J/ApJ/775/92ivo://CDS.VizieR/J/ApJ/775/92doi:10.26093/cds/vizier.17750092CDSKozlowski S.Onken C.A.Kochanek C.S.Udalski A.Szymanski M.K.,Kubiak M.Pietrzynski G.Soszynski I.Wyrzykowski L.Ulaczyk K.,Poleski R.Pietrukowicz P.Skowron J.(the OGLE Collaboration),Meixner M.Bonanos A.Z.2017-06-22T14:29:25Z2014-11-13T09:15:32ZCDS support team

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

cds-question@unistra.frsurveysmagellanic-cloudsquasarsactive-galactic-nucleiinfrared-photometryvisible-astronomyphotometryredshiftedThe Magellanic Quasars Survey (MQS) has now increased the number of quasars known behind the Magellanic Clouds by almost an order of magnitude. All survey fields in the Large Magellanic Cloud (LMC) and 70% of those in the Small Magellanic Cloud (SMC) have been observed. The targets were selected from the third phase of the Optical Gravitational Lensing Experiment (OGLE-III) based on their optical variability, mid-IR, and/or X-ray properties. We spectroscopically confirmed 758 quasars (565 in the LMC and 193 in the SMC) behind the clouds, of which 94% (527 in the LMC and 186 in the SMC) are newly identified. The MQS quasars have long-term (12yr and growing for OGLE), high-cadence light curves, enabling unprecedented variability studies of quasars. The MQS quasars also provide a dense reference grid for measuring both the internal and bulk proper motions of the clouds, and 50 quasars are bright enough (I<~18mag) for absorption studies of the interstellar/intergalactic medium of the clouds.2013ApJ...775...92Khttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/775/92CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJ/701/508 : 5000 AGNs behind the Magellanic clouds (Kozlowski+, 2009)J/ApJS/194/22 : MQS. I. QSOs behind SMC (Kozlowski+, 2011)J/ApJ/746/27 : MQS. II. AGNs behind LMC (Kozlowski+, 2012)http://ogle.astrouw.edu.pl : OGLE homepagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/775/92https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/775/92http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/775/92https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/775/92https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/775/92http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/775/92GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/775/92/agn_mc (Parameters of AGN behind the LMC or the SMC)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/775/92/agn_mc?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/775/92/agn_mc?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/775/92/agn_mc?GETtext/xml+votable180.050000true67.792-69.878193890.0055555555555555564/2068 5/8263 8269 8280 8323 8324 8326 6/33045 33046 33047 33049 33051 33073 33074 33075 33080 33081 33084 33085 33086 33104 33105 33106 33112 33124 33125 33126 33128 33129 33287 33316 33317 33328 33329 37536 375382.367228618189496e-19 3.852589004194616e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/775/92?format=asciiInfraredOpticaldefaultJ/ApJ/775/92/agn_mcParameters of AGN behind the LMC or the SMCrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMCSimbad column added by the CDSobs.fieldcharn_MQSNew or known AGN (4)meta.notecharMQSSource name (JHHMMSS.ss+DDMMSS.s)meta.id;meta.maincharm_MQS[(ab) ] Multiplicity index on MQSmeta.code.multipcharRAJ2000Right Ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainz[0.05/3.8] Spectroscopic redshiftsrc.redshiftfloatDM[37/48] Distance modulus {mu} (1)magphot.mag.distModfloatVmag? The OGLE V-band magnitude (2)magphot.mag;em.opt.VfloatnullableImagThe OGLE I-band magnitudemagphot.mag;em.opt.IfloatAVExtinction in V-band A_V_magphys.absorptionfloatAIExtinction in I-band A_I_magphys.absorptionfloatKVK-correction in V-band K_V_magarith.factor;phot.magfloatKIK-correction in I-band K_I_magarith.factor;phot.magfloatVMAG? Absolute magnitude in V-band (2)magphot.mag;em.opt.VfloatnullableIMAGAbsolute magnitude in I-bandmagphot.mag;em.opt.IfloatOGLEOGLE-III identification ([ls]mcFFF.F.NNNNNN) (<OGLE [LS]MCFFF.F NNNNNNN> in Simbad)meta.idcharClassClass code (as in KK09, Cat. J/ApJ/701/508) (3)meta.code.classcharMIR[0/1] Existence of mid-IR emission: 1=yes;0=nometa.codeintX[0/1] Existence of X-ray emission: 1=yes;0=nometa.codeintVar[0/1] Variable source: 1=yes, 0=nometa.noteintQs[Q123 ] Spectrum Quality Flag: Q1=excellent, Q2=good, Q3=low quality.meta.code.qualcharEmLinesList of emission lines; absorption lines are written "abs()", e.g. "abs(CIV)"meta.noteSimbadSimbad column added by the CDSmeta.ref.urlchar