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<ri:Resource created="2019-02-12T07:26:58Z" 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>Circumstellar disks in the Upper Sco association</title><shortName>J/AJ/156/75</shortName><identifier>ivo://CDS.VizieR/J/AJ/156/75</identifier><altIdentifier>doi:10.26093/cds/vizier.51560075</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Esplin T.L.</name></creator><creator><name>Luhman K.L.</name></creator><creator><name>Miller E.B.</name></creator><creator><name>Mamajek E.E.</name></creator><date role="Updated">2019-03-11T08:37:05Z</date><date role="Created">2019-02-12T07:26:58Z</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>stellar-associations</subject><subject>molecular-clouds</subject><subject>accretion</subject><subject>stellar-spectral-types</subject><subject>line-intensities</subject><subject>infrared-photometry</subject><subject>pre-main-sequence-stars</subject><description>We have performed a survey for new members of the Upper Sco association that have circumstellar disks using mid-infrared photometry from the Wide-field Infrared Survey Explorer (WISE). Through optical and near-infrared spectroscopy, we have confirmed 185 candidates as likely members of Upper Sco with spectral types ranging from mid-K to M9. They comprise ~36% of the known disk-bearing members of the association. We also have compiled all available mid-infrared photometry from WISE and the Spitzer Space Telescope for the known members of Upper Sco, resulting in a catalog of data for 1608 objects. We have used these data to identify the members that exhibit excess emission from disks and we have classified the evolutionary stages of those disks with criteria similar to those applied in our previous studies of Taurus and Upper Sco. Among 484 members with excesses in at least one band (excluding five Be stars), we classify 296 disks as full, 66 as evolved, 19 as transitional, 22 as evolved or transitional, and 81 as evolved transitional or debris. Many of these disks have not been previously reported, including 129 full disks and 50 disks that are at more advanced evolutionary stages.</description><source format="bibcode">2018AJ....156...75E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/156/75</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/II/311">II/311 : WISE All-Sky Data Release (Cutri+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/314">II/314 : UKIDSS-DR8 LAS, GCS and DXS Surveys (Lawrence+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</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/651/L49">J/ApJ/651/L49 : Upper Sco OB association IRAC observations (Carpenter+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/671/1800">J/ApJ/671/1800 : SCUBA observations of {rho} Oph cloud (Andrews+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/688/377">J/ApJ/688/377 : Low-mass objects in Upper Scorpius. II. (Slesnick+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/1646">J/ApJ/705/1646 : Debris disks in Upper Sco (Carpenter+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/712/925">J/ApJ/712/925 : Transition circumstellar disks in Ophiuchus (Cieza+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/758/31">J/ApJ/758/31 : IR photometry for members of Upper Sco (Luhman+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/429/903">J/MNRAS/429/903 : New brown dwarf discs in Upper Scorpius (Dawson+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/579/A66">J/A+A/579/A66 : Accretion in {rho}-Ophiucus (Manara+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/71">J/AJ/156/71 : K2 Campaign 2: young disk-bearing stars in Sco + Oph</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/76">J/AJ/156/76 : New young stars and brown dwarfs in Upper Sco (Luhman+, 2018)</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/AJ/156/75</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/156/75</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/156/75</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/156/75</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/156/75</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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WISE W2 (4.6 micron) band magnitude (5)</description><unit>mag</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W2mag</name><description>[0.01/0.22]? Error in W2mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_W2mag</name><description>Flag on W2mag (4)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>W3mag</name><description>[1.03/12.18]? WISE W3 (12 micron) band magnitude (5)</description><unit>mag</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W3mag</name><description>[0.01/0.46]? Error in W3mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_W3mag</name><description>Flag on W3mag (4)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>W4mag</name><description>[-0.57/8.88]? WISE W4 (22 micron) band magnitude (5)</description><unit>mag</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W4mag</name><description>[0.01/0.53]? Error in W4mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_W4mag</name><description>Flag on W4mag (4)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Exc4.5</name><description>Excess present in [4.5]? (Y=Yes, N=No)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Exc8.0</name><description>Excess present in [8.0]? (Y=Yes, N=No)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Exc24</name><description>Excess present in [24]? (Y=Yes, N=No)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>ExcW2</name><description>Excess present in W2? (Y=Yes, N=No)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>ExcW3</name><description>Excess present in W3? (Y=Yes, N=No)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>ExcW4</name><description>Excess present in W4? (Y=Yes, N=No)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column></table></schema></tableset></ri:Resource>