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<ri:Resource created="2011-12-08T08:13:01Z" 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>EROS-2 Long Period Variables in LMC</title><shortName>J/A+A/536/A60</shortName><identifier>ivo://CDS.VizieR/J/A+A/536/A60</identifier><altIdentifier>doi:10.26093/cds/vizier.35360060</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Spano M.</name></creator><creator><name>Mowlavi N.</name></creator><creator><name>Eyer L.</name></creator><creator><name>Burki G.</name></creator><creator><name>Marquette J.-B.</name></creator><creator><name>Lecoeur-Taibi I.,Tisserand P.</name></creator><date role="Updated">2017-12-07T07:27:13Z</date><date role="Created">2011-12-08T08:13:01Z</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>magellanic-clouds</subject><subject>variable-stars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>The EROS-2 survey has produced a database of millions of time series from stars monitored for more than six years, allowing us to classify some of their sources into different variable star types. Among the so-called, long period variables (LPVs), which are known to follow particular sequences in the period-luminosity diagram, we find long secondary period variables whose variability origin remains a matter of debate. We analyze data for the 856864 variable stars that have been discovered in the Large Magellanic Cloud (LMC) that are present in the EROS-2 database, to detect, classify, and characterize LPVs.</description><source format="bibcode">2011A&amp;A...536A..60S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/536/A60</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/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/454/185">J/A+A/454/185 : EROS-2 microlensing parameters (Hamadache+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/495/249">J/A+A/495/249 : EROS-2 beat Cepheids in Magellanic Clouds (Marquette+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/99/784">J/AJ/99/784 : IR photometry of LMC long-period variables (Hughes+ 1990)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/330/137">J/MNRAS/330/137 : LMC long-period red variables VRc observations (Noda+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/660/1486">J/ApJ/660/1486 : Variability of LMC semiregular variables (Soszynski+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/1242">J/AJ/136/1242 : LMC long-period variables from MACHO (Fraser+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/59/239">J/AcA/59/239 : LMC long-period variables VI light curves (Soszynski+, 2009)</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/536/A60</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/536/A60</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/536/A60</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/536/A60</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/536/A60</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/536/A60</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/536/A60/table3 (Photometric parameters for Long Period Variables)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/536/A60/table3?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/536/A60/table3?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/536/A60/table3?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>80.13023</ra><dec>-69.12148</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>4/2065 2068-2069 5/8259 8265 8268-8269 8280-8281 8284 9352 9354 9376 9378 9384 9386 6/33028-33029 33031 33035 33056-33057 33080-33081 33084-33085 33128-33129 33132-33133 33140-33141 33144 33792-33794 33800 37412 37414 37420 37422 37508 37510 37516 37518 37540 38912-38913</spatial><spectral>8.650015785639275e-20 1.7003137259100215e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/536/A60?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/536/A60/table3</name><description>Photometric parameters for Long Period Variables</description><column><name>Flag</name><description>Note (2)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><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>EROS2</name><description>EROS-2 source name (lmNNNNaNNNNN)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>Remag</name><description>EROS-2 Re magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Be-Re</name><description>EROS-2 Be-Re color index</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ramp</name><description>EROS-2 Re amplitude</description><unit>mag</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Per1</name><description>? First fitted period</description><unit>d</unit><ucd>time.period;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Per2</name><description>? Second fitted period</description><unit>d</unit><ucd>time.period;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Per3</name><description>? Third fitted period</description><unit>d</unit><ucd>time.period;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Per4</name><description>? Fourth fitted period</description><unit>d</unit><ucd>time.period;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Per5</name><description>? 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