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<ri:Resource created="2018-03-15T12:10:59Z" 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>gi photometry of Bootes I</title><shortName>J/MNRAS/461/3702</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/461/3702</identifier><altIdentifier>doi:10.26093/cds/vizier.74613702</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Roderick T.A.</name></creator><creator><name>Mackey A.D.</name></creator><creator><name>Jerjen H.</name></creator><creator><name>Da Costa G.S.</name></creator><date role="Updated">2024-08-16T20:17:57Z</date><date role="Created">2018-03-15T12:10:59Z</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>visible-astronomy</subject><subject>sloan-photometry</subject><description>We present deep stellar photometry of the Bootes I dwarf spheroidal galaxy in g- and i-band filters, taken with the Dark Energy Camera at Cerro Tololo in Chile. Our analysis reveals a large, extended region of stellar substructure surrounding the dwarf, as well as a distinct overdensity encroaching on its tidal radius. A radial profile of the Bootes I stellar distribution shows a break radius indicating the presence of extra-tidal stars. These observations strongly suggest that Bootes I is experiencing tidal disruption, although not as extreme as that exhibited by the Hercules dwarf spheroidal. Combined with revised velocity dispersion measurements from the literature, we see evidence suggesting the need to review previous theoretical models of the Bootes I dwarf spheroidal galaxy.</description><source format="bibcode">2016MNRAS.461.3702R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/461/3702</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/136/2321">J/AJ/136/2321 : Washington photometry of Bootes I stars (Hughes+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/736/146">J/ApJ/736/146 : Radial velocities of stars in Bootes I (Koposov+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/61">J/ApJ/763/61 : Abundances of 7 red giant members of BootesI (Gilmore+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/439/788">J/MNRAS/439/788 : Stromgren and Washington photometry in Boo I (Hughes+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/450/1477">J/MNRAS/450/1477 : VLA 352MHz image of the Bootes field. 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