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<ri:Resource created="2023-11-16T08:31:26Z" status="active" updated="2026-08-03T07:31:16Z" 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>Periods and classifications of RR Lyrae in M15</title><shortName>J/MNRAS/502/818</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/502/818</identifier><altIdentifier>doi:10.26093/cds/vizier/bg-fp-sj</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hoffman A.M.</name></creator><creator><name>Murakami Y.S.</name></creator><creator><name>Zheng W.</name></creator><creator><name>Stahl B.E.</name></creator><creator><name>Filippenko A.V.</name></creator><date role="Updated">2026-08-03T07:31:16Z</date><date role="Created">2023-11-16T08:31:26Z</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>globular-star-clusters</subject><subject>visible-astronomy</subject><description>We present measurements of the periods, amplitudes, and types of 74 RR Lyrae stars in the globular cluster M15 derived from Nickel 1m telescope observations conducted at Lick Observatory in 2019 and 2020. Of these RR Lyrae stars, two were previously reported but without a determination of the period. In addition, we identify five Type II Cepheid variable stars for which we report three novel period determinations, and a further 34 stars with uncertain classifications and periods. 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