J/ApJ/790/146ivo://CDS.VizieR/J/ApJ/790/146doi:10.26093/cds/vizier.17900146CDSFabrycky D.C.Lissauer J.J.Ragozzine D.Rowe J.F.Steffen J.H.,Agol E.Barclay T.Batalha N.Borucki W.Ciardi D.R.Ford E.B.,Gautier T.N.Geary J.C.Holman M.J.Jenkins J.M.Li J.Morehead R.C.,Morris R.L.Shporer A.Smith J.C.Still M.Van Cleve J.2018-01-05T08:57:00Z2017-03-27T14:23:24ZCDS support team

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

cds-question@unistra.frmultiple-starssolar-system-planetsephemeridesstellar-massesstellar-radiiWe report on the orbital architectures of Kepler systems having multiple-planet candidates identified in the analysis of data from the first six quarters of Kepler data and reported by Batalha et al. (2013, J/ApJS/204/24). These data show 899 transiting planet candidates in 365 multiple-planet systems and provide a powerful means to study the statistical properties of planetary systems. Using a generic mass-radius relationship, we find that only two pairs of planets in these candidate systems (out of 761 pairs total) appear to be on Hill-unstable orbits, indicating ~96% of the candidate planetary systems are correctly interpreted as true systems. We find that planet pairs show little statistical preference to be near mean-motion resonances. We identify an asymmetry in the distribution of period ratios near first-order resonances (e.g., 2:1, 3:2), with an excess of planet pairs lying wide of resonance and relatively few lying narrow of resonance. Finally, based upon the transit duration ratios of adjacent planets in each system, we find that the interior planet tends to have a smaller transit impact parameter than the exterior planet does. This finding suggests that the mode of the mutual inclinations of planetary orbital planes is in the range 1.{deg}0-2.{deg}2, for the packed systems of small planets probed by these observations.2014ApJ...790..146Fhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/790/146CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toV/133 : Kepler Input Catalog (Kepler Mission Team, 2009)J/ApJS/197/2 : Transit timing observations from Kepler. I. (Ford+, 2011)J/ApJS/204/24 : Kepler planetary candidates. III. (Batalha+, 2013)J/ApJ/821/47 : KOI transit probabilities of multi-planet syst.https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/790/146https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/790/146http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/790/146https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/790/146https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/790/146http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/790/146GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/790/146/table1 (Characteristics of Planets in Systems with Multiple Transiting Planets)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/790/146/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/790/146/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/790/146/table1?GETtext/xml+votable180.050000true289.739744.64740.0055555555555555564/922 5/3646 3693 3706 3731 3733 3734 3735 3740 3743 3778 3780 3781 3782 3792 6/14573 14578 14579 14581 14582 14583 14588 14591 14730 14731 14733 14734 14735 14744 14750 14751 14768 14770 14771 14776 14778 14779 14780 14781 14782 14794 14816 14818 14819 14828 14830 14914 14918 14919 14920 14921 14923 14929 14930 14931 14944 14945 14946 14948 14949 14950 14952 14953 14955 14957 14958 14959 14964 14965 14966 14968 14969 14971 15044 15060 15061 15062 15104 15105 15107 15108 15109 15110 15116 15118 15119 15132 15136 15137 15139 15140 15141 15142 15145 15146 15147 15148 15149 15150 15153 15154 15155 15156 15158 15160 15172 15174 15232https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/790/146?format=asciidefaultJ/ApJ/790/146/table1Characteristics of Planets in Systems with Multiple Transiting PlanetsSimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintKOIKelper Object of Interest identifier (1)meta.id;meta.maindoublePeriodOrbital perioddtime.perioddoubleT0Barycentric Julian Date of minimum; BJD-2454900.0dtime.epochdoubleTdurEclipse durationhtime.durationfloatRpPlanetary radius; Earth radii(6.3781x10+6m)phys.size.radiusfloatS/NSignal-to-Noisestat.snrfloatM*Stellar masssolMassphys.massfloatR*Stellar radiussolRadphys.size.radiusfloatP/P-? Ratio of orbital periods (2)time.perioddoublenullableDelta-? Orbital separation (3)pos.angDistancefloatnullable_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.main