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<ri:Resource created="2021-10-04T08:18:12Z" 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>Milky Way satellite census. I. DES &amp; PS1</title><shortName>J/ApJ/893/47</shortName><identifier>ivo://CDS.VizieR/J/ApJ/893/47</identifier><altIdentifier>doi:10.26093/cds/vizier.18930047</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Drlica-Wagner A.</name></creator><creator><name>Bechtol K.</name></creator><creator><name>Mau S.</name></creator><creator><name>McNanna M.</name></creator><creator><name>Nadler E.O.</name></creator><creator><name>Pace A.B.,Li T.S.</name></creator><creator><name>Pieres A.</name></creator><creator><name>Rozo E.</name></creator><creator><name>Simon J.D.</name></creator><creator><name>Walker A.R.</name></creator><creator><name>Wechsler R.H.,Abbott T.M.C.</name></creator><creator><name>Allam S.</name></creator><creator><name>Annis J.</name></creator><creator><name>Bertin E.</name></creator><creator><name>Brooks D.</name></creator><creator><name>Burke D.L.,Carnero Rosell A.</name></creator><creator><name>Carrasco Kind M.</name></creator><creator><name>Carretero J.</name></creator><creator><name>Costanzi M.,Da Costa L.N.</name></creator><creator><name>De Vicente J.</name></creator><creator><name>Desai S.</name></creator><creator><name>Diehl H.T.</name></creator><creator><name>Doel P.</name></creator><creator><name>Eifler T.F.,Everett S.</name></creator><creator><name>Flaugher B.</name></creator><creator><name>Frieman J.</name></creator><creator><name>Garcia-Bellido J.</name></creator><creator><name>Gaztanaga E.,Gruen D.</name></creator><creator><name>Gruendl R.A.</name></creator><creator><name>Gschwend J.</name></creator><creator><name>Gutierrez G.</name></creator><creator><name>Honscheid K.,James D.J.</name></creator><creator><name>Krause E.</name></creator><creator><name>Kuehn K.</name></creator><creator><name>Kuropatkin N.</name></creator><creator><name>Lahav O.</name></creator><creator><name>Maia M.A.G.,Marshall J.L.</name></creator><creator><name>Melchior P.</name></creator><creator><name>Menanteau F.</name></creator><creator><name>Miquel R.</name></creator><creator><name>Palmese A.,Plazas A.A.</name></creator><creator><name>Sanchez E.</name></creator><creator><name>Scarpine V.</name></creator><creator><name>Schubnell M.</name></creator><creator><name>Serrano S.,Sevilla-Noarbe I.</name></creator><creator><name>Smith M.</name></creator><creator><name>Suchyta E.</name></creator><creator><name>Tarle G.</name></creator><creator><name>(the DES Collaboration)</name></creator><date role="Updated">2023-08-16T13:36:49Z</date><date role="Created">2021-10-04T08:18:12Z</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>milky-way-galaxy</subject><subject>galaxies</subject><subject>photometry</subject><subject>surveys</subject><subject>absolute-magnitude</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>We report the results of a systematic search for ultra-faint Milky Way satellite galaxies using data from the Dark Energy Survey (DES) and Pan-STARRS1 (PS1). Together, DES and PS1 provide multi-band photometry in optical/near-infrared wavelengths over ~80% of the sky. Our search for satellite galaxies targets ~25000deg^2^ of the high-Galactic-latitude sky reaching a 10{sigma} point-source depth of &gt;~22.5mag in the g and r bands. While satellite galaxy searches have been performed independently on DES and PS1 before, this is the first time that a self-consistent search is performed across both data sets. We do not detect any new high-significance satellite galaxy candidates, recovering the majority of satellites previously detected in surveys of comparable depth. We characterize the sensitivity of our search using a large set of simulated satellites injected into the survey data. We use these simulations to derive both analytic and machine-learning models that accurately predict the detectability of Milky Way satellites as a function of their distance, size, luminosity, and location on the sky. To demonstrate the utility of this observational selection function, we calculate the luminosity function of Milky Way satellite galaxies, assuming that the known population of satellite galaxies is representative of the underlying distribution. We provide access to our observational selection function to facilitate comparisons with cosmological models of galaxy formation and evolution.</description><source format="bibcode">2020ApJ...893...47D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/893/47</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/4">VII/4 : Abell and Zwicky Clusters of Galaxies (Abell+ 1974)</relatedResource><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/VII/202">VII/202 : Globular Clusters in the Milky Way (Harris, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/239">VII/239 : History and Accurate Positions for the NGC/IC Objects (Corwin, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/349">II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)</relatedResource><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/J/MNRAS/389/678">J/MNRAS/389/678 : Extended objects in Magellanic Clouds (Bica+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/397/1748">J/MNRAS/397/1748 : Spectroscopic study of Segue 2 (Belokurov+, 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/ApJ/746/178">J/ApJ/746/178 : The augmented maxBCG cluster catalog (Rykoff+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/750/99">J/ApJ/750/99 : The Pan-STARRS1 photometric system (Tonry+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/558/A53">J/A+A/558/A53 : MW global survey of star clusters. 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