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<ri:Resource created="2020-11-20T08:12:05Z" 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>SpT &amp; NIR color excess of Solar-type stars</title><shortName>J/AJ/160/130</shortName><identifier>ivo://CDS.VizieR/J/AJ/160/130</identifier><altIdentifier>doi:10.26093/cds/vizier.51600130</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lewin C.D.</name></creator><creator><name>Howell E.S.</name></creator><creator><name>Vervack R.J.</name></creator><creator><name>Fernandez Y.R.</name></creator><creator><name>Magri C.,Marshall S.E.</name></creator><creator><name>Crowell J.L.</name></creator><creator><name>Hinkle M.L.</name></creator><date role="Updated">2021-06-17T12:58:04Z</date><date role="Created">2020-11-20T08:12:05Z</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>g-stars</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>two-color-diagrams</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><subject>stellar-spectral-types</subject><description>Although solar-analog stars have been studied extensively over the past few decades, most of these studies have focused on visible wavelengths, especially those identifying solar-analog stars to be used as calibration tools for observations. As a result, there is a dearth of well-characterized solar analogs for observations in the near-infrared, a wavelength range important for studying solar system objects. We present 184 stars selected based on solar-like spectral type and V-J and V-K colors whose spectra we have observed in the 0.8-4.2{mu}m range for calibrating our asteroid observations. Each star has been classified into one of three ranks based on spectral resemblance to vetted solar analogs. Of our set of 184 stars, we report 145 as reliable solar-analog stars, 21 as solar analogs usable after spectral corrections with low-order polynomial fitting, and 18 as unsuitable for use as calibration standards owing to spectral shape, variability, or features at low to medium resolution. We conclude that all but five of our candidates are reliable solar analogs in the longer wavelength range from 2.5 to 4.2{mu}m. The average colors of the stars classified as reliable or usable solar analogs are V-J=1.148, V-H=1.418, and V-K= 1.491, with the entire set being distributed fairly uniformly in R.A. across the sky between -27{deg} and +67{deg} in decl.</description><source format="bibcode">2020AJ....160..130L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/160/130</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/183">II/183 : UBVRI Photometric Standards (Landolt 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/259">I/259 : The Tycho-2 Catalogue (Hog+ 2000)</relatedResource><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/VI/19">VI/19 : UBV Photoelectric Sequences in SA 92-115 (Landolt 1973)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/555/932">J/ApJ/555/932 : IR fluxes of solar-type stars (Spangler+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/89">J/ApJ/705/89 : IRS spectra of solar-type stars (Lawler+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/181/62">J/ApJS/181/62 : Survey of young solar analogs (Metchev+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/212/10">J/ApJS/212/10 : WISE IR excesses for stars within 75pc (Patel+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/587/A65">J/A+A/587/A65 : Visible and near-infrared solar spectra (Reiners+, 2016)</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/160/130</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/160/130</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/160/130</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/160/130</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/160/130</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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23279 23282 23513 23545 23706 23943 24099 24155 24254 24256 24295 24341 24374 24454 24523 24542 24774 25300 25555 25586 26256 26440 26615 27752 27780 28386 28490 28871 28962 29127 29422 29591 29756 30043 30233 30357 30481 30540 31156 31334 31351 31382 31428 31796 31843 31886 32028 32069 32100 32128 32173 32288 32589 32751 36072 36794 40661 40932 42933 43876 44814 44865 44909 45051 48352 48470 48572 48865 48908 49114</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/160/130?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/160/130/table2</name><description>Rankings for solar analog candidates</description><column><name>Name</name><description>Star Name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType><flag>primary</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SAO</name><description>SAO number</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>SpT</name><description>Spectral Type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>[0/23] 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>[5.46/12.43] V band magnitude (1)</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>(V-J)</name><description>[0.77/2.12] V-J color (1)</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>[0.88/2.43] V-H color (1)</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-Ks)</name><description>[0.95/2.5] V-Ks color (1)</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Vmag</name><description>[0.001/0.11] Uncertainty in Vmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_(V-J)</name><description>[0.01/0.11] Uncertainty in (V-J)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_(V-H)</name><description>[0.01/0.12] Uncertainty in (V-H)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_(V-Ks)</name><description>[0.01/10] Uncertainty in (V-Ks)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rank</name><description>[1/3] Rank based on the magnitude ({Delta}) of the deviation of the relative slope (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Notes</name><description>Notes (3)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Fset</name><description>Indicates that the star is in the final set of primary solar catalog (link to table1)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/AJ/160/130/table1</name><description>Final set of 17 primary solar analogs</description><column><name>SAO</name><description>SAO number</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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