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<ri:Resource created="2016-04-20T16:09:45Z" 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>JK photometry of 12 galactic globular clusters</title><shortName>J/AJ/150/176</shortName><identifier>ivo://CDS.VizieR/J/AJ/150/176</identifier><altIdentifier>doi:10.26093/cds/vizier.51500176</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cohen R.E.</name></creator><creator><name>Hempel M.</name></creator><creator><name>Mauro F.</name></creator><creator><name>Geisler D.</name></creator><creator><name>Alonso-Garcia J.</name></creator><creator><name>Kinemuchi K.</name></creator><date role="Updated">2017-12-12T14:44:49Z</date><date role="Created">2016-04-20T16:09:45Z</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>globular-star-clusters</subject><subject>infrared-photometry</subject><description>We present wide field near-infrared (near-IR) photometry of 12 Galactic globular clusters, typically extending from the tip of the cluster red giant branch (RGB) to the main sequence turnoff. Using recent homogenous values of cluster distance, reddening and metallicity, the resulting photometry is directly compared to the predictions of several recent libraries of stellar evolutionary models. Of the sets of models investigated, Dartmouth and Victoria-Regina models best reproduce the observed RGB morphology, albeit with offsets in J-K_S_ color which vary in their significance in light of all sources of observational uncertainty. Therefore, we also present newly recalibrated relations between near-IR photometric indices describing the upper RGB versus cluster iron abundance as well as global metallicity. The influence of enhancements in alpha elements and helium are analyzed, and we find that the former affect the morphology of the upper RGB in accord with model predictions. Meanwhile, the empirical relations we derive are in good agreement with previous results, and minor discrepancies can likely be attributed to differences in the assumed cluster distances and reddenings. In addition, we present measurements of the horizontal branch (HB) and RGB bump magnitudes, finding a non-negligible dependence of the near-IR HB magnitude on cluster metallicity. Lastly, we discuss the influence of assumed cluster distances, reddenings and metallicities on our results, finding that our empirical relations are generally insensitive to these factors to within their uncertainties.</description><source format="bibcode">2015AJ....150..176C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/150/176</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/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/202">VII/202 : Globular Clusters in the Milky Way (Harris, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/563/A76">J/A+A/563/A76 : CaII triplet EWs in 30 globulars (Mauro+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/534/A123">J/A+A/534/A123 : Horizontal branch stars in NGC 2808 (Gratton+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/402/1729">J/MNRAS/402/1729 : JHK photometry of 36 GGCs (Valenti+ 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/139">J/A+A/505/139 : Abundances of red giants in 17 GCs (Carretta+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/117">J/A+A/505/117 : Abundances of red giants in 15 GCs (Carretta+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/361/272">J/MNRAS/361/272 : JHKs photometry of 4 Bulge GCs (Valenti+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/351/1204">J/MNRAS/351/1204 : IR Photometry of 10 GGCs (Valenti+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/391/945">J/A+A/391/945 : HST photometry of 74 GGCs (Piotto+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/121/95">J/A+AS/121/95 : Giant stars abundances in 24 clusters (Carretta+ 1997)</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/150/176</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/150/176</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/150/176</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/150/176</accessURL><mirrorURL 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xsi:type="vs:VOTableType">int</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>RAJ2000</name><description>Hour of Right Ascension (J2000) (1)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000) (1)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>(m-M)0</name><description>Cluster distance modulus (2)</description><unit>mag</unit><ucd>phot.mag.distMod</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E(B-V)</name><description>Reddening (2)</description><unit>mag</unit><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>Metallicity from Carretta et al. (2009A&amp;A...508..695C)</description><unit>log(Sun)</unit><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Fe/H]</name><description>Error in [Fe/H]</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[a/Fe]1</name><description>? Observed [{alpha}/Fe] abundance (3)</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[a/Fe]2</name><description>Assumed [{alpha}/Fe] abundance (4)</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[a/Fe]2</name><description>Error in [a/Fe]2</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[M/H]</name><description>Global metallicity (5)</description><unit>log(Sun)</unit><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[M/H]</name><description>Error in [M/H]</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>V-I</name><description>The {Delta}(V-I) index (2)</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_V-I</name><description>Error in V-I</description><unit>mag</unit><ucd>stat.error;phot.color;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</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><column><name>NED</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/150/176/table3</name><description>Clusters photometric catalog</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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