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<ri:Resource created="2009-10-01T12:18:58Z" 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>Ks photometry of LMC RR Lyrae</title><shortName>J/A+A/502/505</shortName><identifier>ivo://CDS.VizieR/J/A+A/502/505</identifier><altIdentifier>doi:10.26093/cds/vizier.35020505</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Borissova J.</name></creator><creator><name>Rejkuba M.</name></creator><creator><name>Minniti D.</name></creator><creator><name>Catelan M.</name></creator><creator><name>Ivanov V.D.</name></creator><date role="Updated">2017-06-01T08:49:41Z</date><date role="Created">2009-10-01T12:18:58Z</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>magellanic-clouds</subject><subject>variable-stars</subject><subject>infrared-photometry</subject><description>RR Lyrae variable stars are the primary Population II distance indicator. Likewise, the LMC constitutes a key step in the extragalactic distance scale. By combining near-IR photometry and spectroscopically measured metallicities for a homogeneous sample of 50 RR Lyr stars in the Large Magellanic Cloud (LMC), we investigate the metallicity dependence of the period-luminosity relation in the near-infrared (IR), use the newly derived relations to re-derive the distance to the LMC, and compare the distance moduli obtained from RR Lyr and red clump stars.</description><source format="bibcode">2009A&amp;A...502..505B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/502/505</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/II/247">II/247 : Variable Stars in the Large Magellanic Clouds (MACHO, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/53/93">J/AcA/53/93 : OGLE RR Lyrae in LMC (Soszynski+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/423/97">J/A+A/423/97 : LMC RR Lyrae radial velocities. I. (Borissova+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/460/459">J/A+A/460/459 : LMC RR Lyrae Radial velocities. II. 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