J/A+A/587/A64ivo://CDS.VizieR/J/A+A/587/A64doi:10.26093/cds/vizier.35870064CDSSanterne A.Moutou C.Tsantaki M.Bouchy F.Hebrard G.,Adibekyan V.Almenara J.-M.Amard L.Barros S.C.C.Boisse I.,Bonomo A.S.Bruno G.Courcol B.Deleuil M.Demangeon O.Diaz R.F.,Guillot T.Havel M.Montagnier G.Rajpurohit A.S.Rey J.Santos N.C.2018-10-05T14:44:46Z2016-02-17T08:53:08ZCDS support team

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

cds-question@unistra.frmultiple-starssolar-system-planetsradial-velocityWhile giant extrasolar planets have been studied for more than two decades now, there are still some open questions as to their dominant formation and migration processes, as well as to their atmospheric evolution in different stellar environments. In this paper, we study a sample of giant transiting exoplanets detected by the Kepler telescope with orbital periods up to 400 days. We first defined a sample of 129 giant-planet candidates that we followed up with the SOPHIE spectrograph (OHP, France) in a 6-year radial velocity campaign. This allowed us to unveil the nature of these candidates and to measure a false-positive rate of 54.6+/-6.5% for giant-planet candidates orbiting within 400 days of period. Based on a sample of confirmed or likely planets, we then derived the occurrence rates of giant planets in different ranges of orbital periods. The overall occurrence rate of giant planets within 400 days is 4.6+/-0.6%. We recovered, for the first time in the Kepler data, the different populations of giant planets reported by radial velocity surveys. Comparing these rates with other yields, we find that the occurrence rate of giant planets is lower only for hot Jupiters but not for the longer-period planets. We also derive a first measurement of the occurrence rate of brown dwarfs in the brown-dwarf desert with a value of 0.29+/-0.17%. Finally, we discuss the physical properties of the giant planets in our sample. We confirm that giant planets receiving moderate irradiation are not inflated, but we find that they are on average smaller than predicted by formation and evolution models. In this regime of low-irradiated giant planets, we find a possible correlation between their bulk density and the iron abundance of the host star, which needs more detections to be confirmed.2016A&A...587A..64Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/587/A64CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/528/A63 : Velocitometry transit of KOI-428b (Santerne+, 2011)J/A+A/544/L12 : Velocitometry transit of KOI-13 (Santerne+, 2012)J/A+A/571/A37 : KOI-1257 photometric and velocimetric data (Santerne+, 2014)J/A+A/573/A124 : Kepler-117 (KOI-209) transit-timing variations (Bruno+, 2015)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/587/A64https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/587/A64http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/587/A64https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/587/A64https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/587/A64http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/587/A64GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/587/A64/table1 (Kepler candidates from the Q1-Q17 dataset that respect all the criteria defined in Section 2)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/587/A64/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/587/A64/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/587/A64/table1?GETtext/xml+votable180.050000true286.808491449.31641420.0055555555555555566/14577 14579-14581 14583-14586 14591 14733-14735 14746 14749-14750 14753-14754 14757-14759 14762-14765 14767-14768 14770-14772 14776 14779-14781 14783 14794 14816 14818 14824-14826 14828 14918 14920-14921 14924 14926 14928-14929 14931 14933 14935-14936 14938-14939 14942 14947-14948 14954 14958 14960-14961 14963 14971 14973 15040 15105 15107 15109-15110 15112 15114 15118 15120 15122 15126 15129 15139-15141 15143 15146 15148-15150 15153 15156-15157 15160 15168-15169 15172 15174 15200https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/587/A64?format=asciidefaultJ/A+A/587/A64/table1Kepler candidates from the Q1-Q17 dataset that respect all the criteria defined in Section 2KOIKOI numbermeta.id;meta.mainfloatKeplerKepler namemeta.idcharPerPerioddtime.periodfloatDepthDepth%phys.absorption.opticalDepth;arith.ratiofloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintKICKIC numbermeta.idintaSemi-major axis, in R* unitphys.angSize;srcfloatE_aError on a (upper value)stat.error;stat.maxfloate_aError on a (lower value)stat.errorfloatkepmagKepler magnitudemagphot.mag;em.optfloatTeff? Effective temperatureKphys.temperature.effectiveintnullableE_Teff? Error on Teff (upper value)Kstat.error;stat.maxintnullablee_Teff? Error on Teff (lower value)Kstat.error;phys.temperature.effectiveintnullablelogg? Surface gravitylog(cm.s**-2)phys.gravityfloatnullableE_logg? Error on logg (upper value)log(cm.s**-2)stat.error;stat.maxfloatnullablee_logg? Error on logg (lower value)log(cm.s**-2)stat.errorfloatnullable[Fe/H]? Metallicityphys.abund.ZfloatnullableE_[Fe/H]? Error on [Fe/H] (upper value)stat.error;stat.maxfloatnullablee_[Fe/H]? Error on [Fe/H] (lower value)stat.error;phys.abund.FefloatnullableTypeNature of the objectmeta.code.classcharRefReference, in refs.dat filemeta.ref;pos.frame;meta.filecharRV[*] * indicates RV data in tables B1-B3meta.codecharSimbadSimbad column added by the CDSmeta.ref.urlchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainJ/A+A/587/A64/tableb2SOPHIE RV of SB2 starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintBJDBaricentric Julian datedtime.epochdoubleRVARadial velocity of first componentkm/sphys.veloc;pos.heliocentricfloate_RVArms uncertainty on RVAkm/sstat.errorfloatRVBRadial velocity of second componentkm/sphys.veloc;pos.heliocentricdoublee_RVBrms uncertainty on RVBkm/sstat.errorfloatTexpExposure timestime.duration;obs.exposureintS/NSignal-to-noise ratiostat.snrfloatKOITarget KOI numbermeta.id;meta.mainintJ/A+A/587/A64/tableb3SOPHIE RV of SB3 starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintBJDBaricentric Julian datedtime.epochdoubleRVARadial velocity of first componentkm/sphys.veloc;pos.heliocentricfloate_RVArms uncertainty on RVAkm/sstat.errorfloatRVBRadial velocity of second componentkm/sphys.veloc;pos.heliocentricfloate_RVBrms uncertainty on RVBkm/sstat.errorfloatRVCRadial velocity of third componentkm/sphys.veloc;pos.heliocentricfloate_RVCrms uncertainty on RVCkm/sstat.errorfloatTexpExposure timestime.duration;obs.exposureintS/NSignal-to-noise ratiostat.snrfloatKOITarget KOI numbermeta.id;meta.mainintJ/A+A/587/A64/tableb1SOPHIE RV of single starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintBJDBaricentric Julian datedtime.epochdoubleRVRadial velocitykm/sphys.veloc;pos.heliocentricdoublee_RVrms uncertainty on RVkm/sstat.errorfloatVspan? Bisector spankm/sphys.velocfloatnullablee_Vspan? rms uncertainty on Vspankm/sstat.errorfloatnullableFWHM? FWHMkm/sspect.line.widthfloatnullablee_FWHM? rms uncertainty on FWHMkm/sstat.error;phys.angSizefloatnullableTexpExposure timestime.duration;obs.exposureintS/NSignal-to-noise ratiostat.snrfloatKOITarget KOI numbermeta.id;meta.mainintJ/A+A/587/A64/refsReferencesComCommentsmeta.notecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRefReference codemeta.notecharBibCodeBibCodemeta.bib.bibcodecharAutAuthor's namemeta.bib.authorchar