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<ri:Resource created="2020-10-09T12:55:21Z" 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 of MW satellites with Gaia &amp; DES</title><shortName>J/ApJ/875/77</shortName><identifier>ivo://CDS.VizieR/J/ApJ/875/77</identifier><altIdentifier>doi:10.26093/cds/vizier.18750077</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pace A.B.</name></creator><creator><name>Li T.S.</name></creator><date role="Updated">2022-09-05T12:40:21Z</date><date role="Created">2020-10-09T12:55:21Z</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>galaxies</subject><subject>photometry</subject><subject>proper-motions</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><description>We present a new, probabilistic method for determining the systemic proper motions of Milky Way (MW) ultra-faint satellites in the Dark Energy Survey (DES). We utilize the superb photometry from the first public data release (DR1) of the DES to select candidate members and cross-match them with the proper motions from the Gaia DR2. We model the candidate members with a mixture model (satellite and MW) in spatial and proper motion space. This method does not require prior knowledge of satellite membership and can successfully determine the tangential motion of 13 DES satellites. With our method, we present measurements of the following satellites: Columba I, Eridanus III, Grus II, Phoenix II, Pictor I, Reticulum III, and Tucana IV. This is the first systemic proper motion measurement for several of these satellites, and the majority lack extensive spectroscopic follow-up studies. We compare these to the predictions of Large Magellanic Cloud satellites and the vast polar structure. With the high-precision DES photometry, we conclude that most of the newly identified member stars are very metal-poor ([Fe/H]&lt;=-2), similar to other ultra-faint dwarf galaxies, while Reticulum III is likely more metal-rich. We also find potential members in the following satellites that might indicate their overall proper motion: Cetus II, Kim 2, and Horologium II. However, due to the small number of members in each satellite, spectroscopic follow-up observations are necessary to determine the systemic proper motion in these satellites.</description><source format="bibcode">2019ApJ...875...77P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/875/77</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/II/357">II/357 : The Dark Energy Survey (DES): Data Release 1 (Abbott+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 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2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/838/11">J/ApJ/838/11 : Member stars in the MW satellite Tucana III (Simon+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/857/74">J/ApJ/857/74 : Abundances of 7 new member stars in Tucana II (Chiti+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/616/A12">J/A+A/616/A12 : Gaia DR2 sources in GC and dSph (Gaia Collaboration+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/866/22">J/ApJ/866/22 : Spectroscopic analysis of Tuc III stream (Li+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/857/145">J/ApJ/857/145 : MagLiteS Carina II and Carina III spectroscopy (Li+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/620/A155">J/A+A/620/A155 : Gaia proper motions of 7 UFD galaxies (Massari+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/863/25">J/ApJ/863/25 : Deep Magellan obs. of 4 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