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<ri:Resource created="2017-07-27T15:25:49Z" 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>Proper motions and photometry of stars in NGC 3201</title><shortName>J/AJ/153/134</shortName><identifier>ivo://CDS.VizieR/J/AJ/153/134</identifier><altIdentifier>doi:10.26093/cds/vizier.51530134</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sariya D.P.</name></creator><creator><name>Jiang I.-G.</name></creator><creator><name>Yadav R.K.S.</name></creator><date role="Updated">2017-09-04T08:08:07Z</date><date role="Created">2017-07-27T15:25:49Z</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>proper-motions</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>With a high value of heliocentric radial velocity, a retrograde orbit, and suspected to have an extragalactic origin, NGC 3201 is an interesting globular cluster for kinematical studies. Our purpose is to calculate the relative proper motions (PMs) and membership probability for the stars in the wide region of globular cluster NGC 3201. PM based membership probabilities are used to isolate the cluster sample from the field stars. The membership catalog will help address the question of chemical inhomogeneity in the cluster. Archive CCD data taken with a wide-field imager (WFI) mounted on the ESO 2.2m telescope are reduced using the high-precision astrometric software developed by Anderson et al. for the WFI images. The epoch gap between the two observational runs is ~14.3 years. To standardize the BVI photometry, Stetson's secondary standard stars are used. The CCD data with an epoch gap of ~14.3 years enables us to decontaminate the cluster stars from field stars efficiently. The median precision of PMs is better than ~0.8mas/yr for stars having V&lt;18mag that increases up to ~1.5mas/yr for stars with 18&lt;V&lt;20mag. Kinematic membership probabilities are calculated using PMs for stars brighter than V~20mag. An electronic catalog of positions, relative PMs, BVI magnitudes, and membership probabilities in the ~19.7x17arcmin^2^ region of NGC 3201 is presented. We use our membership catalog to identify probable cluster members among the known variables and X-ray sources in the direction of NGC 3201.</description><source format="bibcode">2017AJ....153..134S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/153/134</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/VII/202">VII/202 : Globular Clusters in the Milky Way (Harris, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/801/69">J/ApJ/801/69 : EWs for giant star members of NGC3201 (Mucciarelli+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/584/A59">J/A+A/584/A59 : Proper motions and membership in NGC 6366 (Sariya+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/RMxAA/50.307">J/other/RMxAA/50.307 : RR Lyr light curves in NGC 3201 (Arellano Ferro+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/430/3350">J/MNRAS/430/3350 : Proper motions and membership in NGC 3766 (Yadav+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/62/357">J/AcA/62/357 : Proper motions in 6 globular clusters (Zloczewski+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/543/A87">J/A+A/543/A87 : Stars proper motions and photometry in M55 (Sariya+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/497/371">J/A+A/497/371 : UBVI photometry of NGC 3201 (Kravtsov+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/484/609">J/A+A/484/609 : BVI photometry and proper motions in M67 (Yadav+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/445/155">J/A+A/445/155 : XMM count-rates in M 55 and NGC 3201 (Webb+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/123/279">J/AJ/123/279 : VI Photometry and Variables in NGC 3201 (von Braun+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/131/89">J/A+AS/131/89 : NGC 1750 + NGC 1758 proper motions (Tian+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/454/788">J/ApJ/454/788 : Radial velocities and BV photometry of NGC 3201 (Cote+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/90/83">J/ApJS/90/83 : Binaries in NGC 3201 (Cote+, 1994)</relatedResource><relatedResource>http://archive.eso.org/eso/eso_archive_main.html : ESO Science Archive</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Star</name><description>[1/8322] Running sequential number (ID)</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>[1544.4/4979.9] X position in CCD pixels</description><unit>pix</unit><ucd>pos.cartesian.x;instr.det</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>[247.47/4516.05] Y position in CCD pixels</description><unit>pix</unit><ucd>pos.cartesian.y;instr.det</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>pmRA</name><description>[-104.1/76.65] Relative proper motion along RA {mu}_{alpha}_cos({delta})</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_pmRA</name><description>[0.04/2] rms uncertainty on pmRA {sigma}_{mu}{alpha}cos({delta})_</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmDE</name><description>[-70.9/34.47] Relative proper motion along DEC {mu}_{delta}_</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_pmDE</name><description>[0.06/2] rms uncertainty on pmDE {sigma}_{mu}{delta}_</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Bmag</name><description>[12.55/21.62] Johnson B magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Bmag</name><description>[0/0.17] rms uncertainty on B mag {sigma}_B_</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vmag</name><description>[11.76/20.1] Johnson V magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Vmag</name><description>[0.0001/0.19] rms uncertainty on V mag {sigma}_V_</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Imag</name><description>[9.93/19.12] Cousins I magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Imag</name><description>[0.0002/0.2] rms uncertainty on I mag {sigma}_I_</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mm</name><description>[0/100] Proper-motion membership probability P_{mu}_ (please refer to Section 3 in the paper for details)</description><unit>%</unit><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>R</name><description>Flag 'R' indicates an earlier Reported variable star or X-ray source in the region of NGC 3201 (table3)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table><table><name>J/AJ/153/134/table3</name><description>Membership probability of the known variables in the direction of NGC 3201 and X-ray sources from Webb et al. 2006 (Cat. 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