J/MNRAS/457/1320ivo://CDS.VizieR/J/MNRAS/457/1320doi:10.26093/cds/vizier.74571320CDSTsapras Y.Hundertmark M.Wyrzykowski L.Horne K.Udalski A.,Snodgrass C.Street R.Bramich D.M.Dominik M.Bozza V.,Figuera Jaimes R.Kains N.Skowron J.Szymanski M.K.Pietrzynski G.,Soszynski I.Ulaczyk K.Kozlowski P.Pietrukowicz S.Poleski R.2024-08-15T20:17:50Z2016-02-08T14:33:03ZCDS support team

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

cds-question@unistra.frmultiple-starssolar-system-planetsWe use six years (2003-2008) of Optical Gravitational Lensing Experiment-III microlensing observations to derive the survey detection efficiency for a range of planetary masses and projected distances from the host star. We perform an independent analysis of the microlensing light curves to extract the event parameters and compute the planet detection probability given the data. 2433 light curves satisfy our quality selection criteria and are retained for further processing. The aggregate of the detection probabilities over the range explored yields the expected number of microlensing planet detections. We employ a Galactic model to convert this distribution from dimensionless to physical units, {alpha}/au and M_{earth}_ The survey sensitivity to small planets is highest in the range 1-4au, shifting to slightly larger separations for more massive ones.2016MNRAS.457.1320Thttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/457/1320CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/457/1320https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/457/1320http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/457/1320https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/457/1320https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/457/1320http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/457/1320GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/MNRAS/457/1320/listInformations on fits filerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNxNumber of pixels along X-axismeta.numberintNyNumber of pixels along Y-axismeta.numberintblog10(a)Lower value of orbital radius intervallog(AU)phys.angSize;src.orbitalfloatBlog10(a)Upper value of orbital radius intervallog(AU)phys.angSize;src.orbitalfloatdlog10(a)Resolution in orbital radiuslog(AU)stat.fit.paramfloatblog10(M)Lower value of planetary mass interval in M_{Earth}_ unitphys.massfloatBlog10(M)Upper value of planetary mass interval in M_{Earth}_ unitphys.massfloatdlog10(M)Resolution in planetary massstat.fit.paramfloatsizeSize of FITS fileKibytephys.size;meta.fitsintFileNameName of FITS filemeta.id;meta.fitscharTextTitle of the FITS file (1)meta.title;meta.fitschar