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<ri:Resource created="2010-01-04T21:52:41Z" 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>Light curves of Datura and 2003 CL5 asteroids</title><shortName>J/A+A/507/495</shortName><identifier>ivo://CDS.VizieR/J/A+A/507/495</identifier><altIdentifier>doi:10.26093/cds/vizier.35070495</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Vokrouhlicky D.</name></creator><creator><name>Durech J.</name></creator><creator><name>Michalowski T.</name></creator><creator><name>Krugly Y.N.</name></creator><creator><name>Gaftonyuk N.M.,Krysczynska A.</name></creator><creator><name>Colas F.</name></creator><creator><name>Lecacheux J.</name></creator><creator><name>Molotov I.</name></creator><creator><name>Slyusarev I.,Polinska M.</name></creator><creator><name>Nesvorny D.</name></creator><creator><name>Beshore E.</name></creator><date role="Updated">2017-06-26T11:49:53Z</date><date role="Created">2010-01-04T21:52:41Z</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>Research of asteroid families has been recently refreshed by the discovery of very young ones. These families are of great interest because they represent the product of their parent body fragmentation before orbital and physical evolutionary processes can change them. A cluster of seven objects around the largest body (1270) Datura is of particular interest because it has enough known members and resides in the inner part of the main asteroid belt, facilitating observations. We carried out photometric observations of the two largest members of the Datura family - asteroids (1270) Datura and (90265) 2003 CL5 - with the goal of inferring their physical parameters. We also used numerous astrometric observations of Datura-family members in the past few years to revisit the age of this cluster.</description><source format="bibcode">2009A&amp;A...507..495V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/507/495</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/astorb">B/astorb : Orbits of Minor Planets (Bowell+ 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/P+SS/53.925">J/other/P+SS/53.925 : CCD photometry of 23 minor planets (Szekely+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/465/331">J/A+A/465/331 : Asteroid brightness and geometry (Durech+, 2007)</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/A+A/507/495</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/507/495</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/507/495</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/507/495</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/507/495</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/507/495</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/A+A/507/495/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="8*">char</dataType></column><column><name>FileName</name><description>Name of the file containing the light curve</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column></table><table><name>J/A+A/507/495/lc1270</name><description>Lightcurves of asteroid (1270) Datura</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>JD</name><description>JD epoch corrected for the light-time corresponding to the Earth-asteroid distance</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>br</name><description>Relative brightness in intensity units, mean brightness of each lightcurve is unity</description><ucd>phot.flux;em.opt;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sx</name><description>x component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinates</description><unit>AU</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Sy</name><description>y component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinates</description><unit>AU</unit><ucd>pos.dirCos</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SZ</name><description>Z component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinates</description><unit>AU</unit><ucd>pos.cartesian.z</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ex</name><description>x component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinates</description><unit>AU</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ey</name><description>y component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinates</description><unit>AU</unit><ucd>pos.dirCos</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>EZ</name><description>Z component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinates</description><unit>AU</unit><ucd>pos.cartesian.z</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/A+A/507/495/lc90265</name><description>Lightcurves of asteroid (90265) 2003 CL5</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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