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<ri:Resource created="2017-11-27T14:27:44Z" 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>Space telescope RM project. V. NGC5548 sp. monitoring</title><shortName>J/ApJ/837/131</shortName><identifier>ivo://CDS.VizieR/J/ApJ/837/131</identifier><altIdentifier>doi:10.26093/cds/vizier.18370131</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pei L.</name></creator><creator><name>Fausnaugh M.M.</name></creator><creator><name>Barth A.J.</name></creator><creator><name>Peterson B.M.</name></creator><creator><name>Bentz M.C.</name></creator><creator><name>De Rosa G.,Denney K.D.</name></creator><creator><name>Goad M.R.</name></creator><creator><name>Kochanek C.S.</name></creator><creator><name>Korista K.T.</name></creator><creator><name>Kriss G.A.,Pogge R.W.</name></creator><creator><name>Bennert V.N.</name></creator><creator><name>Brotherton M.</name></creator><creator><name>Clubb K.I.</name></creator><creator><name>Dalla Bonta E.,Filippenko A.V.</name></creator><creator><name>Greene J.E.</name></creator><creator><name>Grier C.J.</name></creator><creator><name>Vestergaard M.</name></creator><creator><name>Zheng W.,Adams S.M.</name></creator><creator><name>Beatty T.G.</name></creator><creator><name>Bigley A.</name></creator><creator><name>Brown J.E.</name></creator><creator><name>Brown J.S.</name></creator><creator><name>Canalizo G.,Comerford J.M.</name></creator><creator><name>Coker C.T.</name></creator><creator><name>Corsini E.M.</name></creator><creator><name>Croft S.</name></creator><creator><name>Croxall K.V.,Deason A.J.</name></creator><creator><name>Eracleous M.</name></creator><creator><name>Fox O.D.</name></creator><creator><name>Gates E.L.</name></creator><creator><name>Henderson C.B.,Holmbeck E.</name></creator><creator><name>Holoien T.W.-S.</name></creator><creator><name>Jensen J.J.</name></creator><creator><name>Johnson C.A.</name></creator><creator><name>Kelly P.L.,Kim S.</name></creator><creator><name>King A.</name></creator><creator><name>Lau M.W.</name></creator><creator><name>Li M.</name></creator><creator><name>Lochhaas C.</name></creator><creator><name>Ma Z.</name></creator><creator><name>Manne-Nicholas E.R.,Mauerhan J.C.</name></creator><creator><name>Malkan M.A.</name></creator><creator><name>McGurk R.</name></creator><creator><name>Morelli L.</name></creator><creator><name>Mosquera A.</name></creator><creator><name>Mudd D.,Sanchez F.M.</name></creator><creator><name>Nguyen M.L.</name></creator><creator><name>Ochner P.</name></creator><creator><name>Ou-Yang B.</name></creator><creator><name>Pancoast A.</name></creator><creator><name>Penny M.T.,Pizzella A.</name></creator><creator><name>Poleski R.</name></creator><creator><name>Runnoe J.</name></creator><creator><name>Scott B.</name></creator><creator><name>Schimoia J.S.</name></creator><creator><name>Shappee B.J.,Shivvers I.</name></creator><creator><name>Simonian G.V.</name></creator><creator><name>Siviero A.</name></creator><creator><name>Somers G.</name></creator><creator><name>Stevens D.J.,Strauss M.A.</name></creator><creator><name>Tayar J.</name></creator><creator><name>Tejos N.</name></creator><creator><name>Treu T.</name></creator><creator><name>Van Saders J.</name></creator><creator><name>Vican L.,Villanueva S.</name></creator><creator><name>Yuk H.</name></creator><creator><name>Zakamska N.L.</name></creator><creator><name>Zhu W.</name></creator><creator><name>Anderson M.D.</name></creator><creator><name>Arevalo P.,Bazhaw C.</name></creator><creator><name>Bisogni S.</name></creator><creator><name>Borman G.A.</name></creator><creator><name>Bottorff M.C.</name></creator><creator><name>Brandt W.N.,Breeveld A.A.</name></creator><creator><name>Cackett E.M.</name></creator><creator><name>Carini M.T.</name></creator><creator><name>Crenshaw D.M.,De Lorenzo-caceres A.</name></creator><creator><name>Dietrich M.</name></creator><creator><name>Edelson R.</name></creator><creator><name>Efimova N.V.</name></creator><creator><name>Ely J.,Evans P.A.</name></creator><creator><name>Ferland G.J.</name></creator><creator><name>Flatland K.</name></creator><creator><name>Gehrels N.</name></creator><creator><name>Geier S.</name></creator><creator><name>Gelbord J.M.,Grupe D.</name></creator><creator><name>Gupta A.</name></creator><creator><name>Hall P.B.</name></creator><creator><name>Hicks S.</name></creator><creator><name>Horenstein D.</name></creator><creator><name>Horne K.,Hutchison T.</name></creator><creator><name>Im M.</name></creator><creator><name>Joner M.D.</name></creator><creator><name>Jones J.</name></creator><creator><name>Kaastra J.</name></creator><creator><name>Kaspi S.,Kelly B.C.</name></creator><creator><name>Kennea J.A.</name></creator><creator><name>Kim M.</name></creator><creator><name>Kim S.C.</name></creator><creator><name>Klimanov S.A.</name></creator><creator><name>Lee J.C.,Leonard D.C.</name></creator><creator><name>Lira P.</name></creator><creator><name>Macinnis F.</name></creator><creator><name>Mathur S.</name></creator><creator><name>Mchardy I.M.</name></creator><creator><name>Montouri C.,Musso R.</name></creator><creator><name>Nazarov S.V.</name></creator><creator><name>Netzer H.</name></creator><creator><name>Norris R.P.</name></creator><creator><name>Nousek J.A.</name></creator><creator><name>Okhmat D.N.,Papadakis I.</name></creator><creator><name>Parks J.R.</name></creator><creator><name>Pott J.-U.</name></creator><creator><name>Rafter S.E.</name></creator><creator><name>Rix H.-W.</name></creator><creator><name>Saylor D.A.,Schnulle K.</name></creator><creator><name>Sergeev S.G.</name></creator><creator><name>Siegel M.</name></creator><creator><name>Skielboe A.</name></creator><creator><name>Spencer M.</name></creator><creator><name>Starkey D.,Sung H.-I.</name></creator><creator><name>Teems K.G.</name></creator><creator><name>Turner C.S.</name></creator><creator><name>Uttley P.</name></creator><creator><name>Villforth C.</name></creator><creator><name>Weiss Y.,Woo J.-H.</name></creator><creator><name>Yan H.</name></creator><creator><name>Young S.</name></creator><creator><name>Zu Y.</name></creator><date role="Updated">2018-03-12T08:28:39Z</date><date role="Created">2017-11-27T14:27:44Z</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><description>We present the results of an optical spectroscopic monitoring program targeting NGC 5548 as part of a larger multiwavelength reverberation mapping campaign. The campaign spanned 6 months and achieved an almost daily cadence with observations from five ground-based telescopes. The H{beta} and HeII{lambda}4686 broad emission-line light curves lag that of the 5100{AA} optical continuum by 4.17_-0.36_^+0.36^days and 0.79_-0.34_^+0.35^days, respectively. The H{beta} lag relative to the 1158{AA} ultraviolet continuum light curve measured by the Hubble Space Telescope is ~50% longer than that measured against the optical continuum, and the lag difference is consistent with the observed lag between the optical and ultraviolet continua. This suggests that the characteristic radius of the broad-line region is ~50% larger than the value inferred from optical data alone. We also measured velocity-resolved emission-line lags for H{beta} and found a complex velocity-lag structure with shorter lags in the line wings, indicative of a broad-line region dominated by Keplerian motion. The responses of both the H{beta} and He II emission lines to the driving continuum changed significantly halfway through the campaign, a phenomenon also observed for CIV, Ly{alpha}, HeII(+OIII]), and SiIV(+OIV]) during the same monitoring period. Finally, given the optical luminosity of NGC5548 during our campaign, the measured H{beta} lag is a factor of five shorter than the expected value implied by the R_BLR_-L_AGN_ relation based on the past behavior of NGC 5548.</description><source format="bibcode">2017ApJ...837..131P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/837/131</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/ApJS/115/185">J/ApJS/115/185 : 3C 390.3 BVRI and H photometry (Dietrich+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/510/659">J/ApJ/510/659 : Size and Structure of AGN in NGC 5548 (Peterson+, 1999)</relatedResource><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/A+A/417/515">J/A+A/417/515 : I Zw 1 unusual emission line spectrum (Veron-Cetty+, 2004)</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/ApJ/698/895">J/ApJ/698/895 : Variations in QSOs optical flux (Kelly+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/716/993">J/ApJ/716/993 : LAMP: reverberation mapping of H and He lines (Bentz+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/189/15">J/ApJS/189/15 : FeII emission in a sample of AGN spectra (Kovacevic+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/732/121">J/ApJ/732/121 : V-band and H{beta} monitoring of Z299-15 (Barth+, 2011)</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/788/48">J/ApJ/788/48 : X-ray through NIR photometry of NGC 2617 (Shappee+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/217/26">J/ApJS/217/26 : Lick AGN monitoring 2011: light curves (Barth+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/806/128">J/ApJ/806/128 : Space telescope RM project. I. NGC5548 (De Rosa+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/806/22">J/ApJ/806/22 : SEAMBHs IV. H{beta} time lags (Du+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/806/129">J/ApJ/806/129 : Space telescope RM project. II. Swift data (Edelson+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/821/56">J/ApJ/821/56 : Space tel. RM project. III. NGC 5548 LCs (Fausnaugh+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/827/118">J/ApJ/827/118 : A new reverberation mapping campain on NGC 5548 (Lu+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/818/30">J/ApJ/818/30 : Lag measurements for z&lt;0.8 QSOs from the SDSS-RM (Shen+, 2016)</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/ApJ/837/131</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/837/131</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/837/131</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/837/131</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/837/131</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/837/131</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/ApJ/837/131/table2</name><description>Flux measurements for continuum and emission lines</description><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>HJD</name><description>Heliocentric Julian Date; JD-2450000</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tel</name><description>Telescope code (1)</description><ucd>meta.code;instr.tel</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>F5100</name><description>[10/13.5] Flux density at 5100{AA} (2)</description><unit>1e-15cW.m**-2.nm**-1</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F5100</name><description>[0.03/0.1] Uncertainty in F5100 (2)</description><unit>1e-15cW.m**-2.nm**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FHb</name><description>[661/822] Linear continuum model H{beta} emission-line flux density (3)</description><unit>1e-15mW.m**-2</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_FHb</name><description>[2/8] Uncertainty in FHb (3)</description><unit>1e-15mW.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FHbSD</name><description>[656/803]? Spectral decomposition method H{beta} emission-line flux density (3)</description><unit>1e-15mW.m**-2</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_FHbSD</name><description>[4/8]? Uncertainty in FHbSD (3)</description><unit>1e-15mW.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FHeIISD</name><description>[21/163]? Spectral decomposition method HeII emission-line flux density (3)</description><unit>1e-15mW.m**-2</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_FHeIISD</name><description>[2/10]? Uncertainty in FHeIISD (3)</description><unit>1e-15mW.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>