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<ri:Resource created="2021-08-17T11:32:46Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>5100{AA} continuum &amp; emission lines LCs of PG2130+099</title><shortName>J/ApJ/890/71</shortName><identifier>ivo://CDS.VizieR/J/ApJ/890/71</identifier><altIdentifier>doi:10.26093/cds/vizier.18900071</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hu C.</name></creator><creator><name>Li Y.-R.</name></creator><creator><name>Du P.</name></creator><creator><name>Zhang Z.-X.</name></creator><creator><name>Li S.-S.</name></creator><creator><name>Huang Y.-K.</name></creator><creator><name>Lu K.-X.,Bai J.-M.</name></creator><creator><name>Ho L.C.</name></creator><creator><name>Bian W.-H.</name></creator><creator><name>Brotherton M.S.</name></creator><creator><name>Yuan Y.-F.</name></creator><creator><name>Aceituno J.,Winkler H.</name></creator><creator><name>Wang J.-M.</name></creator><creator><name>(the SEAMBH Collaboration)</name></creator><date role="Updated">2021-10-04T14:14:33Z</date><date role="Created">2021-08-17T11:32:46Z</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>visible-astronomy</subject><subject>spectroscopy</subject><description>As one of the most interesting Seyfert 1 galaxies, PG 2130+099 has been the target of several reverberation mapping (RM) campaigns over the years. However, its measured broad H{beta} line responses have been inconsistent, with time lags of ~200days, ~25days, and ~10days being reported for different epochs while its optical luminosity changed no more than 40%. To investigate this issue, we conducted a new RM-campaign with homogenous and high cadence (about ~3days) for two years during 2017-2019 to measure the kinematics and structure of the ionized gas. We successfully detected time lags of broad H{beta}, HeII, HeI, and FeII lines with respect to the varying 5100{AA} continuum, revealing a stratified structure that is likely virialized with Keplerian kinematics in the first year of observations, but an inflow kinematics of the broad-line region from the second year. With a central black hole mass of 0.97_-0.18_^+0.15^x10^7^M_{sun}_, PG2130+099 has an accretion rate of 10^2.1+/-0.5^L_Edd_c^-2^, where L_Edd_ is the Eddington luminosity and c is speed of light, implying that it is a super-Eddington accretor and likely possesses a slim, rather than thin, accretion disk. The fast changes of the ionization structures of the three broad lines remain puzzling.</description><source format="bibcode">2020ApJ...890...71H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/890/71</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/613/682">J/ApJ/613/682 : AGN central masses &amp; broad-line region sizes (Peterson+, 2004)</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/753/L2">J/ApJ/753/L2 : Reverberation mapping of AGNs (Assef+, 2012)</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/ApJ/779/109">J/ApJ/779/109 : Long-term monitoring of NGC 5548 (Peterson+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/782/45">J/ApJ/782/45 : SEAMBHs. 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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>JD</name><description>Julian Date of observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F5100</name><description>[4.6e-15/6e-15] 5100{AA} continuum flux, in erg/s/cm^2^/{AA} units</description><unit>cW.m**-2.nm**-1</unit><ucd>meta.unit;phot.flux.density;spect.continuum</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_F5100</name><description>Uncertainty in F5100</description><unit>cW.m**-2.nm**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>FHbeta</name><description>[4.8e-13/6.2e-13] H{beta} line flux, in erg/s/cm^2^ units</description><unit>mW.m**-2</unit><ucd>meta.unit;phot.flux;spect.line</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FHbeta</name><description>Uncertainty in FHbeta</description><unit>mW.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>FHeI</name><description>[4.7e-14/7.3e-14] He I line flux, in erg/s/cm^2^ units</description><unit>mW.m**-2</unit><ucd>meta.unit;phot.flux;spect.line</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FHeI</name><description>Uncertainty in FHeI</description><unit>mW.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>FHeII</name><description>[2.4e-14/1.1e-13] He II line flux, in erg/s/cm^2^ units</description><unit>mW.m**-2</unit><ucd>meta.unit;phot.flux;spect.line</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FHeII</name><description>Uncertainty in FHeII</description><unit>mW.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>FFe</name><description>[3.6e-13/5e-13] Fe II line flux, in erg/s/cm^2^ units</description><unit>mW.m**-2</unit><ucd>meta.unit;phot.flux;spect.line</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FFe</name><description>Uncertainty in FFe</description><unit>mW.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>