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<ri:Resource created="2021-04-30T11:53:21Z" 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>Reverberation mapping &amp; opt. spectra data of AGNs</title><shortName>J/ApJ/886/42</shortName><identifier>ivo://CDS.VizieR/J/ApJ/886/42</identifier><altIdentifier>doi:10.26093/cds/vizier.18860042</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Du P.</name></creator><creator><name>Wang J.-M.</name></creator><date role="Updated">2021-09-17T07:16:32Z</date><date role="Created">2021-04-30T11:53:21Z</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>line-intensities</subject><subject>black-holes</subject><subject>spectroscopy</subject><subject>visible-astronomy</subject><description>The radius-luminosity (R_H{beta}_-L_5100_) relationship of active galactic nuclei (AGNs) established by the reverberation mapping (RM) observations has been widely used as a single-epoch black hole mass estimator in the research of large AGN samples. However, the recent RM campaigns discovered that the AGNs with high-accretion rates show shorter time lags by factors of a few comparing with the predictions from the R_H{beta}_-L_5100_ relationship. The explanation of the shortened time lags has not been finalized yet. We collect eight different single-epoch spectral properties to investigate how the shortening of the time lags correlates with those properties and to determine the origin of the shortened lags. We find that the flux ratio between FeII and H{beta} emission lines shows the most prominent correlation, thus confirming that accretion rate is the main driver for the shortened lags. In addition, we establish a new scaling relation including the relative strength of FeII emission. This new scaling relation can provide less biased estimates of the black hole mass and accretion rate from the single-epoch spectra of AGNs.</description><source format="bibcode">2019ApJ...886...42D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/886/42</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/259">VII/259 : 6dF galaxy survey final redshift release (Jones+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/98/477">J/ApJS/98/477 : Optical spectral atlas of Seyfert nuclei (Ho+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/115/185">J/ApJS/115/185 : 3C 390.3 BVRI and H photometry (Dietrich+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/369/57">J/A+A/369/57 : Monitoring Mkn 279 in BVRI &amp; H{beta} (Santos-Lleo+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/613/682">J/ApJ/613/682 : AGN masses &amp; broad-line region sizes (Peterson+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/164/81">J/ApJS/164/81 : Spectrophotometry of nearby galaxies (Moustakas+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/667/131">J/ApJ/667/131 : Mass function of active black holes (Greene+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/683/L115">J/ApJ/683/L115 : Intermediate-line region in quasars (Hu+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/687/78">J/ApJ/687/78 : FeII emission in quasars (Hu+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/45">J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/755/60">J/ApJ/755/60 : Reverberation mapping for 5 Seyfert 1 galaxies (Grier+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/431/836">J/MNRAS/431/836 : Type 1 AGN at low z. 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