<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2009-12-29T15:59:12Z" status="active" updated="2025-05-19T09:50:00Z" 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>Solar-like oscillations in red giants</title><shortName>J/A+A/506/465</shortName><identifier>ivo://CDS.VizieR/J/A+A/506/465</identifier><altIdentifier>doi:10.26093/cds/vizier.35060465</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hekker S.</name></creator><creator><name>Kallinger T.</name></creator><creator><name>Baudin F.</name></creator><creator><name>De Ridder J.</name></creator><creator><name>Barban C.</name></creator><creator><name>Carier F.,Hatzes A.P.</name></creator><creator><name>Weiss W.W.</name></creator><creator><name>Baglin A.</name></creator><date role="Updated">2016-08-02T10:56:47Z</date><date role="Created">2009-12-29T15:59:12Z</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>giant-stars</subject><subject>photometry</subject><description>We present the results of a statistical study of solar-like oscillations in red-giant stars observed with CoRoT in its exoplanet field during the first long run (LRc01) when the satellite was pointed towards the galactic centre. From the approximately 11400 stars observed, the giants are selected using infrared colours (not dereddened) and the solar-like oscillation signature (a broad envelope with oscillation power at frequencies below 120 microHz). This oscillation power is either detected by a semi-automatic procedure (sap), or by a manual inspection by eye (man).</description><source format="bibcode">2009A&amp;A...506..465H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/506/465</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/B/corot">B/corot : CoRoT observation log (CoRoT, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/479/865">J/A+A/479/865 : CoRoT exoplanet candidates (Loeillet+, 2008)</relatedResource><relatedResource>http://smsc.cnes.fr/COROT : COROT Home Page</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/506/465</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/506/465</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/506/465</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/506/465</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/506/465</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/506/465</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/A+A/506/465/table1 (Oscillation parameters of 778 red giants observed with CoRoT)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/506/465/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/506/465/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/506/465/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>290.58484</ra><dec>1.69915</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/29951 30122 30292-30293 30295 30301 30464 30466-30467 30472-30473</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/506/465?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/506/465/table1</name><description>Oscillation parameters of 778 red giants observed with CoRoT</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>CoRoT</name><description>COROT identification number \linkRole{details from CoRoT for this star}</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>Vmag</name><description>Apparent magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Method</name><description>[sap man] Method used (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>numax</name><description>Frequency of maximum oscillation power</description><unit>uHz</unit><ucd>em.freq;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>deltanu</name><description>? Large frequency separation</description><unit>uHz</unit><ucd>em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_deltanu</name><description>Number of methods used for deltanu determination</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column></table></schema></tableset></ri:Resource>