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<ri:Resource created="2013-06-27T08:37:08Z" 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>Color-metallicity relations. II. M87 GCs</title><shortName>J/ApJ/743/149</shortName><identifier>ivo://CDS.VizieR/J/ApJ/743/149</identifier><altIdentifier>doi:10.26093/cds/vizier.17430149</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yoon S.-J.</name></creator><creator><name>Sohn S.T.</name></creator><creator><name>Lee S.-Y.</name></creator><creator><name>Kim H.-S.</name></creator><creator><name>Cho J.</name></creator><creator><name>Chung C.,Blakeslee J.P.</name></creator><date role="Updated">2013-07-16T13:57:09Z</date><date role="Created">2013-06-27T08:37:08Z</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>hst-photometry</subject><subject>galaxies</subject><description>We here propose a new photometric technique to probe the possible nonlinear nature of globular clusters (GCs) color-metallicity relations (CMRs). In essence, a color distribution of GCs is a "projected" distribution of their metallicities. Since the form of CMRs hinges on which color is used, the shape of color distributions varies depending significantly on the colors. Among other optical colors, the u-band related colors (e.g., u-g and u-z) are theoretically predicted to exhibit significantly less inflected CMRs than other preferred CMRs (e.g., for g-z). As a case study, we performed the Hubble Space Telescope (HST)/WFPC2 archival u-band photometry for the M87 (NGC 4486) GC system with confirmed color bimodality. We show that the u-band color distributions are significantly different from that of g-z and consistent with our model predictions. With more u-band measurements, this method will support or rule out the nonlinear CMR scenario for the origin of GC color bimodality with high confidence.</description><source format="bibcode">2011ApJ...743..149Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/743/149</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/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/197/33">J/ApJS/197/33 : The M87 globular cluster system (Strader+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/703/42">J/ApJ/703/42 : HST photometry of M87 globular clusters (Peng+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/180/54">J/ApJS/180/54 : GC candidates in ACS Virgo survey (Jordan+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/382/1947">J/MNRAS/382/1947 : CT1 photometry in NGC 1399 and NGC 4486 (Forte+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/866">J/AJ/131/866 : Hot populations in M87 globular clusters (Sohn+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/613/279">J/ApJ/613/279 : ACS Virgo Cluster Survey. III. M87 (Jordan+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/559/812">J/ApJ/559/812 : Globular cluster system in M87 (Hanes+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/513/733">J/ApJ/513/733 : Globular cluster system in M87 (Kundu+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/115/1801">J/AJ/115/1801 : VRI photometry of M87 globular clusters (Harris+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/106/493">J/AJ/106/493 : Globular clusters in M87 (Lee+, 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/73/671">J/ApJS/73/671 : M87 globular clusters BVI photometry (Couture+, 1990)</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/ApJ/743/149</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/743/149</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/743/149</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/743/149</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/743/149</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/743/149</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/743/149/table5 (The u-, g-, and z-band magnitudes and their observational errors for the M87 GCs)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/743/149/table5?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/743/149/table5?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/743/149/table5?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>187.7056427</ra><dec>12.3909702</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/27765</spatial><spectral>2.1350832807657816e-19 6.367785378457404e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/743/149?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/743/149/table5</name><description>The u-, g-, and z-band magnitudes and their observational errors for the M87 GCs</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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