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<ri:Resource created="2018-03-05T13:12:29Z" 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>Astro-photometric catalog of the core of NGC 5139</title><shortName>J/ApJ/842/6</shortName><identifier>ivo://CDS.VizieR/J/ApJ/842/6</identifier><altIdentifier>doi:10.26093/cds/vizier.18420006</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bellini A.</name></creator><creator><name>Anderson J.</name></creator><creator><name>Bedin L.R.</name></creator><creator><name>King I.R.</name></creator><creator><name>van der Marel R.P.,Piotto G.</name></creator><creator><name>Cool A.</name></creator><date role="Updated">2021-11-16T13:43:59Z</date><date role="Created">2018-03-05T13:12:29Z</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>hst-photometry</subject><subject>proper-motions</subject><description>We have constructed the most comprehensive catalog of photometry and proper motions ever assembled for a globular cluster (GC). The core of {omega}Cen (NGC 5139) has been imaged over 650 times through WFC3's UVIS and IR channels for the purpose of detector calibration. There exist from 4 to over 60 exposures through each of 26 filters stretching continuously from F225W in the UV to F160W in the infrared. Furthermore, the 11yr baseline between these data and a 2002 ACS survey has allowed us to more than double the proper-motion accuracy and triple the number of well-measured stars compared to our previous groundbreaking effort. This totally unprecedented complete spectral coverage of over 470000 stars within the cluster's core, from the tip of the red giant branch down to the white dwarfs, provides the best astro-photometric observational database yet to understand the multiple-population phenomenon in any GC. In this first paper of the series, we describe in detail the data-reduction processes and deliver the astro-photometric catalog to the astronomical community.</description><source format="bibcode">2017ApJ...842....6B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/842/6</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/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><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/A+AS/115/297">J/A+AS/115/297 : BVRI photometry of Central Field of {omega} Cen (Lynga+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/654/915">J/ApJ/654/915 : Deep FORS1 BR photometry of omega Cen (Sollima+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/663/296">J/ApJ/663/296 : omega Cen (NGC5139) subgiants UBVRIc phot. (Villanova+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/493/959">J/A+A/493/959 : UBV(RI)cHalpha photometry in omega Cen (Bellini+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/710/1032">J/ApJ/710/1032 : Proper motions in {omega} Cen (Anderson+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/140/631">J/AJ/140/631 : HST WFC3/UVIS photometry of omega Cen core (Bellini+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/751/6">J/ApJ/751/6 : Radial velocities in {omega} Cen (Da Costa, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/797/115">J/ApJ/797/115 : HSTPROMO I. Observations and NGC7078 results (Bellini+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/844/164">J/ApJ/844/164 : HST astro-photometric data for NGC5139. III. 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The 1{sigma} uncertainty in intercept of PM fit for RA component computed using actual residuals</description><unit>pix</unit><ucd>stat.error;stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>sigmaY</name><description>[0.0005/0.4]? The 1{sigma} uncertainty in intercept of PM fit for DE component computed using actual residuals</description><unit>pix</unit><ucd>stat.error;stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Time</name><description>[0.7/11]? Time baseline; Julian years</description><unit>yr</unit><ucd>instr.baseline</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>errX</name><description>[0.0006/0.3]? 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Apparent Vega magnitude in Filt (1)</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag><flag>indexed</flag></column><column><name>Nf</name><description>[0/71] Number of exposures a star found in</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ng</name><description>[0/71] Number of good measurements</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>indexed</flag></column><column><name>QFIT</name><description>[0/1]? Quality-of-fit parameter</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag><flag>indexed</flag></column><column><name>f_QFIT</name><description>[*] *: QFIT not available (only one measurement in method3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>fL</name><description>[-18.3/20124] Fraction of light in aperture from neighbors</description><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/ApJ/842/6/table6</name><description>Artificial-star-tests file</description><column><name>YInpix</name><description>Input Y pixel position</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>XInpix</name><description>Input X pixel position</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WInmag</name><description>[-14/-3] Input F606W instrumental magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F438WInmag</name><description>[-14/-0.08] Input F438W instrumental magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>XRecpix</name><description>Recovered X pixel position</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>YRecpix</name><description>Recovered Y pixel position</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F606WM1mag</name><description>[-90.1/-0] Recovered method 1 F606W magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F438WM1mag</name><description>[-90.1/-0] Recovered method 1 F438W magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM2mag</name><description>[-90.1/-0] Recovered method 2 F606W magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F438WM2mag</name><description>[-90.1/-0] Recovered method 2 F438W magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM3mag</name><description>[-90.1/-0] Recovered method 3 F606W magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F438WM3mag</name><description>[-90.1/-0] Recovered method 3 F438W magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>