J/ApJ/809/77ivo://CDS.VizieR/J/ApJ/809/77doi:10.26093/cds/vizier.18090077CDSSullivan P.W.Winn J.N.Berta-Thompson Z.K.Charbonneau D.Deming D.,Dressing C.D.Latham D.W.Levine A.M.Mccullough P.R.Morton T.,Ricker G.R.Vanderspek R.Woods D.2017-01-23T22:00:00Z2016-01-13T08:25:28ZCDS support team

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

cds-question@unistra.frastronomical-modelssolar-system-planetssurveysinfrared-photometrystellar-radiiThe Transiting Exoplanet Survey Satellite (TESS) is a NASA-sponsored Explorer mission that will perform a wide-field survey for planets that transit bright host stars. Here, we predict the properties of the transiting planets that TESS will detect along with the EB stars that produce false-positive photometric signals. The predictions are based on Monte Carlo simulations of the nearby population of stars, occurrence rates of planets derived from Kepler, and models for the photometric performance and sky coverage of the TESS cameras. We expect that TESS will find approximately 1700 transiting planets from 2x10^5^ pre-selected target stars. This includes 556 planets smaller than twice the size of Earth, of which 419 are hosted by M dwarf stars and 137 are hosted by FGK dwarfs. Approximately 130 of the R<2R_{Earth}_ planets will have host stars brighter than Ks=9. Approximately 48 of the planets with R<2R_{Earth}_ lie within or near the habitable zone (0.2<S/S_{Earth}_<2); between 2 and 7 such planets have host stars brighter than Ks=9. We also expect approximately 1100 detections of planets with radii 2-4R_{Earth}_, and 67 planets larger than 4R_{Earth}_. Additional planets larger than 2R_{Earth}_ can be detected around stars that are not among the pre-selected target stars, because TESS will also deliver full-frame images at a 30-minute cadence. The planet detections are accompanied by over 1000 astrophysical false positives. We discuss how TESS data and ground-based observations can be used to distinguish the false positives from genuine planets. We also discuss the prospects for follow-up observations to measure the masses and atmospheres of the TESS planets.2015ApJ...809...77Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/809/77CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toI/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)J/ApJ/807/45 : Habitable zones around M dwarfs (Dressing+, 2015)J/ApJS/210/20 : Small Kepler planets radial velocities (Marcy+, 2014)J/ApJS/208/9 : Intrinsic colors and temperatures of PMS stars (Pecaut+, 2013)J/ApJ/772/L2 : Keck/HIRES radial velocities for HD 97658 (Dragomir+, 2013)J/ApJ/767/95 : Improved parameters of smallest KIC stars (Dressing+, 2013)J/A+A/552/A16 : Limb-darkening for CoRoT, Kepler, Spitzer. II. (Claret+, 2013)J/ApJ/757/112 : Stellar diameters. II. K and M-stars (Boyajian+, 2012)J/A+A/546/A14 : Limb-darkening for CoRoT, Kepler, Spitzer (Claret+, 2012)J/AJ/142/160 : Kepler Mission. II. eclipsing binaries (Slawson+, 2011)J/AJ/141/83 : Eclipsing binaries in Kepler first data release (Prsa+, 2011)J/ApJS/190/1 : A survey of stellar families (Raghavan+, 2010)J/MNRAS/389/869 : Multiplicity among bright stellar systems (Eggleton+, 2008)J/AJ/133/439 : Luminosity function of M7-L8 ultracool dwarfs (Cruz+, 2007)J/A+A/392/741 : Stellar Catalogue in the Chandra DFS (Groenewegen+ 2002)J/A+AS/141/371 : Low-mass stars evolutionary tracks+isochrones (Girardi+, 2000)J/PASP/110/863 : A Stellar Spectral Flux Library: 1150 - 25000 A (Pickles 1998)http://stev.oapd.inaf.it/cgi-bin/trilegal : TRILEGAL 1.6 input formhttp://www.astro.keele.ac.uk/jkt/debcat : Catalog of Eclipsing Binarieshttp://keplerebs.villanova.edu/v2 : Kepler EB cataloghttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/809/77https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/809/77http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/809/77https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/809/77https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/809/77http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/809/77GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/809/77/table6 (Catalog of simulated TESS detections)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/809/77/table6?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/809/77/table6?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/809/77/table6?GETtext/xml+votable180.050000true0.43945.220.0055555555555555565/2526 2545 2897 8265 9354 9362 9731 9738 9739 6/31 90 92 107 114 136 703 737 821 824 839 885 912 931 1134 1203 1204 1209 1400 1441 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46399 46408 46488 46609 46674 46688 46798 46865 46927 47087 47244 47255 47269 47286 47326 47344 47345 47347 47350 47359 47430 47462 47468 47470 47508 47589 47628 47652 47670 47727 47732 47799 47821 47823 47963 48011 48225 48230 48242 48296 48307 48312 48317 48465 48466 48486 49075 49120 49123 49132 49150https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/809/77?format=asciiInfrareddefaultJ/ApJ/809/77/table6Catalog of simulated TESS detectionsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right Ascension in decimal degrees (J2000)degpos.eq.ra;meta.mainDEJ2000Declination in decimal degrees (J2000)degpos.eq.dec;meta.mainRp[0.6/22] Planetary radius in Earth units(6.3781x10+6m)phys.size.radiusfloatPer[0.5/225] Perioddtime.perioddoubleS[0.07/55380] Planetary insolation in Earth unitsphys.size.radiusdoubleK[0.3/28.1] Radial-velocity semiamplitudem/sphys.veloc;src.orbitalfloatR*[0.1/4.1] Stellar radiussolRadphys.size.radiusfloatTeff[2529/11910] Stellar effective temperatureKphys.temperature.effectivedoubleVmag[4.2/19.2] Apparent V band magnitudemagphot.mag;em.opt.VfloatImag[3.7/16.7] Apparent I_C_ band magnitudemagphot.mag;em.opt.IfloatJmag[3.3/15.3] Apparent J band magnitudemagphot.mag;em.IR.JfloatKsmag[3/14.5] Apparent K_s_ band magnitudemagphot.mag;em.IR.KfloatDM[-2.1/8.4] Distance Modulusmagphot.mag.distModfloatDil[1/40.7] Dilution parameter for all detected eclipsesstat.fit.paramfloatlogsigV[-5.1/-2.4] Log standard deviation in relative flux (1)stat.stdevfloatSNR[7.3/1188] Signal-to-Noise Ratiostat.snrdoubleMult[0/4] Number of other planets orbiting the starmeta.numberint