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<ri:Resource created="2014-05-05T11:48:00Z" 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>Optical photometry in 3 Local Group dwarf galaxies</title><shortName>J/ApJ/756/79</shortName><identifier>ivo://CDS.VizieR/J/ApJ/756/79</identifier><altIdentifier>doi:10.26093/cds/vizier.17560079</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sand D.J.</name></creator><creator><name>Strader J.</name></creator><creator><name>Willman B.</name></creator><creator><name>Zaritsky D.</name></creator><creator><name>McLeod B.</name></creator><creator><name>Caldwell N.,Seth A.</name></creator><creator><name>Olszewski E.</name></creator><date role="Updated">2014-05-26T21:16:03Z</date><date role="Created">2014-05-05T11:48:00Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><description>We present deep wide-field photometry of three recently discovered faint Milky Way (MW) satellites: Leo V, Pisces II, and Canes Venatici II. Our main goals are to study the structure and star formation history of these dwarfs; we also search for signs of tidal disturbance. The three satellites have similar half-light radii (~60-90pc) but a wide range of ellipticities. Both Leo V and CVn II show hints of stream-like overdensities at large radii. An analysis of the satellite color-magnitude diagrams shows that all three objects are old (&gt;10Gyr) and metal-poor ([Fe/H]~-2), though neither the models nor the data have sufficient precision to assess when the satellites formed with respect to cosmic reionization. The lack of an observed younger stellar population (&lt;~10Gyr) possibly sets them apart from the other satellites at Galactocentric distances &gt;~150kpc. We present a new compilation of structural data for all MW satellite galaxies and use it to compare the properties of classical dwarfs to the ultra-faints. The ellipticity distribution of the two groups is consistent at the ~2{sigma} level. However, the faintest satellites tend to be more aligned toward the Galactic Center, and those satellites with the highest ellipticity (&gt;~0.4) have orientations ({Delta}{theta}_GC_) in the range 20{deg}&lt;~{Delta}{theta}_GC_&lt;~40{deg}. This latter observation is in rough agreement with predictions from simulations of dwarf galaxies that have lost a significant fraction of their dark matter halos and are being tidally stripped.</description><source format="bibcode">2012ApJ...756...79S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/756/79</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/144/4">J/AJ/144/4 : Dwarf galaxies in the Local Group (McConnachie+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/88">J/AJ/142/88 : Segue 3 photometric and kinematic data (Fadely+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/718/530">J/ApJ/718/530 : Leo IV g- and r-band photometry (Sand+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/710/1664">J/ApJ/710/1664 : BV photometry in Leo IV and Leo V dSphs (de Jong+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/694/L144">J/ApJ/694/L144 : Spectroscopic study of Leo V dSph (Walker+, 2009)</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/MNRAS/354/708">J/MNRAS/354/708 : Leo I VI photometry (Bellazzini+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/2840">J/AJ/126/2840 : BVI CCD photometry of Sextans dSph galaxy (Lee+, 2003)</relatedResource><relatedResource>http://www.sdss.org/ : SDSS home 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