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<ri:Resource created="2007-04-25T17:36:28Z" 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>BR photometry of Fornax dSph center</title><shortName>J/AJ/131/912</shortName><identifier>ivo://CDS.VizieR/J/AJ/131/912</identifier><altIdentifier>doi:10.26093/cds/vizier.51310912</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Olszewski E.W.</name></creator><creator><name>Mateo M.</name></creator><creator><name>Harris J.</name></creator><creator><name>Walker M.G.</name></creator><creator><name>Coleman M.G.,Da Costa G.S.</name></creator><date role="Updated">2017-06-20T13:16:28Z</date><date role="Created">2007-04-25T17:36:28Z</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>galaxies</subject><subject>photometry</subject><subject>ccd-photometry</subject><description>We have imaged the recently discovered stellar overdensity located approximately one core radius from the center of the Fornax dwarf spheroidal galaxy using the Magellan Clay 6.5m telescope with the Magellan Instant Camera. Superb seeing conditions allowed us to probe the stellar populations of this overdensity and of a control field within Fornax to a limiting magnitude of R=26. The color-magnitude diagram of the overdensity field is virtually identical to that of the control field, with the exception of the presence of a population arising from a very short (less than 300Myr in duration) burst of star formation 1.4Gyr ago.</description><source format="bibcode">2006AJ....131..912O</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/131/912</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/J/PASP/110/533">J/PASP/110/533 : BR photometry of Fornax bright stars (Stetson+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/134/59">J/A+AS/134/59 : Central Fornax Cluster. 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