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<ri:Resource created="2021-02-01T07:35:37Z" 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>SDSS RM project: continuum lags</title><shortName>J/ApJ/880/126</shortName><identifier>ivo://CDS.VizieR/J/ApJ/880/126</identifier><altIdentifier>doi:10.26093/cds/vizier.18800126</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Homayouni Y.</name></creator><creator><name>Trump J.R.</name></creator><creator><name>Grier C.J.</name></creator><creator><name>Shen Y.</name></creator><creator><name>Starkey D.A.</name></creator><creator><name>Brandt W.N.,Fonseca Alvarez G.</name></creator><creator><name>Hall P.B.</name></creator><creator><name>Horne K.</name></creator><creator><name>Kinemuchi K.</name></creator><creator><name>Li J.I.-H.,McGreer I.D.</name></creator><creator><name>Sun M.</name></creator><creator><name>Ho L.C.</name></creator><creator><name>Schneider D.P.</name></creator><date role="Updated">2021-04-28T12:24:48Z</date><date role="Created">2021-02-01T07:35:37Z</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>surveys</subject><subject>visible-astronomy</subject><description>We present accretion disk structure measurements from continuum lags in the Sloan Digital Sky Survey Reverberation Mapping (SDSS-RM) project. Lags are measured using the JAVELIN software from the first-year SDSS-RM g and i photometry, resulting in well-defined lags for 95 quasars, 33 of which have lag S/N&gt;2{sigma}. We also estimate lags using the ICCF software and find consistent results, though with larger uncertainties. Accretion disk structure is fit using a Markov chain Monte Carlo approach, parameterizing the measured continuum lags as a function of disk size normalization, wavelength, black hole mass, and luminosity. In contrast with previous observations, our best-fit disk sizes and color profiles are consistent (within 1.5{sigma}) with the Shakura &amp; Sunyaev (1973A&amp;A....24..337S) analytic solution. We also find that more massive quasars have larger accretion disks, similarly consistent with the analytic accretion disk model. The data are inconclusive on a correlation between disk size and continuum luminosity, with results that are consistent with both no correlation and the Shakura &amp; Sunyaev expectation. The continuum lag fits have a large excess dispersion, indicating that our measured lag errors are underestimated and/or our best-fit model may be missing the effects of orientation, spin, and/or radiative efficiency. We demonstrate that fitting disk parameters using only the highest-S/N lag measurements biases best-fit disk sizes to be larger than the disk sizes recovered using a Bayesian approach on the full sample of well-defined lags.</description><source format="bibcode">2019ApJ...880..126H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/880/126</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/286">VII/286 : SDSS quasar catalog, fourteenth data release (Paris+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/622/129">J/ApJ/622/129 : Lag-luminosity relationship in AGN (Sergeev+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/166/470">J/ApJS/166/470 : SDSS-Spitzer type I QSOs IR photometry (Richards+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/698/895">J/ApJ/698/895 : Variations in QSOs optical flux (Kelly+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/733/60">J/ApJ/733/60 : Accretion rate of AGNs from COSMOS surveys (Trump+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/788/48">J/ApJ/788/48 : X-ray through NIR photometry of NGC 2617 (Shappee+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/806/22">J/ApJ/806/22 : SEAMBHs IV. 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