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<ri:Resource created="2018-01-19T13:02:03Z" 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>HST/Gemini proper motions for Pyxis</title><shortName>J/ApJ/840/30</shortName><identifier>ivo://CDS.VizieR/J/ApJ/840/30</identifier><altIdentifier>doi:10.26093/cds/vizier.18400030</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fritz T.K.</name></creator><creator><name>Linden S.T.</name></creator><creator><name>Zivick P.</name></creator><creator><name>Kallivayalil N.</name></creator><creator><name>Beaton R.L.</name></creator><creator><name>Bovy J.,Sales L.V.</name></creator><creator><name>Sohn T.</name></creator><creator><name>Angell D.</name></creator><creator><name>Boylan-Kolchin M.</name></creator><creator><name>Carrasco E.R.</name></creator><creator><name>Damke G.,Davies R.</name></creator><creator><name>Majewski S.</name></creator><creator><name>Neichel B.</name></creator><creator><name>van der Marel R.</name></creator><date role="Updated">2019-10-10T12:51:53Z</date><date role="Created">2018-01-19T13:02:03Z</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>hst-photometry</subject><description>We present a proper motion measurement for the halo globular cluster Pyxis, using Hubble Space Telescope/ACS data as the first epoch and GeMS/GSAOI Adaptive Optics data as the second, separated by a baseline of ~5 years. This is both the first measurement of the proper motion of Pyxis and the first calibration and use of Multi-Conjugate Adaptive Optics data to measure an absolute proper motion for a faint, distant halo object. Consequently, we present our analysis of the Adaptive Optics data in detail. We obtain a proper motion of {mu}_{alpha}_cos({delta})=1.09+/-0.31mas/yr and {mu}_{delta}_=0.68+/-0.29mas/yr. From the proper motion and line-of-sight velocity, we find that the orbit of Pyxis is rather eccentric, with its apocenter at more than 100kpc and its pericenter at about 30kpc. We also investigate two literature-proposed associations for Pyxis with the recently discovered ATLAS stream and the Magellanic system. Combining our measurements with dynamical modeling and cosmological numerical simulations, we find it unlikely Pyxis is associated with either system. We examine other Milky Way satellites for possible association using the orbit, eccentricity, metallicity, and age as constraints and find no likely matches in satellites down to the mass of Leo II. We propose that Pyxis probably originated in an unknown galaxy, which today is fully disrupted. Assuming that Pyxis is bound and not on a first approach, we derive a 68% lower limit on the mass of the Milky Way of 0.95x10^12^M_{sun}_.</description><source format="bibcode">2017ApJ...840...30F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/840/30</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/195">VII/195 : Globular Clusters in the Milky Way (Harris, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/118/1671">J/AJ/118/1671 : Fornax cluster 4 VI photometry (Buonanno+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/360/185">J/MNRAS/360/185 : VI photometry of the Leo II galaxy (Bellazzini+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/459/423">J/A+A/459/423 : VI and [Fe/H] of Fornax dSph RGB stars (Battaglia+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/465/815">J/A+A/465/815 : Abundances of Sgr dSph stars (Sbordone+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/684/1143">J/ApJ/684/1143 : BHB candidates in the Milky Way (Xue+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/690/1236">J/ApJ/690/1236 : COSMOS photometric redshift catalog (Ilbert+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/4">J/AJ/144/4 : Dwarf galaxies in the Local Group (McConnachie+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/540/A27">J/A+A/540/A27 : Spectroscopy in Galactic globular clusters (Saviane+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/206/10">J/ApJS/206/10 : CANDELS multiwavelength catalog (Galametz+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/779/102">J/ApJ/779/102 : Metallicities of RGB stars in dwarf galaxies (Kirby+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/797/115">J/ApJ/797/115 : HSTPROMO I. 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