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<ri:Resource created="2010-02-01T13:11:52Z" 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>BVRI photometry of candidate subdwarfs</title><shortName>J/AJ/134/778</shortName><identifier>ivo://CDS.VizieR/J/AJ/134/778</identifier><altIdentifier>doi:10.26093/cds/vizier.51340778</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Marshall J.L.</name></creator><date role="Updated">2017-11-06T12:23:15Z</date><date role="Created">2010-02-01T13:11:52Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>Wide-band photometry</subject><subject>subdwarf-stars</subject><description>Optical (BVRI) photometric measurements of a sample of 564 candidate cool subdwarfs in the nearby halo are presented. The stars generally span the color range 0.4&lt;(B-V)&lt;1.8; hence, the sample is composed of early F- through early M-type stars on the subdwarf sequence. The sample is selected from the revised NLTT catalog of Gould and Salim and Salim and Gould via a reduced proper motion diagram. The photometry is precise and accurate; in particular, for stars with 9&lt;V&lt;13.5 the photometry is accurate to 0.013, 0.015, 0.012, and 0.013mag in V, B-V, V-R, and V-I, respectively. For stars with 13.5&lt;V&lt;16 the photometry is accurate to 0.022, 0.018, 0.013, and 0.018mag in the same bands.</description><source format="bibcode">2007AJ....134..778M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/134/778</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/I/98">I/98 : NLTT Catalogue (Luyten, 1979)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/582/1011">J/ApJ/582/1011 : Revised NLTT Catalog (Salim+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/98/1693">J/AJ/98/1693 : UBVRI photometry of 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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>NLTT</name><description>The NLTT identification number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>n_NLTT</name><description>[1/2]? Possible variability (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>o_NLTT</name><description>Number of observations of NLTT</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</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>Vmag</name><description>The V band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B-V</name><description>The (B-V) color index</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>V-R</name><description>The (V-R) color index</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>V-I</name><description>The (V-I) color index</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>V-J</name><description>The (V-J) color index</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>V-H</name><description>The (V-H) color index</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>V-K</name><description>The (V-K) color index</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>