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<ri:Resource created="2020-10-07T08:34:57Z" 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>PKS 1510-089 spectroscopic light curves</title><shortName>J/A+A/642/A59</shortName><identifier>ivo://CDS.VizieR/J/A+A/642/A59</identifier><altIdentifier>doi:10.26093/cds/vizier.36420059</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rakshit S.</name></creator><date role="Updated">2021-04-27T11:40:55Z</date><date role="Created">2020-10-07T08:34:57Z</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>spectroscopy</subject><subject>visible-astronomy</subject><description>Reverberation results of the flat spectrum radio quasar PKS 1510-089 from 8.5 years of spectroscopic monitoring carried out at Steward Observatory over nine observing seasons between December 2008 and June 2017 are presented. Optical spectra show strong H{beta}, H{gamma}, and FeII emission lines overlying on a blue continuum. All the continuum and emission line light curves show significant variability with fractional root-mean-square variations of 37.30+/-0.06% (f_5100_), 11.88+/-0.29% (H{beta}), and 9.61+/-0.71% (H{gamma}); however, along with thermal radiation from the accretion disk, non-thermal emission from the jet also contributes to f5100. Several methods of time series analysis (ICCF, DCF, von Neumann, Bartels, javelin, 2) are used to measure the lag between the continuum and line light curves. The observed frame broad line region size is found to be 61.1^+4.0^_3.2_ (64.7^+27.1^_10.6_) light-days for H{beta} (H{gamma}). Using the line of 1262+/-247km/s measured from the root-mean-square spectrum, the black hole mass of PKS 1510-089 is estimated to be 5.71^+0.62^_0.58_x1^0^7M_{sun}_.</description><source format="bibcode">2020A&amp;A...642A..59R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/642/A59</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/A+A/642/A59</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/642/A59</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/642/A59</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/642/A59</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/642/A59</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/642/A59</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><spectral>3.8949892233750168e-19 3.8949892233750168e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/642/A59/table1</name><description>Spectrosocpic data</description><column><name>MJD</name><description>Modified Julian date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>F5100</name><description>Monochromatic continuum flux at 5100{AA}</description><unit>1e-17W.m**-2.nm**-1</unit><ucd>phot.flux.density;spect.continuum</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F5100</name><description>rms uncertainty on F5100</description><unit>1e-17W.m**-2.nm**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FHb</name><description>H{beta} line flux</description><unit>1e-18W.m**-2</unit><ucd>phot.flux;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_FHb</name><description>rms uncertainty on FHb</description><unit>1e-18W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FHg</name><description>H{gamma} line flux</description><unit>1e-18W.m**-2</unit><ucd>phot.flux;spect.line</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_FHg</name><description>rms uncertainty on FHg</description><unit>1e-18W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F5100D</name><description>Detrended monochromatic continuum flux at 5100{AA}</description><unit>1e-17W.m**-2.nm**-1</unit><ucd>phot.flux.density;spect.continuum</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F5100D</name><description>rms uncertainty on F51005D</description><unit>1e-17W.m**-2.nm**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FHbD</name><description>Detrended H{beta} line flux</description><unit>1e-18W.m**-2</unit><ucd>phot.flux;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_FHbD</name><description>rms uncertainty on FHbD</description><unit>1e-18W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FHgD</name><description>Detrended H{gamma} line flux</description><unit>1e-18W.m**-2</unit><ucd>phot.flux;spect.line</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_FHgD</name><description>rms uncertainty on FHgD</description><unit>1e-18W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>