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<ri:Resource created="2010-07-21T15:36:07Z" 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 black hole-bulge relationship</title><shortName>J/AJ/135/928</shortName><identifier>ivo://CDS.VizieR/J/AJ/135/928</identifier><altIdentifier>doi:10.26093/cds/vizier.51350928</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Shen J.</name></creator><creator><name>Vanden Berk D.E.</name></creator><creator><name>Schneider D.P.</name></creator><creator><name>Hall P.B.</name></creator><date role="Updated">2018-07-02T11:15:38Z</date><date role="Created">2010-07-21T15:36:07Z</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>active-galactic-nuclei</subject><subject>apparent-magnitude</subject><subject>redshifted</subject><subject>spectroscopy</subject><description>We have measured the stellar velocity dispersions ({sigma}_*_) and estimated the central black hole (BH) masses for over 900 broad-line active galactic nuclei (AGNs) observed with the Sloan Digital Sky Survey. The sample includes objects which have redshifts up to z=0.452, high-quality spectra, and host galaxy spectra dominated by an early-type (bulge) component. The AGN and host galaxy spectral components were decomposed using an eigenspectrum technique. The BH masses (M_BH_) were estimated from the AGN broad-line widths, and the velocity dispersions were measured from the stellar absorption spectra of the host galaxies. The range of black hole masses covered by the sample is approximately 10^6^&lt;M_BH_&lt;10^9^M_{sun}_. We find no significant evolution in the M_BH_-{sigma}_*_ relation with redshift, up to z~0.4, after controlling for possible dependences on other variables. Interested readers can contact the authors to obtain the eigenspectrum decomposition coefficients of our objects.</description><source format="bibcode">2008AJ....135..928S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/135/928</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/ApJ/614/91">J/ApJ/614/91 : Black hole mass and accretion rate of AGNs (Wu+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/613/682">J/ApJ/613/682 : AGN central masses and broad-line region sizes (Peterson+ 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/84">J/AJ/131/84 : AGNs and host galaxies information (Vanden Berk+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/294">II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)</relatedResource><relatedResource>http://www.sdss.org/ : SDSS Home Page</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/AJ/135/928</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/135/928</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/135/928</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL 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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>SDSS</name><description>Source identification (HHMMSS.ss+DDMMDD.s)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>imag</name><description>SDSS apparent i band magnitude</description><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Hfrac</name><description>[0/1] Host galaxy fractional flux contribution</description><ucd>phys.luminosity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>phi</name><description>Host galaxy classification angle (2)</description><unit>deg</unit><ucd>src.morph.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>S/N</name><description>The i band spectroscopic signal-to-noise</description><ucd>stat.snr;instr.bandpass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>S/N(H)</name><description>Host galaxy S/N</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>gMAG</name><description>Host galaxy absolute SDSS g band magnitude</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logL1</name><description>Host subtracted AGN monochromatic continuum luminosity at 5100 Angstroms (erg/s/{AA})</description><unit>log(uW.nm**-1)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logL2</name><description>Host not subtracted AGN monochromatic continuum luminosity at 5100 Angstroms</description><unit>log(uW.nm**-1)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>sigma</name><description>? 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