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<ri:Resource created="2011-05-20T09:38:21Z" 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>LMC long-period variables from MACHO</title><shortName>J/AJ/136/1242</shortName><identifier>ivo://CDS.VizieR/J/AJ/136/1242</identifier><altIdentifier>doi:10.26093/cds/vizier.51361242</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fraser O.J.</name></creator><creator><name>Hawley S.L.</name></creator><creator><name>Cook K.H.</name></creator><date role="Updated">2011-09-06T08:38:46Z</date><date role="Created">2011-05-20T09:38:21Z</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>visible-astronomy</subject><subject>kron-cousins-photometry</subject><description>We present a new analysis of the long-period variables in the Large Magellanic Cloud (LMC) from the MACHO Variable Star Catalog. Three-quarters of our sample of evolved, variable stars have periodic light curves. We characterize the stars in our sample using the multiple periods found in their frequency spectra. 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