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<ri:Resource created="2012-05-18T15:25:28Z" 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>Variable stars in NGC 5024 (M53)</title><shortName>J/MNRAS/416/2265</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/416/2265</identifier><altIdentifier>doi:10.26093/cds/vizier.74162265</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Arellano Ferro A.</name></creator><creator><name>Figuera Jaimes R.</name></creator><creator><name>Giridhar S.</name></creator><creator><name>Bramich D.M.,Hernandez Santisteban J.V.</name></creator><creator><name>Kuppuswamy K.</name></creator><date role="Updated">2024-07-15T20:16:37Z</date><date role="Created">2012-05-18T15:25:28Z</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>globular-star-clusters</subject><subject>variable-stars</subject><subject>photometry</subject><description>We report CCD V and I time series photometry of the globular cluster NGC 5024 (M53). The technique of difference image analysis has been used which enables photometric precisions better than 10mmag for stars brighter than V~18.5mag even in the crowded central regions of the cluster. The high photometric precision has resulted in the discovery of two new RR1 stars and 13 SX Phe stars. A detailed identification chart is given for all the variable stars in the field of our images of the cluster. 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J/A+A/358/547</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Per4</name><description>? Period from Dekany &amp; Kovacs, 2009 Cat. J/A+A/507/803</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>DK09</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/MNRAS/416/2265/table3</name><description>Fourier coefficients Ak for k=0,1,2,3,4, and phases {phi}(21, 31 and 41) for the 19 RR0-type and 9 RR1-type variables for which the Fourier decomposition fit was successful</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Fourier coefficient A3 (V mag)</description><unit>mag</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_A3</name><description>? rms uncertainty on A3</description><unit>mmag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>A4</name><description>? Fourier coefficient A4 (V mag)</description><unit>mag</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_A4</name><description>? rms uncertainty on A4</description><unit>mmag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>phi21</name><description>Phase {phi}_21_</description><unit>rad</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_phi21</name><description>rms uncertainty on phi21</description><unit>mrad</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>phi31</name><description>? 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