<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2000-03-13T13:24:28Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>HST studies of the WLM globular cluster</title><shortName>J/ApJ/521/577</shortName><identifier>ivo://CDS.VizieR/J/ApJ/521/577</identifier><altIdentifier>doi:10.26093/cds/vizier.15210577</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hodge P.W.</name></creator><creator><name>Dolphin A.E.</name></creator><creator><name>Smith T.R. Mateo M.</name></creator><date role="Updated">2000-03-13T12:24:31Z</date><date role="Created">2000-03-13T13:24:28Z</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>metallicity</subject><subject>globular-star-clusters</subject><subject>two-color-diagrams</subject><subject>galaxies</subject><description>We have obtained V and I images of the lone globular cluster that belongs to the dwarf Local Group irregular galaxy known as WLM. The color-magnitude diagram of the cluster shows that it is a normal old globular cluster with a well-defined giant branch reaching to M_V_=-2.5, a horizontal branch at M_V_=+0.5, and a subgiant branch extending to our photometry limit of M_V_=+2.0. A best fit to theoretical isochrones indicates that this cluster has a metallicity of [Fe/H]=-1.52{+/-}0.08 and an age of 14.8{+/-}0.6 Gyr, thus indicating that it is similar to normal old halo globulars in our Galaxy. From the fit we also find that the distance modulus of the cluster is 24.73{+/-}0.07 and the extinction is A_V_=0.07{+/-}0.06, both values that agree within the errors with data obtained for the galaxy itself by others.</description><source format="bibcode">1999ApJ...521..577H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/521/577</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/521/577</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/521/577</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/521/577</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/521/577</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/521/577</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/521/577</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><facility>HST</facility><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/521/577/table1</name><description>V and I photometry of the WLM globular cluster</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Xpos</name><description>X coordinate on the chip</description><unit>pix</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ypos</name><description>Y coordinate on the chip</description><unit>pix</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vmag</name><description>V band magnitude</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Vmag</name><description>uncertainty in Vmag</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Imag</name><description>I band magnitude</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Imag</name><description>uncertainty in Imag</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>V-I</name><description>V-I color</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_V-I</name><description>uncertainty in the V-I color</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>