<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2026-08-07T09:02:58Z" status="active" updated="2026-08-07T08:05:43Z" 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>Swift and LCO LCs of PG 1302-102</title><shortName>J/ApJ/964/167</shortName><identifier>ivo://CDS.VizieR/J/ApJ/964/167</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Liu T.</name></creator><creator><name>Edelson R.</name></creator><creator><name>Hernandez Santisteban J.V.</name></creator><creator><name>Kara E.</name></creator><creator><name>Montano J.,Gelbord J.</name></creator><creator><name>Horne K.</name></creator><creator><name>Barth A.J.</name></creator><creator><name>Cackett E.M.</name></creator><creator><name>Kaplan D.L.</name></creator><date role="Updated">2026-08-07T08:05:43Z</date><date role="Created">2026-08-07T09:02:58Z</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>quasars</subject><subject>ultraviolet-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>infrared-photometry</subject><description>We present an intensive multiwavelength monitoring campaign of the quasar PG 1302-102 with Swift and the Las Cumbres Observatory network telescopes. At z~0.3, it tests the limits of the reverberation mapping (RM) technique in probing the accretion disk around a supermassive black hole (SMBH) and extends the parameter space to high masses and high accretion rates. This is also the first time the RM technique has been applied to test disk structures predicted in the SMBH binary model that has been suggested for this source. PG 1302-102 was observed at a ~daily cadence for ~9 months in 14 bands spanning from X-ray to UV and optical wavelengths, and it shows moderate to significant levels of variability correlated between wavelengths. We measure the interband time lags, which are consistent with a {tau}{propto}{lambda}^4/3^ relation as expected from standard disk reprocessing, albeit with large uncertainties. The disk size implied by the lag spectrum is consistent with the expected disk size for its black hole mass within uncertainties. While the source resembles other reverberation-mapped active galactic nuclei in many respects, and we do not find evidence supporting the prevalent hypothesis that it hosts an SMBH binary, we demonstrate the feasibility of studying SMBH binaries from this novel angle and suggest possibilities for the LSST Deep Drilling Fields.</description><source format="bibcode">2024ApJ...964..167L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/964/167</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/II/207">II/207 : Palomar-Green catalog UV-excess stellar objects (Green+ 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/157">III/157 : An Ultraviolet Atlas of Quasar and Blazar Spectra (Kinney+, 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/85">VIII/85 : SPECFIND V2.0 Catalog of radio continuum spectra (Vollmer+ 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/104">VIII/104 : SPECFIND V3.0 Catalog of radio continuum spectra (Stein+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/358">I/358 : Gaia DR3 Part 4. Variability (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/361">I/361 : Gaia Focused Product Release (Gaia FPR) (Gaia Collaboration, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/676/262">J/ApJ/676/262 : PKS1302-102 intergalactic absorption system (Cooksey+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/397/1177">J/MNRAS/397/1177 : Swift-XRT observations of GRBs (Evans+, 2009)</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/MNRAS/438/3058">J/MNRAS/438/3058 : 15GHz variability of {gamma}-ray blazars (Richards+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/453/1562">J/MNRAS/453/1562 : CRTS close supermassive black hole binaries (Graham+, 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/AJ/152/25">J/AJ/152/25 : The UV-bright Quasar Survey (UVQS) DR1 (Monroe+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/821/56">J/ApJ/821/56 : Space telescope RM project. III. LCs (Fausnaugh+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/840/41">J/ApJ/840/41 : X-ray/UV Swift monitoring of NGC 4151 (Edelson+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/233/17">J/ApJS/233/17 : Swift/BAT AGN sp. survey. V. X-ray data (Ricci+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/870/123">J/ApJ/870/123 : Swift optical &amp; UV flux of four AGNs (Edelson+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/896/1">J/ApJ/896/1 : SEAMBHs. XI. Mrk 142 X-ray to optical LCs (Cackett+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/261/2">J/ApJS/261/2 : BASS. XXII. Swift/BAT AGN Sp. Survey DR2 cat. (Koss+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/947/62">J/ApJ/947/62 : griz light curves of Mrk 335 (Kara+, 2023)</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/964/167</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/964/167</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/964/167</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/964/167</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/964/167</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/964/167</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><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>UV</waveband><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/964/167/table2</name><description>Swift UV and optical light curves</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>Band</name><description>Swift/UVOT filter identifier</description><ucd>meta.code;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>MJD</name><description>[59551/59816.1] Modified Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>[3.16/21.02] Observed flux in Band; 10^-15^erg/s/cm^2^/{AA}</description><unit>1e-17W.m**-2.nm**-1</unit><ucd>phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Flux</name><description>[0.08/0.8] Uncertainty in Flux</description><unit>1e-17W.m**-2.nm**-1</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJ/964/167/table3</name><description>Inter-calibrated LCO light curves</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>Band</name><description>[BVugriz] LCO filter identifier</description><ucd>meta.code;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>MJD</name><description>[59256.3/60172.5] Modified Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>[2.53/5.34] Observed flux in Band</description><unit>mJy</unit><ucd>phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Flux</name><description>[0.009/0.2] Uncertainty in Flux</description><unit>mJy</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>