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<ri:Resource created="2004-11-23T21:58:13Z" 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>Nuclear star clusters in late-type spiral galaxies</title><shortName>J/AJ/127/105</shortName><identifier>ivo://CDS.VizieR/J/AJ/127/105</identifier><altIdentifier>doi:10.26093/cds/vizier.51270105</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Boker T.</name></creator><creator><name>Sarzi M.</name></creator><creator><name>Mclaughlin D.E.</name></creator><creator><name>Van Der Marel R.P.</name></creator><creator><name>Rix H.-W.,Ho L.C.</name></creator><creator><name>Shields J.C.</name></creator><date role="Updated">2023-04-06T16:51:00Z</date><date role="Created">2004-11-23T21:58:13Z</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>stellar-associations</subject><subject>apparent-magnitude</subject><description>We investigate the structural properties of nuclear star clusters in late-type spiral galaxies. More specifically, we fit analytical models to Hubble Space Telescope images of 39 nuclear clusters in order to determine their effective radii after correction for the instrumental point-spread function. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Galaxy name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Dist</name><description>Distance from Paper I (2002AJ....123.1389B), assuming Ho=70km/s/Mpc</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SB</name><description>Observed peak disk surface brightness (1)</description><unit>mag.arcsec**-2</unit><ucd>phot.mag.sb</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Imag</name><description>Nuclear cluster apparent I-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>IMAG</name><description>Nuclear cluster absolute I-band magnitude (2)</description><unit>mag</unit><ucd>phys.magAbs;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMod</name><description>Name of best-fitting ISHAPE model (3)</description><ucd>meta.id;stat.fit</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>f_BMod</name><description>Flag on BMod (4)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>ARad</name><description>? 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