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<ri:Resource created="2022-06-13T13:17:46Z" 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>g- and r- band LCs of Q0957+561 &amp; SBS0909+532</title><shortName>J/ApJ/905/7</shortName><identifier>ivo://CDS.VizieR/J/ApJ/905/7</identifier><altIdentifier>doi:10.26093/cds/vizier.19050007</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cornachione M.A.</name></creator><creator><name>Morgan C.W.</name></creator><creator><name>Burger H.R.</name></creator><creator><name>Shalyapin V.N.,Goicoechea L.J.</name></creator><creator><name>Vrba F.J.</name></creator><creator><name>Dahm S.E.</name></creator><creator><name>Tilleman T.M.</name></creator><date role="Updated">2022-09-05T14:19:14Z</date><date role="Created">2022-06-13T13:17:46Z</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>gravitational-lensing</subject><subject>photometry</subject><subject>visible-astronomy</subject><description>We present a microlensing analysis of updated light curves in three filters, the g-band, r-band, and H-band, for the gravitationally lensed quasars Q0957+561 and SBS0909+532. Both systems display prominent microlensing features which we analyze using our Bayesian Monte Carlo technique to constrain the quasar continuum emission region sizes in each band. We report sizes as half-light radii scaled to a 60{deg} inclination angle. For Q0957+561 we measure log(r_1/2_/cm)=16.54_-0.33_^+0.33^, 16.66_-0.62_^+0.37^, and 17.37_-0.40_^+0.49^ in g-, r-, and H-band, respectively. For SBS0909+532 we measure log(r_1/2_/cm)=15.83_-0.33_^+0.33^, 16.21_-0.62_^+0.37^, and 17.90_-0.63_^+0.61^ in the g-, r-, and H-band respectively. With size measurements in three bands spanning the quasar rest frame ultraviolet to optical, we can place constraints on the scaling of accretion disk size with wavelength, r{propto}{lambda}^1/{beta}^. In a joint analysis of both systems we find a slope shallower than that predicted by thin disk theory, {beta}=0.35_-0.08_^+0.16^, consistent with other constraints from multi-epoch microlensing studies.</description><source format="bibcode">2020ApJ...905....7C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/905/7</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/640/579">J/ApJ/640/579 : Near-infrared spectra of 27 SDSS quasars (Glikman+, 2006)</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/A+A/540/A132">J/A+A/540/A132 : Optical follow-up of Q0957+561 in 2005-2010 (Shalyapin+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/806/129">J/ApJ/806/129 : Space telescope RM project. II. 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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>HJD</name><description>[117/8900] Heliocentric Julian Date, HJD-2450000</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Amag</name><description>[2.19/3.2] Apparent image A magnitude in Filt</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Amag</name><description>[0.001/0.04] Uncertainty in Amag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Bmag</name><description>[2.26/3.8] Apparent image B magnitude in Filt</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Bmag</name><description>[0.001/0.04] Uncertainty in Bmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Obs</name><description>Observatory (not for Tables 2 and 4) (1)</description><ucd>meta.id;instr.obsty</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Filt</name><description>r-band (from Teide Observatory, LRT, and USNO) or g-band from LRT (Table 2)</description><ucd>meta.code;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table><table><name>J/ApJ/905/7/sbs0909</name><description>Combined table from original tables</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>[117/8900] Heliocentric Julian Date, HJD-2450000</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Amag</name><description>[2.19/3.2] Apparent image A magnitude in Filt</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Amag</name><description>[0.001/0.04] Uncertainty in Amag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Bmag</name><description>[2.26/3.8] Apparent image B magnitude in Filt</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Bmag</name><description>[0.001/0.04] Uncertainty in Bmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Obs</name><description>Observatory (not for Tables 2 and 4) (1)</description><ucd>meta.id;instr.obsty</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Filt</name><description>r-band (from MDM, WIYN, LRT, and USNO) or g-band from LRT (Table 4)</description><ucd>meta.code;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table></schema></tableset></ri:Resource>