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<ri:Resource created="2010-01-26T13:33:13Z" 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>Optical spectroscopy of Cha-II PMS stars</title><shortName>J/ApJ/680/1295</shortName><identifier>ivo://CDS.VizieR/J/ApJ/680/1295</identifier><altIdentifier>doi:10.26093/cds/vizier.16801295</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Spezzi L.</name></creator><creator><name>Alcala J.M.</name></creator><creator><name>Covino E.</name></creator><creator><name>Frasca A.</name></creator><creator><name>Gandolfi D.</name></creator><creator><name>Oliveira I.,Chapman N.</name></creator><creator><name>Evans II N.J.</name></creator><creator><name>Huard T.L.</name></creator><creator><name>Jorgensen J.K.</name></creator><creator><name>Merin B.,Stapelfeldt K.R.</name></creator><date role="Updated">2017-07-05T06:59:38Z</date><date role="Created">2010-01-26T13:33:13Z</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>molecular-clouds</subject><subject>pre-main-sequence-stars</subject><subject>line-intensities</subject><description>We discuss the results of the optical spectroscopic follow-up of pre-main-sequence (PMS) objects and candidates selected in the Chamaeleon II dark cloud based on data from the Spitzer Legacy survey "From Molecular Cores to Planet Forming Disks" (c2d) and from previous surveys. Our sample includes both objects with infrared excess selected according to c2d criteria and referred to as young stellar objects and other cloud members and candidates selected from complementary optical and near-infrared data. We characterize the sample of objects by deriving their physical parameters.</description><source format="bibcode">2008ApJ...680.1295S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/680/1295</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/A+A/399/995">J/A+A/399/995 : SOFI and ISOCAM observations of Cha II (Persi+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/470/281">J/A+A/470/281 : WFI optical photometry in Cha II dark cloud (Spezzi+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/676/427">J/ApJ/676/427 : MIPS and IRAC Chamaeleon II PMS data (Alcala+, 2008)</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/ApJ/680/1295</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/680/1295</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/680/1295</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/680/1295</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/680/1295</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/680/1295</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/ApJ/680/1295/tables (Spectral types, line widths and physical parameters for pre-main-sequence objects and candidates in Cha II)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/680/1295/tables?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/680/1295/tables?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/680/1295/tables?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>191.2767917</ra><dec>-77.3370889</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/10283 6/41126 41127</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/680/1295?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/680/1295/tables</name><description>Spectral types, line widths and physical parameters for pre-main-sequence objects and candidates in Cha II</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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