J/ApJ/756/52ivo://CDS.VizieR/J/ApJ/756/52doi:10.26093/cds/vizier.17560052CDSMorgan C.W.Hainline L.J.Chen B.Tewes M.Kochanek C.S.Dai X.,Kozlowski S.Blackburne J.A.Mosquera A.M.Chartas G.Courbin F.,Meylan G.2017-06-19T07:57:55Z2014-04-29T08:10:55ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frquasarsgravitational-lensinginfrared-photometryvisible-astronomyphotometryx-ray-sourcesWe present four new seasons of optical monitoring data and six epochs of X-ray photometry for the doubly imaged lensed quasar Q J0158-4325. The high-amplitude, short-period microlensing variability for which this system is known has historically precluded a time delay measurement by conventional methods. We attempt to circumvent this limitation by the application of a Monte Carlo microlensing analysis technique, but we are only able to prove that the delay must have the expected sign (image A leads image B). Despite our failure to robustly measure the time delay, we successfully model the microlensing at optical and X-ray wavelengths to find a half-light radius for soft X-ray emission log (r_1/2,X,soft_/cm)=14.3^+0.4^_-0.5_, an upper limit on the half-light radius for hard X-ray emission log (r_1/2,X,hard_/cm)<=14.6, and a refined estimate of the inclination-corrected scale radius of the optical R-band (rest frame 3100{AA}) continuum emission region of log (r_s_/cm)=15.6+/-0.3.2012ApJ...756...52Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/756/52CatalogResearchIsServedByTAP VizieR generic servicerelated-toVII/258 : Quasars and Active Galactic Nuclei (13th Ed.) (Veron+ 2010)J/A+A/553/A121 : 2 lensed quasars light curves (Eulaers+, 2013)J/A+A/551/A104 : Lensed QSO UM673/Q0142-100 VRi light curves (Ricci+, 2013)J/A+A/536/A53 : R-band light curves of HE 0435-1223 (Courbin+, 2011)J/ApJ/679/1144 : Galaxy clusters in LOS to background QSOs. I. (Lopez+, 2008)J/ApJ/660/146 : HE 1104-1805 differential light curves (Poindexter+, 2007)http://www.cosmograil.org/ : COSMOSGRAIL project home pagehttp://www.cfa.harvard.edu/castles/ : CASTLES survey home pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/756/52https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/756/52http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/756/52https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/756/52https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/756/52http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/756/52GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tap2.762881831355591e-19 3.3785437584409506e-19X-rayOpticalInfrareddefaultJ/ApJ/756/52/table1Q J0158-4325 light curvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHJDHeliocentric Julian Date; HJD-2450000dtime.epochdoubleSeeing[0.9/2.1] Seeingarcsecinstr.obsty.seeingfloatmagA[1.6/1.9] R-band magnitude of QSO image A (1)magphot.mag;em.opt.Rfloate_magA[0.005/0.03] Uncertainty in magAmagstat.errorfloatu_magA[)] magA not used in the analysis (2)meta.code.errorcharmagB[2.4/3.0] R-band magnitude of QSO image B (1)magphot.mag;em.opt.Rfloate_magB[0.01/0.07] Uncertainty in magBmagstat.errorfloatu_magB[)] magB not used in the analysis (2)meta.code.errorcharTelSource of the observation (3)meta.id;instr.telchar