders of the host rock (<xref ref-type="fig" rid="F11">Figure&#x20;11A</xref>). However, in most of the sediment, the siliciclastic detritus predominates (<xref ref-type="table" rid="T2">Table&#x20;2</xref>) which points to the allochthonous origin of the detritus. According to the results of the HMF and LMF analysis (<xref ref-type="fig" rid="F5">Figure&#x20;5</xref>; <xref ref-type="table" rid="T2">Table&#x20;2</xref>) it can be concluded that the source of the clastic detritus is connected to the wider river Otu&#x10d;a catchment area. Downstream from the source, river Otu&#x10d;a flows through the upper Carboniferous deposits (<xref ref-type="bibr" rid="B121">&#x160;u&#x161;njar et&#x20;al., 1973</xref>) (<xref ref-type="fig" rid="F1">Figure&#x20;1C</xref>, unit 1), mostly clayey shales and sandstones, accompanied by conglomerates. In the composition of the clayey shales quartz, muscovite, chlorite, plagioclase, kaolinite, organic substance, and pyrite can be found. In the layered, well-sorted, and fine-grained sandstones the detritus is composed mainly of quartz, muscovite, chlorite, lithic fragments, and a small amount of plagioclase (<xref ref-type="bibr" rid="B116">Soka&#x10d; et&#x20;al., 1976</xref>). Traces of such mineral assemblages can be recognized within the composition of LMF from LCC where quartz grains prevail (84&#x2013;92%), together with the occurrence of muscovite and feldspar (<xref ref-type="table" rid="T2">Table&#x20;2</xref>), while the presence of chlorite and kaolinite is confirmed by XRD analysis (<xref ref-type="table" rid="T2">Table&#x20;2</xref>). Potential source area could be found within the clastic-pyroclastic series of middle to upper Triassic (<xref ref-type="fig" rid="F1">Figure&#x20;1C</xref>, unit 3), composed of shales, quartz-calcarenites, subgraywacke sandstones, calcilutites, breccias, and tuffitic rocks (<xref ref-type="bibr" rid="B116">Soka&#x10d; et&#x20;al., 1976</xref>). The subgraywacke shows pronounced domination of quartz, followed by chert, plagioclase, and platy minerals such as biotite, muscovite, and chlorite, all comparable with the composition of the analyzed samples (<xref ref-type="table" rid="T2">Table&#x20;2</xref>; <xref ref-type="fig" rid="F5">Figure&#x20;5</xref>). Furthermore, other rocks within the clastic-pyroclastic series contain angular quartz, chert/radiolarite, and in smaller amounts fragments of older sandstones and shales, similar to the investigated samples. The predominance of pyroxenes among the THM in investigated samples points to the upper part of the middle Triassic clastic-pyroclastic series as the possible source rocks (<xref ref-type="bibr" rid="B116">Soka&#x10d; et&#x20;al., 1976</xref>). Pyroxenes, as chemically unstable detrital constituents, possibly indicate higher erosion rates of the source rocks, rapid transport, and short grain residence time in the river (<xref ref-type="bibr" rid="B113">Sevastjanova et&#x20;al., 2012</xref>; <xref ref-type="bibr" rid="B135">Wacha et&#x20;al., 2019</xref>). Although present, garnet grains are not the dominant phase within the composition of THM in LCC detrital sediments (Chapter 4.3, <xref ref-type="fig" rid="F5">Figure&#x20;5</xref>) but the overall mineral assemblage is almost identical except for the absence of corundum and apatite. The apatite absence could be related to the sample preparation process and chemical dissolution. The relatively abundant well-rounded opaque grains within HMF resembles to Fe-Mn nodules, which are common in clastic cave sediments and Terra Rossa type soils and paleosols (<xref ref-type="bibr" rid="B31">Durn et&#x20;al., 2018</xref>; unpublished data) (<xref ref-type="fig" rid="F5">Figures 5D,E,H</xref>). Their occurrence could be related to the earlier mentioned Terra Rossa type soil in the Gra&#x10d;ac karst polje (<xref ref-type="fig" rid="F1">Figure&#x20;1B</xref>, <xref ref-type="bibr" rid="B54">Ivanovi&#x107; et&#x20;al., 1973</xref>). To conclude, the mineral composition of the clastic detritus in which there is high proportion of quartz, followed by feldspars, muscovite, opaque minerals, biotite, chlorite, chromite, pyroxenes, zircon, rutile, garnets, epidote, zoisite/clinozoisite group minerals and chromite can indicate a diverse source area, but the one that is geographically connected to the nearby river Otu&#x10d;a catchment&#x20;area.</p>
</sec>
<sec id="s5-2">
<title>Sedimentary Facies and Depositional Environments</title>
<p>Due to the unique characteristic of cave environments, it is sometimes difficult to interpret specific depositional conditions within sequences of detrital cave deposits. Cave sediments represent the most complex terrestrial depositional environment where the law of superposition is often violated, facies are usually diachronous and re-deposition along the same cave passage is very common (<xref ref-type="bibr" rid="B140">White, 2007</xref>; <xref ref-type="bibr" rid="B146">Zupan Hajna et&#x20;al., 2020</xref> and references within). However, we were able to describe and interpret three lithofacies types within the sedimentary profile DC-SP in the LCC; the Breakdown facies (Bd), the Diamicton facies (Di) and the Slackwater facies (Sw) (<xref ref-type="fig" rid="F3">Figure&#x20;3A</xref>; <xref ref-type="table" rid="T1">Table&#x20;1</xref>).</p>
<p>Sediments of the Bd facies are commonly formed by the gravitational collapse of the host-rock or speleothems from the ceiling of the caves. Such facies type has been described in other caves, and is considered as an autochthonous type of sediment (e.g., <xref ref-type="bibr" rid="B16">Bosch and White, 2004</xref>; <xref ref-type="bibr" rid="B140">White, 2007</xref>). The transport of material, in this case, is very short, as is confirmed by the angularity of collapsed blocks and poor sorting of the debris (<xref ref-type="table" rid="T1">Table&#x20;1</xref>; <xref ref-type="fig" rid="F11">Figure&#x20;11A</xref>). Collapsed sediments are common near the cave entrances (e.g., <xref ref-type="bibr" rid="B12">Bo&#x10d;i&#x107; et&#x20;al., 2012</xref>; <xref ref-type="bibr" rid="B42">Haddad-Martim et&#x20;al., 2017</xref>), although they can often be seen as big accumulations of unsorted boulders and cobbles on the floor of big chambers within caves (<xref ref-type="bibr" rid="B36">Forn&#xf3;s et&#x20;al., 2014</xref>). Deposition is, besides other processes, often triggered by the cryofracturing process within cave channels during the cold periods (<xref ref-type="bibr" rid="B139">White, 2019</xref>). Hence, it can be assumed that sedimentation of the Bd facies in the channel of the LCC could also happen during a relatively cold period. That assumption is confirmed by palynological data which shows that the base of the investigated profile was formed during a period of cold and dry climate (see Chapter 4.4). The silty matrix within the Bd facies is the result of secondary infiltration (e.g., <xref ref-type="bibr" rid="B83">Martini, 2011</xref>) due to the existence of occasional and relatively insignificant water flow within the open cave channel. This is evidenced by the preserved/transformed phytoclast ratio according to <xref ref-type="bibr" rid="B112">Sebag et&#x20;al. (2006)</xref>. Even though this index was introduced by <xref ref-type="bibr" rid="B112">Sebag et&#x20;al. (2006)</xref> for Holocene alluvial sediments, our data show a distribution of the index (<xref ref-type="fig" rid="F10">Figure&#x20;10</xref>) which allows us to distinguish the paleoenvironment, confirming a transition from a fluvial paleoenvironment in the lower (older) part of the section (DC-SP 1&#x2014;Bd facies) to a non-aquatic terrestrial paleoenvironment toward the youngest part of the section (DC-SP 8&#x2014;Late Bronze Age). Such interpretation shows a good correlation with the sedimentological data. The appearance of microscopic-sized charcoal remains (<xref ref-type="fig" rid="F7">Figure&#x20;7B</xref>) and possible traces of guano and bone remains (<xref ref-type="table" rid="T2">Table&#x20;2</xref>) between collapsed blocks of the Bd facies indicate that during the deposition of the Bd facies the cave channel was already fully developed and well connected to the surface in an open-air environment. Charcoal remains could indicate occurrences of wildfires in the area. Deposits of this type are formed during the vadose, air-filled stages of cave development (<xref ref-type="bibr" rid="B46">Hill, 1999</xref>). However, the distribution of palynofacies shown on <xref ref-type="fig" rid="F10">Figure&#x20;10</xref> in the lower part of the section, could also be a reflection of palynomorph transport by hydrological mechanism of cave drip water into the vadose cave channel.</p>
<fig id="F10" position="float">
<label>FIGURE 10</label>
<caption>
<p>Diagram for discrimination of depositional environments according to palynofacies analysis applied to samples from DC-SP profile in the Lower Cerova&#x10d;ka Cave with optical indices &#x201c;AOM contents&#x201d; (aquatic or microbial production) and &#x201c;preserved/transformed ratio&#x201d; (preservation degree of terrestrial plant debris) (according to <xref ref-type="bibr" rid="B112">Sebag et&#x20;al., 2006</xref>).</p>
</caption>
<graphic xlink:href="feart-09-672229-g010.tif"/>
</fig>
<p>Coevally to the Bd facies, the sediments of the Di facies were deposited (<xref ref-type="fig" rid="F11">Figures 11A,D</xref>), as implied by their lateral contact. The red clayey silt resembles the Terra Rossa type soils and palaeosols whose genesis within the karst has not yet been unambiguously resolved. Polygenetic, detrital, and residual origins are most commonly mentioned (<xref ref-type="bibr" rid="B29">Durn et&#x20;al., 2007</xref>). Similar red clayey-silty sediments in caves are interpreted as a composite of detritus introduced into the cave, and the insoluble residue from the dissolution of the host rock (e.g., <xref ref-type="bibr" rid="B52">Iacoviello and Martini, 2012</xref>). Mostly allogenic origin of the Di sediment within LCC is confirmed by mineralogy reflecting the composition of the river Otu&#x10d;a drainage area (Samples DC-SP 2, 3 in <xref ref-type="table" rid="T2">Table&#x20;2</xref>; Chapters 4.3 and 5.1). Although the vast majority of this interval is formed by finer sediment (Samples DC-SP 2, 3; <xref ref-type="fig" rid="F4">Figure&#x20;4A</xref>), a significant number of larger clasts and bone fragments were found within (<xref ref-type="fig" rid="F3">Figures 3A</xref>, <xref ref-type="fig" rid="F11">11A</xref>), could indicate depositional mechanisms by non-selective agents within cave specific environments. The aeolian contribution could also played important role in creating fine-grained sediment sequences within the cave. However, in the close vicinity of the LCC, there are no occurrences of loess on the surface (<xref ref-type="fig" rid="F1">Figure&#x20;1C</xref>). Loess and loess-like deposits were widespread in the Adriatic region during oxygen isotope stage 3 (<xref ref-type="bibr" rid="B136">Wacha et&#x20;al., 2018</xref>; <xref ref-type="bibr" rid="B145">Zhang et&#x20;al., 2018</xref>). Nevertheless, aeolian sediments also play a significant role in the forming of polygenetic Terra Rossa type of soils (<xref ref-type="bibr" rid="B29">Durn et&#x20;al., 2007</xref>) which were found in the river Otu&#x10d;a catchment area (<xref ref-type="fig" rid="F1">Figure&#x20;1C</xref>, unit 9). According to paleontological data, it is necessary to mention that most probably intertwining of the depositional and biological processes resulted in today&#x2019;s distribution of clasts and fossil remains within the sediment. Despite the fact that all parts of the <italic>U. spelaeus</italic> body are represented (Chapter 4.5), there is a lack of articulated sets and high fragmentation with indications of certain movements and destruction of the faunal material within the sampled DC-SP 2 interval of Di facies (<xref ref-type="table" rid="T1">Table&#x20;1</xref>; <xref ref-type="fig" rid="F3">Figure&#x20;3</xref>). In density-mediated attrition, low-density elements are quickly destructed and removed from the assemblage (<xref ref-type="bibr" rid="B73">Lyman, 1994</xref>), which does not explain why there are very few fragments of major limb bones. The post-depositional disturbance is possible. However, based on data on body parts representation and fragmentation, it is possible that a larger dispersal of the skeletal material occurred even before, when bear carcasses were lying on the fossil surface of the cave. Except for a single questionable finding of cut marks (<xref ref-type="bibr" rid="B126">Trbojevi&#x107; Vuki&#x10d;evi&#x107; and Babi&#x107;, 2008</xref>), no traces of butchering were previously found on cave bear bones from LCC, so it is safe to assume that hominins were not responsible for the accumulation and dispersal of cave bear bones. Since the cave has probably been used for a very long time by several generations of cave bears (<xref ref-type="bibr" rid="B77">Malez, 1965b</xref>), lack of articulated skeletons can be also explained as a result of trampling by other cave bears. However, high fragmentation and under-representation of major long bones may be due to scavenging activities of large carnivore predators, whose presence should not be ruled out despite the lack of corresponding taphonomic traces within the analyzed assemblage. Bears used caves as shelter and for hibernation, and were often targeted by other large carnivores, mostly hyenas, who entered deep into caves in search of them (<xref ref-type="bibr" rid="B27">Diedrich, 2012</xref>). To conclude, described lack of complete skeletons or articulated sets, as well as high fragmentation undoubtedly indicate certain movements and destruction of the faunal material within the sediment, although taphonomic processes could have a significant influence (Chapter 4.5). Given the chaotic arrangement of clasts and random orientation of long bones with no visible textures in the clayey silt, the facies of the red clayey silt is interpreted as Di facies (e.g., <xref ref-type="bibr" rid="B16">Bosch and White, 2004</xref>; <xref ref-type="bibr" rid="B140">White, 2007</xref>; <xref ref-type="bibr" rid="B42">Haddad-Martim et&#x20;al., 2017</xref>). This type of sediment could be formed by high-density debris flows within the caves and by the redeposition of older clastic cave deposits. Distinguishing facies types within this type of deposits is not always unambiguous because cave sediments deposited near cave entrances are often transported by nonselective mechanisms such as slumping, creeping, and collapsing. Such processes result in the fact that they are mainly built of similar ratios of silt, clay and sand, which makes it difficult to recognize unconformities (<xref ref-type="bibr" rid="B42">Haddad-Martim et&#x20;al., 2017</xref>). The chaotic character of the Di facies (see description in <xref ref-type="table" rid="T1">Table&#x20;1</xref>) and the possible redeposition of the sediments, is supported by the results of the palynological analysis which shows signs of redeposition, for example high (relative) values of phytoclasts fragments especially corroded charcoal remains (<xref ref-type="fig" rid="F10">Figure&#x20;10</xref>). Deposition of the Di facies sediments took place during a period of a colder and drier climate (Chapter 4.4). Such occurrence of poorly sorted fossiliferous sediments coincides with the results of previous research within the LCC (e.g., <xref ref-type="bibr" rid="B79">Malez, 1960b</xref>). Namely, the horizon of the Di facies could be related to deposits earlier described in the caves of the nearby Gra&#x10d;ac area as sediment composed of reddish-brown phosphate clays with numerous osteological remains of the Late Pleistocene with traces of the Upper Paleolithic culture (<xref ref-type="bibr" rid="B79">Malez, 1960b</xref>; <xref ref-type="bibr" rid="B55">Ivanovi&#x107; et&#x20;al., 1976</xref>). Those sediments were correlated to the Last Glacial Period. Although cave bears are one of the most abundant taxon recovered from Pleistocene cave sites in Croatia (<xref ref-type="bibr" rid="B87">Miracle, 1991</xref>), with Cerova&#x10d;ke caves being one of the most important cave bear sites (<xref ref-type="bibr" rid="B96">Paunovi&#x107; et&#x20;al., 1999</xref>), our paleontological data are limited by the relatively modest sample size. Therefore, <italic>U. spelaeus</italic> remains within the investigated sequence cannot be used as a precise stratigraphic marker. The earliest appearance of the <italic>U. spelaeus</italic> dates back to the end of the Middle-Late Pleistocene transition, and it became extinct in central Europe during the LGM, around 24 ka BP (<xref ref-type="bibr" rid="B66">Kurt&#xe9;n, 1958</xref>, <xref ref-type="bibr" rid="B67">1968</xref>; <xref ref-type="bibr" rid="B94">Pacher and Stuart, 2009</xref>). Within Dinaric karst there are dated cave bear specific sites (e.g., Kri&#x17e;na jama) with ages of cave bear thanatocenoses around 47&#x2013;45 ka and &#x3e;94 ka BP (<xref ref-type="bibr" rid="B15">Bos&#xe1;k et&#x20;al., 2012</xref>). To establish a chronological framework of the Di facies of the LCC luminescence dating was performed. Although it is a new approach in the region, the application of luminescence dating techniques has proven to be a suitable chronometer in cave settings (e.g., <xref ref-type="bibr" rid="B88">Montanari et&#x20;al., 2019</xref>). In general, luminescence techniques enable the determination of depositional ages of sediments by determining the point in time when quartz or potassium-rich feldspar grains were last exposed to daylight during transport before final deposition (for the basic principles of luminescence dating see <xref ref-type="bibr" rid="B101">Preusser et&#x20;al., 2008</xref>, <xref ref-type="bibr" rid="B106">Rhodes 2011</xref>; <xref ref-type="bibr" rid="B143">Wintle 2008</xref>). According to the obtained luminescence age, the sediment directly overlying cave bear remains entered the cave environment 53.7&#x20;&#xb1; 6.9 ka ago (<xref ref-type="table" rid="T3">Table&#x20;3</xref>), which correlates well with oxygen isotope stage 3 (OIS3). The obtained date does not necessarily indicate the time of deposition at the investigated site but the time when the sediment entered the cave environment. It also indicates that this part of the sequence is not older than &#x223c;54 ka. The end of deposition of the Di facies is marked by a change in color from reddish to gray to yellow and the appearance of a discontinuous flowstone level (<xref ref-type="table" rid="T1">Table&#x20;1</xref>; <xref ref-type="fig" rid="F11">Figure&#x20;11C</xref>). Similar it is also described in other caves of the investigated area (reddish-brown phosphate clays phase covered with flowstone&#x2014;<xref ref-type="bibr" rid="B55">Ivanovi&#x107; et&#x20;al., 1976</xref>).</p>
<fig id="F11" position="float">
<label>FIGURE 11</label>
<caption>
<p>Facies types and age on profile DC-SP in the Lower Cerova&#x10d;ka Cave <bold>(A)</bold> Facies distribution with indicated sampling spots, <bold>(B)</bold> detail from upper part of Slackwater facies with indicated sampling spot and luminescence age, <bold>(C)</bold> <sup>14</sup>C age with indicated sampling spot within flowstone fragment, <bold>(D)</bold> detail from diamicton facies with visible larger clasts and bone fragments of <italic>Ursus spelaeus</italic> with indicated sampling spot and luminescence age [authors of photographs <bold>(A)</bold> DTP, <bold>(B)</bold>&#x2013;<bold>(D)</bold> NB].</p>
</caption>
<graphic xlink:href="feart-09-672229-g011.tif"/>
</fig>
<p>A thin layer of laminated flowstone composed of columnar sparry calcite was determined with visible crystal growth directions (<xref ref-type="sec" rid="s10">Supplementary Material S2</xref>). Millimeter-sized sparry calcite possibly indicate a relatively high growth rate of the flowstone. We assumed <italic>in situ</italic> genesis of the flowstone because platy fragments (<xref ref-type="fig" rid="F9">Figures 9A&#x2013;C</xref>) are distributed at the same horizontal level with visible distinct uneven base/nucleation plane shoving traces of the underlying silty-clayey sediment (<xref ref-type="sec" rid="s10">Supplementary Material S2</xref>). However, due to the thin and discontinuous horizon (<xref ref-type="fig" rid="F3">Figure&#x20;3A</xref>), an allochthonous origin is not excluded. If <italic>in situ</italic>, the flowstone within the sedimentary profile is an indicator of change in the cave environment since their formation implies the absence of the detrital input (<xref ref-type="bibr" rid="B42">Haddad-Martim et&#x20;al., 2017</xref>). Flowstones could be formed from sheets of flowing water derived from fissures or major conduits (<xref ref-type="bibr" rid="B33">Fairchild et&#x20;al., 2006</xref>) or as subaqueous flowstones fed with turbulent underground stream water (Wr&#xf3;blewski et&#x20;al., 2017). As valuable marker horizons for dating, they were previously used in this region as source material for acquiring <sup>14</sup>C ages within caves (e.g., <xref ref-type="bibr" rid="B12">Bo&#x10d;i&#x107; et&#x20;al., 2012</xref>). Within this study the obtained <sup>14</sup>C age from the flowstone is supported by the pIRIR<sub>225</sub> dating of the sediment horizon below the flowstone.</p>
<p>Comparing &#x3b4;<sup>13</sup>C of the LCC speleothem sample (<xref ref-type="table" rid="T4">Table&#x20;4</xref>) of 5.3&#x2030; to the Modri&#x10d; cave speleothem (<xref ref-type="bibr" rid="B107">Rudzka et&#x20;al., 2012</xref>) that has a mean value of &#x2212;7.37&#x2030; (2<italic>&#x3c3;</italic> &#x3d; 1.74&#x2030;), it could be concluded that the speleothem in the Modri&#x10d; cave had a lower amount of DCF. Therefore, the most likely date for the LCC speleothem would be the OxCal Reservoir function date 17,949&#x2013;17,562&#xa0;cal BC (median 17,758&#xa0;cal BC) for DCF &#x3d; 15%. The formation of a relatively thin flowstone layer within the sedimentary profile in LCC, therefore, could be related to the known period-related phenomena in the border zone between the temperate Mediterranean and the periglacial/glacial parts of Europe (<xref ref-type="bibr" rid="B120">Suri&#x107; and Jura&#x10d;i&#x107;, 2010</xref>) when the formation of speleothems were rare or slow. Speleothem deposition ceased during the Last Glacial Maximum (LGM) in most of Europe and began again around 15 ka ago (<xref ref-type="bibr" rid="B39">Gascoyne, 1992</xref>; <xref ref-type="bibr" rid="B70">Lowe and Walker, 1997</xref>; <xref ref-type="bibr" rid="B85">Mihevc, 2001</xref>; <xref ref-type="bibr" rid="B120">Suri&#x107; and Jura&#x10d;i&#x107;, 2010</xref>). According to our data, the pronounced collapse processes and deposition of both Bd and Di facies sediments happened probably during local LGM, sometimes before &#x223c;19.5 ka from today (<sup>14</sup>C age 17,949&#x2013;17,562&#xa0;cal BC&#x2014;<xref ref-type="table" rid="T4">Table&#x20;4</xref>, <xref ref-type="fig" rid="F11">Figure&#x20;11C</xref>), before postglacial warming commenced. The Dinaric mountains were glaciated during the Middle and Late Pleistocene (<xref ref-type="bibr" rid="B49">Hughes and Woodward, 2009</xref>). Therefore, periglacial influence on the LCC could be expected. If the flowstone is allochthonous (e.g., spallation from the ceiling), the obtained age could still be used as the oldest possible date when deposition of the upper section of the DC-SP profile commenced. Sedimentation in a calm aquatic environment therefore set on after &#x223c;19.5 ka ago, as evidenced by the sedimentary filling of the cave channel which covers the flowstone marker horizon. This phase is characterized by gray to yellow laminated silt (<xref ref-type="table" rid="T1">Table&#x20;1</xref>; <xref ref-type="fig" rid="F3">Figure&#x20;3A</xref>) which can be interpreted as slackwater deposit (Sw facies) (e.g., <xref ref-type="bibr" rid="B16">Bosch and White, 2004</xref>; <xref ref-type="bibr" rid="B140">White, 2007</xref>; <xref ref-type="bibr" rid="B52">Iacoviello and Martini, 2012</xref>; Ballesteros et&#x20;al., 2017). These fine-grained sediments (<xref ref-type="fig" rid="F4">Figure&#x20;4</xref>) entered the cave after flood events and settled during calmer conditions with very low flow velocities (often submerged cave channels). The allogenic origin of the Sw sediment is confirmed by the mineralogy, reflecting the composition of the river Otu&#x10d;a drainage area (Samples DC-SP 5&#x2013;7 in <xref ref-type="table" rid="T2">Table&#x20;2</xref>; Chapters 4.3 and 5.1). Although the detritus was transported underground by turbulent flows rich in suspended sediment, the final depositional mechanism of this sediment type is very likely related to deposition from stagnant water suspension, as evidenced by the particle size characteristics and the lamination of the sediment. This is also confirmed by the fining upwards sequence observed in the upper part of the Sw facies interval (<xref ref-type="fig" rid="F4">Figure&#x20;4B</xref>; <xref ref-type="table" rid="T1">Table&#x20;1</xref>). Slight reduction of the grain size from the base to the top indicating a decrease in the hydrodynamic energy conditions of the cave, is commonly observed within the Sw facies (<xref ref-type="bibr" rid="B36">Forn&#xf3;s et&#x20;al., 2014</xref>). This is also confirmed by the palynofacies analysis, results of which indicate sedimentation in a calm palustrine environment (<xref ref-type="fig" rid="F10">Figure&#x20;10</xref>). However, the laminated structure of the sediment in the lower part of the SW facies followed by a slight increase of the sand content (<xref ref-type="fig" rid="F3">Figures 3A</xref>, <xref ref-type="fig" rid="F4">4B</xref>), described as vertical alterations of silty laminae and silty-sandy laminae (<xref ref-type="table" rid="T1">Table&#x20;1</xref>), could also resemble sediments deposited in stagnant hydrological conditions in regions prone to glaciation. Nearby areas of southern Velebit Mt. were prone to glaciation, documented with morphological moraine features and with glacial and glacio-fluvial sediments (<xref ref-type="bibr" rid="B93">Nikler, 1973</xref>; <xref ref-type="bibr" rid="B62">Krklec et&#x20;al., 2015</xref>; <xref ref-type="bibr" rid="B80">Marjanac and Marjanac, 2016</xref>; <xref ref-type="bibr" rid="B134">Veli&#x107; et&#x20;al., 2017</xref>). The retreat of mountain glaciers in the southern Velebit Mt. is therefore dated roughly around 20.7&#x2013;22.7&#xa0;ka ago (<xref ref-type="bibr" rid="B108">Sar&#x131;kaya et&#x20;al., 2020</xref>). Even so, there is no data about glacial chronology and processes in the very close vicinity of LCC. It should be mentioned that warming and deglaciation in the inland part of the Dinarides commenced mainly after 12.5&#xa0;ka BP. It can be seen from increased speleothem growth in the Dinaric karst (<xref ref-type="bibr" rid="B47">Horvatin&#x10d;i&#x107; et&#x20;al., 2003</xref>). Hence, we assume that it is highly possible to recognize glacial/periglacial influence on the deposition of Sw facies. According to our data, the Sw sediments were deposited during the Late Pleistocene (starting after &#x223c;19.5&#xa0;ka). In caves within glaciated regions, similar varve-like deposits are common (<xref ref-type="bibr" rid="B35">Ford and Williams, 2007</xref>). Even though the grain-size curves of the Sw facies (<xref ref-type="fig" rid="F4">Figure&#x20;4A</xref>) resemble the varve-like sediments (<xref ref-type="bibr" rid="B131">Valen et&#x20;al., 1997</xref>; <xref ref-type="bibr" rid="B35">Ford and Williams, 2007</xref>), the glacial-related depositional environment through the whole profile of the Sw facies sediments is ambiguous and needs further proof. Grain-size distribution curves themselves do not point to an unambiguous conclusion, it is necessary to compare them with known sediment ages to resolve the glacial-related origin of the laminae (<xref ref-type="bibr" rid="B125">Tischler et&#x20;al., 2020</xref>).</p>
<p>The termination of allogenic siliciclastic sedimentation in an aquatic environment and consequently the end of the ponor function of this part of the LCC channel cannot be precisely dated within our research. Nevertheless, our data revealed a relatively young age in comparison to the known data within the wider area of the Dinaric karst where cave sediments cover the time span of the last &#x223c;5&#xa0;Ma&#xa0;years (<xref ref-type="bibr" rid="B146">Zupan Hajna et&#x20;al., 2020</xref>; <xref ref-type="bibr" rid="B148">Zupan Hajna et&#x20;al., 2021</xref>). We can conclude that this pronounced sedimentary environment shift is visible in the profile DC-SP with the onset of a Holocene Late Bronze Age layer (<xref ref-type="bibr" rid="B128">Tresi&#x107; Pavi&#x10d;i&#x107;, 2020</xref>). As known, the cessation of allogeneic sedimentation in caves is mostly controlled by tectonics and therefore related to changes in the hydrological regimes due to the separation of cave systems from active watercourses (<xref ref-type="bibr" rid="B146">Zupan Hajna et&#x20;al., 2020</xref>). At Postojnska Cave, the sequence follows the series of events: formation of the fault, growth of the initial conduit due to groundwater circulation through the fault, infilling of the conduit with allogenic sediment, abandonment due to regional base level lowering, and continued motion along the fault (<xref ref-type="bibr" rid="B109">Sasowsky et&#x20;al., 2003</xref>). Locally in LCC, it could be related to the permanent neotectonic uplift of this area (<xref ref-type="bibr" rid="B98">Prelogovi&#x107;, 1975</xref>). Especially pronounced uplift along the main NW&#x2013;SE faults, e.g., along the Lika fault (<xref ref-type="fig" rid="F1">Figure&#x20;1C</xref>), was recorded during the Pliocene and Quaternary (<xref ref-type="bibr" rid="B98">Prelogovi&#x107;, 1975</xref>). Maximum uplift of the local mountains was calculated of up to 1,200&#xa0;m, with vertical shifts on individual faults averaging from 300 to 500&#xa0;m (<xref ref-type="bibr" rid="B98">Prelogovi&#x107;, 1975</xref>). The sedimentary profile DC-SP, and the obtained data therefore possibly reveal the sedimentation history of the youngest inactive cave level within Mt. Crnopac. The same phases in the development of allogenic cave sediments occurred earlier in the higher cave levels within the mountain. It is evidenced with similar facies types (Sw) of detrital sediments which were found within the hypsometrically highest horizontal level of the todays CCS (<xref ref-type="bibr" rid="B122">Talaja and Kure&#x10d;i&#x107;, 2017</xref>). Considering that caves and their sediments are often related to the former base level and can conserve this information for long periods (<xref ref-type="bibr" rid="B92">Neuhuber et&#x20;al., 2021</xref>), the average offset rate of local ongoing uplift/base level drop can be roughly estimated. Considering the relative displacement value of &#x223c;80&#xa0;m between today&#x2019;s LCC entrance (at 624&#x20;m a.s.l.), and the recent active ponor phase on the polje level we have calculated the relative displacement rate. It is based on the obtained <sup>14</sup>C age of 17,949&#x2013;17,562&#xa0;cal BC (before approximately 19.5&#xa0;ka from today) of the flowstone strata identified within the DC-SP profile (<xref ref-type="table" rid="T4">Table&#x20;4</xref>). The displacement rate gives us a relatively high value up to &#x223c;0.004&#x20;m per year. The calculated result is higher and not unambiguously comparable with fault slip rates calculated in the area of External Dinarides (<xref ref-type="bibr" rid="B56">Kastelic and Carafa, 2012</xref>). Therefore, due to scarce data without numerous variables, we believe that the computed rate could only be used as a rough estimation and basis for further research. Even if we use the combination of absolute and relative methods in order to get an accurate and robust age estimate (<xref ref-type="bibr" rid="B44">H&#xe4;uselman et&#x20;al., 2015</xref>), the critical problems identified are lack of data regarding the timing of the cessation of the allogenic sediment input. The archeological data suggests that the LCC was used for specific purposes during the Late Bronze Age (<xref ref-type="bibr" rid="B128">Tresi&#x107; Pavi&#x10d;i&#x107;, 2020</xref>), such as food storage and as a temporary dwelling in specific circumstances which surely indicate already ceased sediment input. However, due to the possible large time gap between the cessation of the Sw deposition and the onset of the Late Bronze Age, we cannot use that data for accurate calculations.</p>
</sec>
</sec>
<sec sec-type="conclusion" id="s6">
<title>Conclusion</title>
<p>The allogenic cave deposits in Croatia have been poorly explored, especially from the point of view of their origin and depositional mechanisms. Numerical dating is also absent. This is the first detailed study of detrital cave sediments with reliable luminescence age constraints in the Croatian part of the Dinaric karst region. The presented data are a significant contribution to solving the complex stratigraphy and genesis of a multilevel cave system of Mt. Crnopac and Dinaric karst. Our conclusions are as follows:<list list-type="simple">
<list-item>
<label>&#x2003;&#x2022;</label>
<p>The genesis of the LCC and its entrance channel is related to the denudation effect of the sinking waters of the Gra&#x10d;ac karst polje, mainly under saturated conditions.</p>
</list-item>
<list-item>
<label>&#x2022;</label>
<p>Within the investigated sedimentary profile (DC-SP) three lithofacies types were identified: Breakdown deposits (Bd), Diamicton deposits (Di), and Slackwater deposits (Sw) covered with an archaeological Late Bronze Age and Modern period deposits.</p>
</list-item>
<list-item>
<label>&#x2022;</label>
<p>The mineral composition of cave detrital sediments points to an allochthonous origin, derived from the wider Otu&#x10d;a river catchment&#x20;area.</p>
</list-item>
<list-item>
<label>&#x2022;</label>
<p>The source rocks which derived the siliciclastic detritus found within the entrance channel of the LCC belong to the upper Carboniferous clastic series, middle to upper Triassic clastic-pyroclastic series, Terra Rossa type of sediments, and arguably in some extent to the insoluble remnant of the host&#x20;rock.</p>
</list-item>
<list-item>
<label>&#x2022;</label>
<p>Sedimentary facies analysis coupled with the palynofacies analysis revealed changes in depositional events within the LCC, ranging from intensive collapse processes with fluvial influence through re-deposition by mechanisms of high density flows to the forming of stagnant water environments with laminated sediments, and finally to the terrestrial environment with pronounced human activity.</p>
</list-item>
<list-item>
<label>&#x2022;</label>
<p>Numerous bones of <italic>U. spelaeus</italic> were found, giving us a broad estimation of the stratigraphic position of the Di facies sediments spanning from the early Late Pleistocene to the Last Glacial Maximum.</p>
</list-item>
<list-item>
<label>&#x2022;</label>
<p>The lack of complete skeletons or even articulated sets, as well as high fragmentation, indicate movements and destruction of the faunal material as a result of taphonomic processes coupled with re-deposition within the fossiliferous interval.</p>
</list-item>
<list-item>
<label>&#x2022;</label>
<p>Deposition of first allochthonous detrital cave sediment sequence (Di facies) within the LCC channel commenced around or after &#x223c;54 ka ago as evidenced by luminescence dating. For the first time in Croatia, luminescence dating contributed to resolving the chronostratigraphy of clastic sedimentary sequence within the cave environment.</p>
</list-item>
<list-item>
<label>&#x2022;</label>
<p>The major shift in sedimentation mechanisms between collapse and redeposition processes, and deposition within stagnant water conditions commenced through the period after 19.5 ka from today up to the onset of the Late Bronze&#x20;Age.</p>
</list-item>
<list-item>
<label>&#x2022;</label>
<p>The cessation of allogenic sedimentation within the LCC is related to the permanent neotectonic uplift of the area, especially pronounced uplift along the main NW&#x2013;SE faults.</p>
</list-item>
</list>
</p>
</sec>
</body>
<back>
<sec id="s7">
<title>Data Availability Statement</title>
<p>The original contributions presented in the study are included in the article/<xref ref-type="sec" rid="s10">Supplementary Material</xref>, further inquiries can be directed to the corresponding author.</p>
</sec>
<sec id="s8">
<title>Author Contributions</title>
<p>TK conceptualized, drafted and prepared the paper with the contribution of all coauthors. DP (archaeology), TK, NB, and LW (geology and sedimentology) conducted the field work and sampling. TK conducted detailed sedimentological and mineralogical analysis as well as laser diffraction particle size distribution. NB performed morphological analysis. KB performed palynological, SR macropaleontological and AG XRD analysis. CL performed luminescence dating and all related analyses and data evaluation. AS performed radiocarbon dating. DP acquired photogrammetric data. LR performed laser scanning of the cave and prepared the 3D model. MF accompanied the luminescence dating part and gave advice during lab work and elaboration of the manuscript. All authors reviewed the manuscript and approved the final version.</p>
</sec>
<sec sec-type="COI-statement" id="s9">
<title>Conflict of Interest</title>
<p>Author DP, was employed by the company Kaducej d.o.o. </p>
<p>The remaining authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.</p>
</sec>
<ack>
<p>The authors are thankful to the archaeological firm Kaducej Ltd. which conducted rescue archaeological excavation at LCC, from March to May 2019. Excavation gives us insight into geological layers, and the opportunity to sample sediments. All relevant photogrammetric data about the test trench was also provided by Kaducej Ltd. The archaeological excavation was the first part of the revitalization project: Centre of Excellence Cerovac Caves - Sustainable Management of Natural Heritage and the Karst Underground, under the direction of Public Institution Park prirode Velebit with partners Zadar County, Public Institution Natura&#x2014;Jadera and Zagreb Speleological Union, co-funded by the European Regional Development Fund. The authors would also like to thank to Mirjana Dru&#x161;kovi&#x107;, Dragica Kova&#x10d;i&#x107;, Antun &#x160;krti&#x107; and Damir Galovi&#x107; from Croatian Geological Survey for the sample preparations. This work was partially funded by the University of Zagreb within the project &#x201c;Geomorphological and hydromorphological research at selected sites of the Dinaric Karst in Croatia.&#x201d; The research was also supported by the Croatian Geological Survey through program funding provided by the Croatian Ministry of Science and Education. The authors would like to thank the editor (Dr. Aurel Per&#x015F;oiu), and the two reviewers (Dr. Andrea Zerboni, and Dr. Christos Pennos) for their comments.</p>
</ack>
<sec id="s10">
<title>Supplementary Material</title>
<p>The Supplementary Material for this article can be found online at: <ext-link ext-link-type="uri" xlink:href="https://www.frontiersin.org/articles/10.3389/feart.2021.672229/full#supplementary-material">https://www.frontiersin.org/articles/10.3389/feart.2021.672229/full&#x23;supplementary-material</ext-link>
</p>
<supplementary-material xlink:href="DataSheet2.PDF" id="SM1" mimetype="application/PDF" xmlns:xlink="http://www.w3.org/1999/xlink"/>
<supplementary-material xlink:href="Image1.JPEG" id="SM2" mimetype="application/JPEG" xmlns:xlink="http://www.w3.org/1999/xlink"/>
<supplementary-material xlink:href="DataSheet1.PDF" id="SM3" mimetype="application/PDF" xmlns:xlink="http://www.w3.org/1999/xlink"/>
</sec>
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