J/A+A/553/A53ivo://CDS.VizieR/J/A+A/553/A53doi:10.26093/cds/vizier.35530053CDSSluse D.Kishimoto M.Anguita T.Wucknitz O.Wambsganss J.2013-10-06T22:39:05Z2013-05-02T08:52:04ZCDS support team

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

cds-question@unistra.frgravitational-lensingactive-galactic-nucleiquasarsWe provide the microlensing maps generated to study microlensing in the mid-infrared range for a cusp-configuration lensed AGN. The maps provided correspond to images which are respectively saddle-point and minimum of the arrival time surface. We also provide simulated images of sources with a disc-like brightness profile or a ring-like brightness profile corresponding to an accretion disc or a torus brightness distribution. These source profiles should be convolved with microlensing maps of the same spatial resolution to simulate microlensing of the corresponding source and generate probability density function (PDF) of microlensing similar to those shown in Figures 3,4,5,8. These maps can also be used to generate synthetic microlensing lightcurves (Figure 9) or derive PDF for the Rcusp relation (Figure 10).2013A&A...553A..53Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/553/A53CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/553/A53https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/553/A53http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/553/A53https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/553/A53https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/553/A53http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/553/A53GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/553/A53/nosourceList of source profiles unavailable (too large)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTypeSource profile typesrc.morph.typecharlambdaWavelength (see paper for assumptions)umem.wlfloatlogLSource Luminosity (see paper for assumptions)log(mW.m**-2)phys.luminosityfloatRes[low/high ] Spatial resolutionpos.angResolutioncharJ/A+A/553/A53/sourcesList of source profiles availablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTypeSource profile typesrc.morph.typecharlambdaWavelength (see paper for assumptions)umem.wlfloatlogLSource Luminosity (see paper for assumptions)log(mW.m**-2)phys.luminosityfloatRes[low/high ] Spatial resolutionpos.angResolutioncharFileNameFor sources.dat, name of the associated fits file in subdirectory fitsmeta.id;meta.fitscharFITSDownload the FITS imagemeta.ref.urlcharJ/A+A/553/A53/mapsList of microlensing maps availablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTypeLensed image typesrc.morph.typecharFcmFraction of compact matter (in %)%stat.fit.paramintRes[low/high ] Spatial resolutionpos.angResolutioncharFileNameName of the associated fits file in subdirectory fitsmeta.id;meta.fitscharFITSDownload the FITS imagemeta.ref.urlchar