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<ri:Resource created="2010-06-11T09:55:32Z" 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>Low-mass population in {rho} Oph cloud</title><shortName>J/A+A/515/A75</shortName><identifier>ivo://CDS.VizieR/J/A+A/515/A75</identifier><altIdentifier>doi:10.26093/cds/vizier.35150075</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Alves de Oliveira C.</name></creator><creator><name>Moraux E.</name></creator><creator><name>Bouvier J.</name></creator><creator><name>Bouy H.</name></creator><creator><name>Marmo C.</name></creator><creator><name>Albert L.</name></creator><date role="Updated">2010-08-08T12:31:47Z</date><date role="Created">2010-06-11T09:55:32Z</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>young-stellar-objects</subject><subject>infrared-photometry</subject><subject>millimeter-astronomy</subject><subject>photometry</subject><subject>submillimeter-astronomy</subject><description>Star formation theories are currently divergent regarding the fundamental physical processes that dominate the substellar regime. Observations of nearby young open clusters allow the brown dwarf (BD) population to be characterised down to the planetary mass regime, which ultimately must be accommodated by a successful theory. We used near-IR deep images (reaching completeness limits of approximately 20.5mag in J, and 18.9mag in H and Ks taken with the Wide Field IR Camera (WIRCam) at the Canada France Hawaii Telescope (CFHT) to identify candidate members of {rho} Oph in the substellar regime. A spectroscopic follow-up of a small sample of the candidates allows us to assess their spectral type, and subsequently their temperature and membership. We select 110 candidate members of the {rho} Ophiuchi molecular cloud, from which 80 have not previously been associated with the cloud. We observed a small sample of these and spectroscopically confirm six new brown dwarfs with spectral types ranging from M6.5 to M8.25.</description><source format="bibcode">2010A&amp;A...515A..75A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/515/A75</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/ApJ/438/813">J/ApJ/438/813 : Stellar population in {rho} Oph cloud core (Strom+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/112/109">J/ApJS/112/109 : Rho Oph Near-IR Positions and Photometry (Barsony+, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/359/113">J/A+A/359/113 : X-ray and IR study of Rho Oph dark cloud (Grosso+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/372/173">J/A+A/372/173 : ISOCAM observations of rho Ophiuchi cloud (Bontemps+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/55/653">J/PASJ/55/653 : Chandra X-ray flares in rho Ophiuchi (Imanishi+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/426/171">J/A+A/426/171 : H_2_ flows in rho Ophiuchi A (Khanzadyan+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/613/393">J/ApJ/613/393 : X-ray and radio sources in {rho} Oph Core A (Gagne+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/1733">J/AJ/130/1733 : Optical spectroscopy of {rho} Oph stars (Wilking+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/630/381">J/ApJ/630/381 : Mid-IR imaging in {rho} Oph (Barsony+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/429/963">J/A+A/429/963 : XMM-Newton observation of the rho Oph cloud (Ozawa+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/430/549">J/A+A/430/549 : C^18^O/C^17^O near rho Oph (Wouterloot+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/447/609">J/A+A/447/609 : 1.2mm continuum observations in rho Oph cloud (Stanke+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/452/245">J/A+A/452/245 : Near-IR photometry of PMS stars in rho Oph (Natta+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/485/155">J/A+A/485/155 : HK photometry of rho Oph PMS stars (Alves de Oliveira+, 2008)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/515/A75/table4?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>246.3297917</ra><dec>-24.3242778</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/42981 42983 42992</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/515/A75?format=ascii</footprint><waveband>Infrared</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/515/A75/table4</name><description>List of substellar candidate members in {rho} Oph</description><column><name>OName</name><description>Simbad Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Flag</name><description>Properties of the candidate members 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PSF photometry Ks magnitude from WIRCam/CFHT</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ksmag</name><description>? Ksmag photometric error</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[3.6]</name><description>? IRAC 3.6um magnitude as retrieved from the NASA/IPAC Infrared Science Archive</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[3.6]</name><description>? [3.6] photometric error</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[4.5]</name><description>? 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[24] photometric error</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SpT</name><description>MK spectral type as determined in this study</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>AV</name><description>? AV as determined in this study</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ref</name><description>References for {rho} Ophiuchi members, according to these studies (1)</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column></table></schema></tableset></ri:Resource>