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<ri:Resource created="2006-04-09T08:19:19Z" 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>ACS VI photometry of M31 halo RR Lyrae</title><shortName>J/AJ/127/2738</shortName><identifier>ivo://CDS.VizieR/J/AJ/127/2738</identifier><altIdentifier>doi:10.26093/cds/vizier.51272738</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Brown T.M.</name></creator><creator><name>Ferguson H.C.</name></creator><creator><name>Smith E.</name></creator><creator><name>Kimble R.A.</name></creator><creator><name>Sweigart A.V.,Renzini A.</name></creator><creator><name>Rich R.M.</name></creator><date role="Updated">2023-12-20T08:24:12Z</date><date role="Created">2006-04-09T08:19:19Z</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>variable-stars</subject><subject>photometry</subject><description>We present a complete census of RR Lyrae stars in a halo field of the Andromeda galaxy. These deep observations, taken as part of a program to measure the star formation history in the halo, spanned a period of 41 days with sampling on a variety of timescales, enabling the identification of short- and long-period variables. Although the long-period variables cannot be fully characterized within the time span of this program, the enormous advance in sensitivity provided by the Advanced Camera for Surveys on the Hubble Space Telescope allows accurate characterization of the RR Lyrae population in this field. We find 29 RRab stars with a mean period of 0.594 days, 25 RRc stars with a mean period of 0.316 days, and one RRd star with a fundamental period of 0.473 days and a first-overtone period of 0.353 days. These 55 RR Lyrae stars imply a specific frequency S_RR_~5.6, which is large given the high mean metallicity of the halo, but not surprising given that these stars arise from the old, metal-poor tail of the distribution.</description><source format="bibcode">2004AJ....127.2738B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/127/2738</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/A+A/402/113">J/A+A/402/113 : (RI)c photometry of variables in M31 (Joshi+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/124/234">J/AJ/124/234 : M31 outer halo UBVRI phot. and metallicity (Reitzel+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/125/1298">J/AJ/125/1298 : C star population in outer disk of M31 (Battinelli+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/351/1071">J/MNRAS/351/1071 : POINT-AGAPE Survey. 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