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<ri:Resource created="2021-12-14T09:09:18Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>CCD photometry of 23 minor planets</title><shortName>J/other/PSS/53.9</shortName><identifier>ivo://CDS.VizieR/J/other/PSS/53.925</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Szekely P.</name></creator><creator><name>Kiss L.L.</name></creator><creator><name>Szabo Gy.M.</name></creator><creator><name>Sarneczky K.</name></creator><creator><name>Csak B.</name></creator><creator><name>Varadi M.,Meszaros Sz.</name></creator><date role="Updated">2022-11-18T08:20:57Z</date><date role="Created">2021-12-14T09:09:18Z</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>ccd-photometry</subject><description>We present CCD photometric observations of 23 main-belt asteroids, of which 8 have never been observed before thus the data of these objects are the first in the literature. The majority showed well detectable light variations, exceeding 0.1m. We have determined synodic periods for 756 Lilliana (9.36),1270 Datura (3.4), 1400 Tirela (13.36), 1503 Kuopio (9.98), 3682 Welther (3.59), 7505 Furushu (4.14) and 11436 1969 QR (2.6), while uncertain period estimates were possible for 469 Argentina (12.3), 546 Herodias (10.4) and 1026 Ingrid (5.3). The shape of the lightcurves of 3682 Welther changed on a short time-scale and showed dimmings that might be attributed to eclipses in a binary system. For the remaining objects, only lower limits of the periods and amplitudes were concluded.</description><source format="bibcode">2005P&amp;SS...53..925S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/PSS/53.925</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/other/PSS/53.925</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/other/PSS/53.925</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/other/PSS/53.925</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/other/PSS/53.925</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/other/PSS/53.925</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/other/PSS/53.925</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><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/></coverage><tableset><schema><name>default</name><table><name>J/other/PSS/53.925/objects</name><description>Asteroid list</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ast</name><description>Asteroid number</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Asteroid name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column><column><name>FiltLC</name><description>[RX] Filter of LC light curve</description><ucd>instr.bandpass</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>LC</name><description>Name of the file containing the light curve</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>FiltCL</name><description>[RX] Filter of CL composite light curve</description><ucd>instr.bandpass</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>CL</name><description>Name of the file containing the composite light curve</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>FiltCL2</name><description>[RX] Filter of CL2 composite light curve</description><ucd>instr.bandpass</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>CL2</name><description>Name of the file containing the second composite light curve</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column></table></schema></tableset></ri:Resource>