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<ri:Resource created="2016-06-22T15:40:40Z" 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>Stellar masses of optical &amp; IR QSO hosts</title><shortName>J/ApJ/819/L27</shortName><identifier>ivo://CDS.VizieR/J/ApJ/819/L27</identifier><altIdentifier>doi:10.26093/cds/vizier.18199027</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhang Z.</name></creator><creator><name>Shi Y.</name></creator><creator><name>Rieke G.H.</name></creator><creator><name>Xia X.</name></creator><creator><name>Wang Y.</name></creator><creator><name>Sun B.</name></creator><creator><name>Wan L.</name></creator><date role="Updated">2017-09-22T16:16:39Z</date><date role="Created">2016-06-22T15:40:40Z</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>quasars</subject><subject>redshifted</subject><subject>galaxies</subject><subject>infrared-sources</subject><subject>galaxy-classification-systems</subject><description>The relation between star formation rates (SFRs) and stellar masses, i.e., the galaxy main sequence, is a useful diagnostic of galaxy evolution. We present the distributions relative to the main sequence of 55 optically selected PG and 12 near-IR-selected Two Micron All Sky Survey (2MASS) quasars at z&lt;=0.5. We estimate the quasar host stellar masses from Hubble Space Telescope or ground-based AO photometry, and the SFRs through the mid-infrared aromatic features and far-IR photometry. We find that PG quasar hosts more or less follow the main sequence defined by normal star-forming galaxies while 2MASS quasar hosts lie systematically above the main sequence. PG and 2MASS quasars with higher nuclear luminosities seem to have higher specific SFRs (sSFRs), although there is a large scatter. No trends are seen between sSFRs and SMBH masses, Eddington ratios, or even morphology types (ellipticals, spirals, and mergers). Our results could be placed in an evolutionary scenario with quasars emerging during the transition from ULIRGs/mergers to ellipticals. However, combined with results at higher redshift, they suggest that quasars can be widely triggered in normal galaxies as long as they contain abundant gas and have ongoing star formation.</description><source format="bibcode">2016ApJ...819L..27Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/819/L27</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/II/294">II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/219/18">J/ApJS/219/18 : LIRAS: LoCuSS IR AGN survey (Xu+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/214/23">J/ApJS/214/23 : IR spectra and photometry of z&lt;0.5 quasars (Shi+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/720/368">J/ApJ/720/368 : Color-magnitude relations of galaxies in CDFs (Xue+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/701/587">J/ApJ/701/587 : A deep HST H-band imaging survey. II. QSOs (Veilleux+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/692/556">J/ApJ/692/556 : Star forming galaxy templates (Rieke+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/182/628">J/ApJS/182/628 : Spitzer quasar and ULIRG evolution study (Veilleux+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/383/1513">J/MNRAS/383/1513 : 2MASS, SDSS and FIRST fluxes of QSOs (Labita+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/667/673">J/ApJ/667/673 : FIRST-2MASS red quasar survey (Glikman+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/663/81">J/ApJ/663/81 : SED of hard X-ray selected AGN in XMDS (Polletta+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/625/78">J/ApJ/625/78 : QSOs properties (Hao+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/143/277">J/ApJS/143/277 : IRAS 1Jy sample of ultraluminous galaxies. I. 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