J/MNRAS/448/3608ivo://CDS.VizieR/J/MNRAS/448/3608doi:10.26093/cds/vizier.74483608CDSBovaird T.Lineweaver C.H.Jacobsen S.K.2024-08-14T20:20:31Z2015-12-18T15:50:43ZCDS support team

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

cds-question@unistra.frmultiple-starssolar-system-planetsWe analyse a sample of multiple-exoplanet systems which contain at least three transiting planets detected by the Kepler mission ('Kepler multiples'). We use a generalized Titius-Bode relation to predict the periods of 228 additional planets in 151 of these Kepler multiples. These Titius-Bode-based predictions suggest that there are, on average, 2+/-1 planets in the habitable zone of each star. We estimate the inclination of the invariable plane for each system and prioritize our planet predictions by their geometric probability to transit. We highlight a short list of 77 predicted planets in 40 systems with a high geometric probability to transit, resulting in an expected detection rate of ~15%, ~3 times higher than the detection rate of our previous Titius-Bode-based predictions.2015MNRAS.448.3608Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/448/3608CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toV/133 : Kepler Input Catalog (Kepler Mission Team, 2009)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/448/3608https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/448/3608http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/448/3608https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/448/3608https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/448/3608http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/448/3608GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/448/3608/tablec2 (All 228 planet predictions in 151 systems)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/448/3608/tablec2?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/448/3608/tablec2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/448/3608/tablec2?GETtext/xml+votable180.050000true292.479712538.51492220.0055555555555555565/3734 3742 3780 6/14579-14580 14582 14585-14587 14590-14591 14731 14733-14735 14744 14751 14753-14758 14760-14761 14763-14765 14767 14770 14772 14774-14775 14778-14779 14781 14794 14816 14819 14824 14826 14828 14921 14923 14925 14929-14934 14941-14943 14948 14950 14952-14953 14958-14960 14962-14964 14966 14973 14975 15041 15060 15105 15107-15108 15110 15115-15116 15119 15126-15128 15131 15137 15139-15142 15146-15150 15156-15157 15160 15168 15170-15172 15174 15232https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/448/3608?format=asciidefaultJ/MNRAS/448/3608/tablec177 planet predictions with a high geometric probability to transit (Ptrans>=0.55) in 40 Kepler systems (subset of table C2)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameSystem name, KOI-NNNNmeta.id;pos.framecharNins[0/6] Number of planet inserted in the systemmeta.numberintGamma? Measure of the fractional amount by which the chi^2^2/d.o.f. improves, divided by the number of planets inserted (1)stat.fit.paramfloatnullableDGamma? DGamma=(Gamma1-Gamma2)/Gamma2 (2)stat.fit.paramfloatnullablechi2/dofi? Chi^2^/d.o.f value before planets are insertedstat.fit.paramfloatnullablechi2/doff? Chi^2^/d.o.f value after planets are insertedstat.fit.paramfloatnullableNp[1/7] Inserted planet identification numbermeta.idintn_Np[E] E: planet is extrapolated (3)meta.notecharPerPerioddtime.periodfloate_Perrms uncertainty on Perdstat.errorfloataSemi-major axis of the planetAUphys.size.smajAxisfloatRmaxMaximum radius in Earth radius (4)phys.angSize;srcfloatTeffEffective temperatureKphys.temperature.effectiveintPtransprobability to transitstat.fit.goodnessfloatJ/MNRAS/448/3608/tablec2All 228 planet predictions in 151 systemsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameSystem name, KOI-NNNNmeta.id;pos.framecharNins[0/6] Number of planet inserted in the systemmeta.numberintGamma? Measure of the fractional amount by which the chi^2^2/d.o.f. improves, divided by the number of planets inserted (1)stat.fit.paramfloatnullableDGamma? DGamma=(Gamma1-Gamma2)/Gamma2 (2)stat.fit.paramfloatnullablechi2/dofi? Chi^2^/d.o.f value before planets are insertedstat.fit.paramfloatnullablechi2/doff? Chi^2^/d.o.f value after planets are insertedstat.fit.paramfloatnullableNp[1/7] Inserted planet identification numbermeta.idintn_Np[E] E: planet is extrapolated (3)meta.notecharPerPerioddtime.periodfloate_Perrms uncertainty on Perdstat.errorfloataSemi-major axis of the planetAUphys.size.smajAxisfloatRmaxMaximum radius in Earth radius (4)phys.angSize;srcfloatTeffEffective temperatureKphys.temperature.effectiveintPtransprobability to transitstat.fit.goodnessfloatSimbadSimbad 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.main