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<ri:Resource created="2022-12-19T09:12:48Z" 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>The CGS. X. Stellar mass parameters for bulges</title><shortName>J/ApJS/262/54</shortName><identifier>ivo://CDS.VizieR/J/ApJS/262/54</identifier><altIdentifier>doi:10.26093/cds/vizier.22620054</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gao H.</name></creator><creator><name>Ho L.C.</name></creator><creator><name>Li Z.-Y.</name></creator><date role="Updated">2023-09-27T10:27:14Z</date><date role="Created">2022-12-19T09:12:48Z</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>visible-astronomy</subject><subject>two-color-diagrams</subject><description>We measure optical colors for the bulges of 312 disk galaxies from the Carnegie-Irvine Galaxy Survey and convert their previously available R-band structural parameters to stellar-mass parameters. We also measure their average stellar-mass surface density in the central 1kpc ({Sigma}1). Comparing the mass-based Kormendy relation with the original one based on flux, we find that the majority of the classifications into classical and pseudo bulges, as well as their overall statistical properties, remain essentially unchanged. While the bulge-type classifications of the Kormendy relation are robust against stellar population effects, the mass-based classification criteria do produce better agreement between bulge structural properties and their stellar populations. Moreover, the mass-based Kormendy relation reveals a population of ultradense bulges akin to high-z compact early-type galaxies, which are otherwise hidden in the original Kormendy relation. These bulges are probably relics of spheroids assembled in the early universe, although for some we cannot rule out some contribution from secular growth. We confirm previous studies that {Sigma}1 correlates well with bulge surface densities.</description><source format="bibcode">2022ApJS..262...54G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/262/54</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/VII/237">VII/237 : HYPERLEDA. I. 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(Ho+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/197/22">J/ApJS/197/22 : The Carnegie-Irvine Galaxy Survey (GGS). II. (Li+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/750/93">J/ApJ/750/93 : NIR observations of XMM-LSS J02182-05102 (Papovich+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/749/121">J/ApJ/749/121 : Surface brightness profiles if z=2 galaxies (Szomoru+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/821/114">J/ApJ/821/114 : The CGS. IV. Elliptical galaxies colors (Huang+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/845/87">J/ApJ/845/87 : CGS. V. Statistical study of bars &amp; buckled bars (Li+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/862/100">J/ApJ/862/100 : Carnegie-Irvine Galaxy Survey VII. S0 galaxies (Gao+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/244/34">J/ApJS/244/34 : The CGS. VIII. R-band images of disk galaxies (Gao+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/247/20">J/ApJS/247/20 : CGS. IX. R single-Sersic fits to ellipticals (Gao+, 2020)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/262/54</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/262/54</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/262/54</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/262/54</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/262/54</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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