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<ri:Resource created="2005-08-22T08:30:40Z" 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>2MASS photometry of hot subdwarf stars</title><shortName>J/AJ/126/1455</shortName><identifier>ivo://CDS.VizieR/J/AJ/126/1455</identifier><altIdentifier>doi:10.26093/cds/vizier.51261455</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Stark M.A.</name></creator><creator><name>Wade R.A.</name></creator><date role="Updated">2023-04-06T16:50:57Z</date><date role="Created">2005-08-22T08:30:40Z</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>early-type-stars</subject><subject>infrared-photometry</subject><subject>subdwarf-stars</subject><subject>horizontal-branch-stars</subject><description>Utilizing the Two Micron All Sky Survey (2MASS) Second Incremental Data Release Catalog, we have retrieved near-IR magnitudes for several hundred hot subdwarfs (sdO and sdB stars) drawn from the Catalogue of Spectroscopically Identified Hot Subdwarfs by Kilkenny et al. (1988SAAOC..12....1K). This sample size greatly exceeds that of previous studies of hot subdwarfs. Examining 2MASS photometry alone or in combination with visual photometry (Johnson BV or Stroemgren uvby) available in the literature, we show that it is possible to identify hot subdwarf stars that exhibit atypically red IR colors, which can be attributed to the presence of an unresolved late-type companion. Utilizing this large sample, we attempt for the first time to define an approximately volume-limited sample of hot subdwarfs. We discuss the considerations, biases, and difficulties in defining such a sample. We find that, of the hot subdwarfs in Kilkenny et al. (1988SAAOC..12....1K), about 40% in a magnitude-limited sample have colors that are consistent with the presence of an unresolved late-type companion. Binary stars are overrepresented in a magnitude-limited sample. In an approximately volume-limited sample the fraction of composite-color binaries is about 30%.</description><source format="bibcode">2003AJ....126.1455S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/126/1455</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></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Notes</name><description>Individual remarks (5)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>SpType</name><description>MK spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>u_B-mag</name><description>Uncertainty flag on B-mag</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>2MASS</name><description>Display the 2MASS data</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Filt</name><description>Filter used in mag (4)</description><ucd>instr.setup</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Seq</name><description>Sequence number assigned by us (G1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>n_Seq</name><description>[*] indicates a note detailed in notes.dat</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>B-mag</name><description>? The (B-mag) color</description><unit>mag</unit><ucd>phot.color</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ID</name><description>First identifier that appears in KHD (Kilkenney et al., 1988SAAOC..12....1K)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>RAJ2000</name><description>Hour of right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>NoteID</name><description>Notes about the designations of the star (2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="38*">char</dataType></column><column><name>SID</name><description>The SIMBAD identifier (3)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="34*">char</dataType></column><column><name>Jmag</name><description>The J-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Jmag</name><description>? The 1 {sigma} error in Jmag (2)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Hmag</name><description>The H-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Hmag</name><description>? The 1 {sigma} error in Hmag (2)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ksmag</name><description>The K_s_ band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Ksmag</name><description>? The 1 {sigma} error in Kmag (2)</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>l_J-Ks</name><description>Limit flag on J-Ks</description><ucd>meta.code.error;phot.color;em.IR.J</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>J-Ks</name><description>The (J-Ks) color (3)</description><unit>mag</unit><ucd>phot.color;em.IR.J;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_J-Ks</name><description>? The 1 {sigma} error in J-Ks</description><unit>mag</unit><ucd>stat.error;phot.color;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/AJ/126/1455/notes</name><description>Individual notes</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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