J/ApJ/806/248ivo://CDS.VizieR/J/ApJ/806/248doi:10.26093/cds/vizier.18060248CDSWang J.Fischer D.A.Horch E.P.Xie J.-W.2017-11-03T13:02:34Z2017-09-27T09:49:14ZCDS support team

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

cds-question@unistra.frmultiple-starssolar-system-planetseffective-temperaturestellar-distanceinfrared-photometryvisible-astronomybroad-band-photometryAs hundreds of gas giant planets have been discovered, we study how these planets form and evolve in different stellar environments, specifically in multiple stellar systems. In such systems, stellar companions may have a profound influence on gas giant planet formation and evolution via several dynamical effects such as truncation and perturbation. We select 84 Kepler Objects of Interest (KOIs) with gas giant planet candidates. We obtain high-angular resolution images using telescopes with adaptive optics (AO) systems. Together with the AO data, we use archival radial velocity data and dynamical analysis to constrain the presence of stellar companions. We detect 59 stellar companions around 40 KOIs for which we develop methods of testing their physical association. These methods are based on color information and galactic stellar population statistics. We find evidence of suppressive planet formation within 20 AU by comparing stellar multiplicity. The stellar multiplicity rate (MR) for planet host stars is 0_-0_^+5^% within 20 AU. In comparison, the stellar MR is 18%+/-2% for the control sample, i.e., field stars in the solar neighborhood. The stellar MR for planet host stars is 34%+/-8% for separations between 20 and 200 AU, which is higher than the control sample at 12%+/-2%. Beyond 200 AU, stellar MRs are comparable between planet host stars and the control sample. We discuss the implications of the results on gas giant planet formation and evolution.2015ApJ...806..248Whttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/806/248CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toV/133 : Kepler Input Catalog (Kepler Mission Team, 2009)J/AJ/144/42 : Infrared photometry of 90 KOIs (Adams+, 2012)J/A+A/566/A103 : Kepler planet host candidates imaging (Lillo-Box+, 2014)J/ApJ/783/4 : Properties of Kepler multi-planet candidate systemsJ/ApJ/791/35 : Detection of 715 Kepler planet candidates host starshttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/806/248https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/806/248http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/806/248https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/806/248https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/806/248http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/806/248GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/806/248/table1 (RV and AO Data for 97 KOIs)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/806/248/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/806/248/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/806/248/table1?GETtext/xml+votable180.050000true286.8084719449.316398890.0055555555555555565/3778 6/14583 14585 14587 14589 14734 14746 14750 14751 14753 14755 14757 14759 14760 14765 14768 14769 14770 14774 14779 14781 14818 14824 14825 14826 14920 14924 14926 14928 14930 14934 14935 14936 14939 14941 14942 14943 14945 14970 14971 14973 14975 15040 15105 15107 15110 15118 15124 15131 15140 15141 15143 15145 15146 15150 15153 15155 15156 15158 15160 15169 15174 15178 15200https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/806/248?format=asciiOpticalInfrareddefaultJ/ApJ/806/248/table1RV and AO Data for 97 KOIsPerOrbital perioddtime.perioddoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintKOIKepler Object of Interest identifier (K0NNNN.NN)meta.id;meta.maincharKIC[3323887/12735740] Kepler Input Catalog numbermeta.idintRAJ2000Right Ascension in decimal degrees (J2000)degpos.eq.ra;meta.mainDEJ2000Declination in decimal degrees (J2000)degpos.eq.dec;meta.mainKpmagKepler magnitudemagphot.mag;em.optfloatTeffStellar effective temperatureKphys.temperature.effectivefloatloggStellar surface gravitylog(cm.s**-2)phys.gravityfloatDistDistancepcpos.distance;pos.heliocentricfloatNpl[1/6] Number of planetmeta.idintRplPlanet radius(6.3781x10+6m)phys.size.radiusfloate_RplUncertainty in Rpl(6.3781x10+6m)stat.errorfloatTstart? Start time in MJDdtime.startdoublenullableTend? End time in MJDdtime.enddoublenullableNrv[5/104]? Number of radial velocity measurementsmeta.numberintnullableTelTelescope namemeta.id;instr.telcharBandBand(s) used in the observation (J,K,JK,JHK,rz)instr.setup;obscharWork[check-] KOI with AO image taken through this workmeta.codecharSimbadSimbad column added by the CDSmeta.ref.urlcharJ/ApJ/806/248/table2Visual Companion Detections with AO DataDistP? Distance of primarypcpos.distance;pos.heliocentricfloatnullableE_DistP? Upper limit uncertainty in DistPpcstat.error;stat.maxfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintKOIKepler Object of Interest identifier (K0NNNN)meta.id;meta.maincharn_KOI[*] Note on KOI (1)meta.notecharDmagDifferential magnitude in Bandmagphot.mag;arith.difffloatBand[rizJHK] Band of the magnitudeinstr.bandpasscharSepCompanion separationarcsecpos.angDistancefloatSepa? Companion separation in AUAUpos.distance;src.orbitalfloatnullablee_DistP? Lower limit uncertainty in DistPpcstat.errorfloatnullableDistS? Distance of secondarypcpos.distance;pos.heliocentricfloatnullableE_DistS? Upper limit uncertainty in DistSpcstat.error;stat.maxfloatnullablee_DistS? Lower limit uncertainty in DistSpcstat.errorfloatnullableSigni? Detection significance in {sigma} unitinstr.saturationfloatnullablePA? Position angledegpos.posAngfloatnullableProb? Probability of associationmeta.id.assoc;stat.probabilityfloatnullableRefReference code (2)meta.notechar