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<ri:Resource created="2000-03-16T10:14:22Z" 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 observations of old clusters in the LMC</title><shortName>J/ApJ/527/199</shortName><identifier>ivo://CDS.VizieR/J/ApJ/527/199</identifier><altIdentifier>doi:10.26093/cds/vizier.15270199</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Johnson J.A.</name></creator><creator><name>Bolte M.</name></creator><creator><name>Stetson P.B.</name></creator><creator><name>Hesser J.E.</name></creator><creator><name>Somerville R.S.</name></creator><date role="Updated">2000-03-16T09:14:34Z</date><date role="Created">2000-03-16T10:14:22Z</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>hertzsprung-russell-diagram</subject><subject>magellanic-clouds</subject><subject>photometry</subject><description>We present V, V-I color-magnitude diagrams (CMDs) for three old star clusters in the Large Magellanic Cloud (LMC): NGC 1466, NGC 2257, and Hodge 11. Our data extend {~}3 mag below the main-sequence turnoff, allowing us to determine accurate relative ages and the blue straggler frequencies. Based on a differential comparison of the CMDs, any age difference between the three LMC clusters is less than 1.5 Gyr. Comparing their CMDs to those of M92 and M3, the LMC clusters, unless their published metallicities are significantly in error, are the same age as the old Galactic globulars. The similar ages to Galactic globulars are shown to be consistent with hierarchical clustering models of galaxy formation. The blue straggler frequencies are also similar to those of Galactic globular clusters. We derive a true distance modulus to the LMC of (m - M)_0_ = 18.46 {+/-} 0.09 [assuming (m - M)_0_ = 14.61 for M92] using these three LMC clusters.</description><source format="bibcode">1999ApJ...527..199J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/527/199</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/300/665">J/MNRAS/300/665 : HST VI Photometry of Six LMC Old Globular Clusters</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/527/199</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/527/199</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/527/199</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/527/199</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/527/199</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/527/199</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/527/199/table2a</name><description>V and I photometry of NGC 1466</description><column><name>Vmag</name><description>V band magnitude</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><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 pixel position on Chip</description><unit>pix</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ypos</name><description>Y pixel position on Chip</description><unit>pix</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>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 V-I</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chip</name><description>Chip number (1 is the PC chip)</description><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/ApJ/527/199/table2b</name><description>V and I photometry of NGC 2257</description><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 V-I</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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