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<ri:Resource created="2023-11-03T10:48:42Z" status="active" updated="2025-06-13T15:25:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>FOSSIL. III. LCs of Trans-Neptunian Objects</title><shortName>J/ApJS/267/33</shortName><identifier>ivo://CDS.VizieR/J/ApJS/267/33</identifier><altIdentifier>doi:10.26093/cds/vizier.22670033</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ashton E.</name></creator><creator><name>Chang C.-K.</name></creator><creator><name>Chen Y.-T.</name></creator><creator><name>Lehner M.J.</name></creator><creator><name>Wang S.-Y.,Alexandersen M.</name></creator><creator><name>Choi Y.-J.</name></creator><creator><name>Fraser W.C.</name></creator><creator><name>Granados Contreras A.P.</name></creator><creator><name>Ito T.,JeongAhn Y.</name></creator><creator><name>Ji J.</name></creator><creator><name>Kavelaars JJ</name></creator><creator><name>Kim M.-J.</name></creator><creator><name>Lawler S.M.</name></creator><creator><name>Li J.,Lin Z.-Y.</name></creator><creator><name>Lykawka P.S.</name></creator><creator><name>Moon H.-K.</name></creator><creator><name>More S.</name></creator><creator><name>Munoz-Gutierrez M.A.,Ohtsuki K.</name></creator><creator><name>Pike R.E.</name></creator><creator><name>Terai T.</name></creator><creator><name>Urakawa S.</name></creator><creator><name>Yoshida F.</name></creator><creator><name>Zhang H.,Zhao H.</name></creator><creator><name>Zhou J.-L.</name></creator><creator><name>The FOSSIL Collaboration</name></creator><date role="Updated">2023-12-11T20:12:56Z</date><date role="Created">2023-11-03T10:48:42Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>asteroids</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>surveys</subject><description>From the first phase of the high-cadence Formation of the Outer Solar System: an Icy Legacy (FOSSIL) survey, we analyzed lightcurves, ranging from one to four nights in length, of 371 trans-Neptunian objects (TNOs) for periodicity. We found 29 TNOs with periodic lightcurves, one of which is a good candidate for a close/contact binary. Another of the periodic FOSSIL TNOs could potentially have the fastest of all known TNO spin rates, with a period of 1.3hr. We do not have total confidence in the period and thus plan to obtain a more detailed lightcurve for confirmation. The periodic TNOs have an average rotation period of 11.2hr, close to the value obtained by Alexandersen+ (2019, J/ApJS/244/19), which had similar cadence, but different from other surveys. In regards to contention in the literature about whether smaller TNOs are more irregular in shape and thus have larger lightcurve amplitudes, we found that there is a weak correlation between absolute magnitude and lightcurve amplitude in a subset of 194 FOSSIL TNOs, even when using the more appropriate brightest (minimum) absolute magnitude instead of the time-averaged value.</description><source format="bibcode">2023ApJS..267...33A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/267/33</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/3023">J/AJ/127/3023 : R magnitudes of Kuiper Belt object 2001QG298 (Sheppard+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/1283">J/A+A/505/1283 : (84922) 2003 VS2 differential light curve (Duffard+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/522/A93">J/A+A/522/A93 : Short-term variability of 29 minor planets (Thirouin+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/241">J/AJ/154/241 : Phot. of a Kuiper Belt object: 2002 CC_249_ (Thirouin+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/244/19">J/ApJS/244/19 : OSSOS. XII. Subaru/HSC obs. of 65 TNOs (Alexandersen+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/157/228">J/AJ/157/228 : Cold Classical TNOs: LCs &amp; rot. properties (Thirouin+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/159/25">J/AJ/159/25 : PS1 light curves and rot. periods of new asteroids (Lo+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/259/7">J/ApJS/259/7 : FOSSIL. II. Subaru/HSC light curves of Hildas (Chang+, 2022)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/267/33</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/267/33</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/267/33</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/267/33</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/267/33</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/267/33</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJS/267/33/table3 (Astronometric and photometric measurements for 435 FOSSIL TNOs)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/267/33/table3?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/267/33/table3?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/267/33/table3?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>225.29811611</ra><dec>-15.06650389</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/4537 4638 4660 6445 11209 6/18127 18156-18157 18160 18162-18163 18168-18169 18556 18558-18559 18644-18646 25759 25779 25785-25789 25826-25827 25832 44813 44815 44824 44826 44848</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/267/33?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJS/267/33/tnos</name><description>List of TNOs with unique IDs; table added by CDS</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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