J/PASP/128/G4502ivo://CDS.VizieR/J/PASP/128/G4502doi:10.26093/cds/vizier.61293502CDSMullally F.Coughlin J.L.Thompson S.E.Christiansen J.Burke C.,Clarke B.D.Haas M.R.2025-09-09T14:14:45Z2017-08-28T14:08:40ZCDS support team

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

cds-question@unistra.frmultiple-starssolar-system-planetsWe present a new automated method to identify instrumental features masquerading as small, long-period planets in the Kepler planet candidate catalog. These systematics, mistakenly identified as planet transits, can have a strong impact on occurrence rate calculations because they cluster in a region of parameter space where Kepler's sensitivity to planets is poor. We compare individual transit-like events to a variety of models of real transits and systematic events and use a Bayesian information criterion to evaluate the likelihood that each event is real. We describe our technique and test its performance on simulated data. Results from this technique are incorporated in the Kepler Q1-Q17 DR24 planet candidate catalog of Coughlin et al. (2016, Cat. J/ApJS/224/12)2016PASP..128g4502Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASP/128/G4502CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toV/133 : Kepler Input Catalog (Kepler Mission Team, 2009)J/ApJS/217/18 : Potential transit signals in Kepler Q1-Q17 (Seader+, 2015)J/ApJS/224/12 : Kepler planetary candidates. VII. 48-month (Coughlin+, 2016)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PASP/128/G4502https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PASP/128/G4502http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PASP/128/G4502https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/PASP/128/G4502https://vizier.iucaa.in/viz-bin/votable?-source=J/PASP/128/G4502http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/PASP/128/G4502GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/PASP/128/G4502/table1 (Summary of planet candidate KOIs from Q1-Q17 DR24 with periods greater than 150 days examined by Marshall)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/PASP/128/G4502/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/PASP/128/G4502/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/PASP/128/G4502/table1?GETtext/xml+votable180.050000true289.217547.884460.0055555555555555565/3646 3683 3690-3691 3694-3695 3704 3731 3733-3735 3741 3777 3782 3785-3786 3789 3792 6/14578-14579 14581-14583 14588-14589 14591 14730-14731 14744 14746 14750-14753 14755 14757-14759 14769-14772 14774 14792 14795 14824-14825 14827 14916 14918-14919 14921 14928-14930 14948-14949 14953 14955-14957 14959-14960 14969 14971 14973 14975 15040 15044-15045 15060 15104 15107 15113-15114 15116 15118-15121 15124-15126 15132 15134 15136 15139 15150 15153 15160-15161 15172 15174 15200https://cdsarc.cds.unistra.fr/viz-bin/moc/J/PASP/128/G4502?format=asciidefaultJ/PASP/128/G4502/table1Summary of planet candidate KOIs from Q1-Q17 DR24 with periods greater than 150 days examined by MarshallrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintKOIKOI name (KNNNNN.NN)meta.idcharKICKepler identification numbermeta.id;meta.mainintTCEThreshold crossing event. Order in which this KOI was found around the target star by the Kepler pipeline in Q1-Q17stat.fit.paramintNTransNumber of observed transits as measured by the pipelinemeta.numberintPerPeriod (1)dtime.perioddoublee_Per? rms uncertainty on Perdstat.errordoublenullableRadRadius in R_{Earth}_ (1)(6.3781x10+6m)phys.angSize;srcdoublee_Rad? rms uncertainty on Rad(6.3781x10+6m)stat.errordoublenullableScoreConfidence Marshall assigns to a KOI (2)stat.fit.goodnessdoubleSimbadSimbad column added by the CDSmeta.ref.urlchar_RAPositions from KIC catalog (right ascension part)degpos.eq.ra;meta.main_DEPositions from KIC catalog (declination part)degpos.eq.dec;meta.main