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<ri:Resource created="2004-11-14T22:13:55Z" 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>Satellites orbiting isolated galaxies</title><shortName>J/ApJ/598/260</shortName><identifier>ivo://CDS.VizieR/J/ApJ/598/260</identifier><altIdentifier>doi:10.26093/cds/vizier.15980260</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Prada F.</name></creator><creator><name>Vitvitska M.</name></creator><creator><name>Klypin A.</name></creator><creator><name>Holtzman J.A.</name></creator><creator><name>Schlegel D.J.,Grebel E.K.</name></creator><creator><name>Rix H.-W.</name></creator><creator><name>Brinkmann J.</name></creator><creator><name>Mckay T.A.</name></creator><creator><name>Csabai I.</name></creator><date role="Updated">2004-11-14T21:17:02Z</date><date role="Created">2004-11-14T22:13:55Z</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>radial-velocity</subject><description>Using the Sloan Digital Sky Survey (SDSS), we probe the halo mass distribution by studying the velocities of satellites orbiting isolated galaxies. In a subsample that covers 2500{deg}^2^ on the sky, we detect about 3000 satellites with absolute blue magnitudes going down to M_B_=-14; most of the satellites have M_B_=-16 to -18, comparable to the magnitudes of M32 and the Magellanic Clouds.</description><source format="bibcode">2003ApJ...598..260P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/598/260</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/J/AJ/123/567">J/AJ/123/567 : SDSS quasar catalog, I: Early Data Release (Schneider+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/125/1817">J/AJ/125/1817 : SDSS Early-Type Galaxies Catalog (Bernardi+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/2579">J/AJ/126/2579 : SDSS quasar catalog. 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