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<ri:Resource created="2021-11-05T06:29:54Z" 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>632 Gaia Ultracompact Dwarf galaxy candidates</title><shortName>J/ApJ/899/140</shortName><identifier>ivo://CDS.VizieR/J/ApJ/899/140</identifier><altIdentifier>doi:10.26093/cds/vizier.18990140</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Voggel K.T.</name></creator><creator><name>Seth A.C.</name></creator><creator><name>Sand D.J.</name></creator><creator><name>Hughes A.</name></creator><creator><name>Strader J.</name></creator><creator><name>Crnojevic D.,Caldwell N.</name></creator><date role="Updated">2023-06-14T12:45:19Z</date><date role="Created">2021-11-05T06:29:54Z</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>globular-star-clusters</subject><subject>galaxies</subject><subject>visible-astronomy</subject><subject>photometry</subject><subject>two-color-diagrams</subject><description>Tidally stripped galaxy nuclei and luminous globular clusters (GCs) are important tracers of the halos and assembly histories of nearby galaxies, but are difficult to reliably identify with typical ground-based imaging data. In this paper we present a new method to find these massive star clusters using Gaia DR2, focusing on the massive elliptical galaxy Centaurus A (Cen A). We show that stripped nuclei and GCs are partially resolved by Gaia at the distance of Cen A, showing characteristic astrometric and photometric signatures. We use this selection method to produce a list of 632 new candidate luminous clusters in the halo of Cen A out to a projected radius of 150kpc. Adding in broadband photometry and visual examination improves the accuracy of our classification. In a spectroscopic pilot program we have confirmed five new luminous clusters, which includes the 7th and 10th most luminous GC in Cen A. Three of the newly discovered GCs are further away from Cen A than all previously known GCs. Several of these are compelling candidates for stripped nuclei. We show that our novel Gaia selection method retains at least partial utility out to distances of ~25Mpc and hence is a powerful tool for finding and studying star clusters in the sparse outskirts of galaxies in the local universe.</description><source format="bibcode">2020ApJ...899..140V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/899/140</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/150/367">J/ApJS/150/367 : Globular clusters in NGC 5128 (Peng+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/2187">J/AJ/132/2187 : MCT1 photometry of NGC 5128 globular clusters (Harris+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/494">J/AJ/134/494 : NGC5128 globular clusters UBVRICMT1 phot. &amp; RV (Woodley+,2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/386/1443">J/MNRAS/386/1443 : 2dF study of globular clusters in NGC 5128 (Beasley+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/523/A48">J/A+A/523/A48 : Gaia photometry (Jordi+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/139/1871">J/AJ/139/1871 : Kinematics of globulars in NGC 5128 (Woodley+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/708/1335">J/ApJ/708/1335 : Spectroscopy of globulars in NGC 5128 (Woodley+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/199">J/AJ/142/199 : Sizes and luminosities of stellar systems (Brodie+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/84">J/AJ/143/84 : New candidate globular clusters in NGC 5128 (Harris+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/760/87">J/ApJ/760/87 : Globular clusters of M60 with HST (Strader+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/145/101">J/AJ/145/101 : Updated nearby galaxy catalog (Karachentsev+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/445/2385">J/MNRAS/445/2385 : HST/ACS Coma Cluster Survey. 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