Planetary Candidates Observed By Kepler. Vi. Planet Sample from Q1-Q16 (47 Months)

dc.contributor.utaustinauthorCochran, William D.en_US
dc.creatorMullally, F.en_US
dc.creatorCoughlin, Jeffrey L.en_US
dc.creatorThompson, Susan E.en_US
dc.creatorRowe, Jasonen_US
dc.creatorBurke, Christopheren_US
dc.creatorLatham, David W.en_US
dc.creatorBatalha, Natalie M.en_US
dc.creatorBryson, Stephen T.en_US
dc.creatorChristiansen, Jessieen_US
dc.creatorHenze, Christopher E.en_US
dc.creatorOfir, Aviven_US
dc.creatorQuarles, Billyen_US
dc.creatorShporer, Avien_US
dc.creatorVan Eylen, Vincenten_US
dc.creatorVan Laerhoven, Christaen_US
dc.creatorShah, Yashen_US
dc.creatorWolfgang, Angieen_US
dc.creatorChaplin, W. J.en_US
dc.creatorXie, Ji-Weien_US
dc.creatorAkeson, Rachelen_US
dc.creatorArgabright, Vicen_US
dc.creatorBachtell, Ericen_US
dc.creatorBarclay, Thomasen_US
dc.creatorBorucki, William J.en_US
dc.creatorCaldwell, Douglas A.en_US
dc.creatorCampbell, Jennifer R.en_US
dc.creatorCatanzarite, Joseph H.en_US
dc.creatorCochran, William D.en_US
dc.creatorDuren, Riley M.en_US
dc.creatorFleming, Scott W.en_US
dc.creatorFraquelli, Dorothyen_US
dc.creatorGirouard, Forrest R.en_US
dc.creatorHaas, Michael R.en_US
dc.creatorHelminiak, Krzysztof G.en_US
dc.creatorHowell, Steve B.en_US
dc.creatorHuber, Danielen_US
dc.creatorLarson, Kippen_US
dc.creatorGautier, Thomas N., IIIen_US
dc.creatorJenkins, Jon M.en_US
dc.creatorLi, Jieen_US
dc.creatorLissauer, Jack J.en_US
dc.creatorMcArthur, Scoten_US
dc.creatorMiller, Chrisen_US
dc.creatorMorris, Robert L.en_US
dc.creatorPatil-Sabale, Animaen_US
dc.creatorPlavchan, Peteren_US
dc.creatorPutnam, Dustinen_US
dc.creatorQuintana, Elisa V.en_US
dc.creatorRamirez, Solangeen_US
dc.creatorAguirre, V. Silvaen_US
dc.creatorSeader, Shawnen_US
dc.creatorSmith, Jeffrey C.en_US
dc.creatorSteffen, Jason H.en_US
dc.creatorStewart, Chrisen_US
dc.creatorStober, Jeremyen_US
dc.creatorStill, Martinen_US
dc.creatorTenenbaum, Peteren_US
dc.creatorTroeltzsch, Johnen_US
dc.creatorTwicken, Joseph D.en_US
dc.creatorZamudio, Khadeejah A.en_US
dc.date.accessioned2016-10-28T19:35:31Z
dc.date.available2016-10-28T19:35:31Z
dc.date.issued2015-04en_US
dc.description.abstractWe present the sixth catalog of Kepler candidate planets based on nearly four years of high precision photometry. This catalog builds on the legacy of previous catalogs released by the Kepler project and includes 1493 new Kepler Objects of Interest (KOIs) of which 554 are planet candidates, and 131 of these candidates have best-fit radii < 1.5 R-circle plus. This brings the total number of KOIs and planet candidates to 7348 and 4175 respectively. We suspect that many of these new candidates at the low signal-to-noise ratio limit may be false alarms created by instrumental noise, and discuss our efforts to identify such objects. We re-evaluate all previously published KOIs with orbital periods of >50 days to provide a consistently vetted sample that can be used to improve planet occurrence rate calculations. We discuss the performance of our planet detection algorithms, and the consistency of our vetting products. The full catalog is publicly available at the NASA Exoplanet Archive.en_US
dc.description.departmentMcDonald Observatoryen_US
dc.description.sponsorshipNASAs Science Mission Directorateen_US
dc.description.sponsorshipAssociation of Universities for Research in Astronomy, Inc., under NASA NAS5-26555en_US
dc.description.sponsorshipNASA Office of Space Science NNX13AC07Gen_US
dc.description.sponsorshipNational Aeronautics and Space Administration under the Exoplanet Exploration Programen_US
dc.description.sponsorshipDanish National Research Foundation DNRF106en_US
dc.description.sponsorshipASTERISK project (ASTER-oseismic Investigations with SONG and Kepler) - European Research Council 267864en_US
dc.identifierdoi:10.15781/T2QV3C631
dc.identifier.citationMullally, Fergal, Jeffrey L. Coughlin, Susan E. Thompson, Jason Rowe, Christopher Burke, David W. Latham, Natalie M. Batalha et al. "PLANETARY CANDIDATES OBSERVED BY KEPLER. VI. PLANET SAMPLE FROM Q1–Q16 (47 MONTHS)." The Astrophysical Journal Supplement Series, Vol. 217, No. 2 (Apr., 2015): 31. Harvarden_US
dc.identifier.doi10.1088/0067-0049/217/2/31en_US
dc.identifier.issn0067-0049en_US
dc.identifier.urihttp://hdl.handle.net/2152/42977
dc.language.isoEnglishen_US
dc.relation.ispartofen_US
dc.relation.ispartofserialAstrophysical Journal Supplement Seriesen_US
dc.rightsAdministrative deposit of works to Texas ScholarWorks: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University.en_US
dc.rights.restrictionOpenen_US
dc.subjectcatalogsen_US
dc.subjecteclipsesen_US
dc.subjectplanetary systemsen_US
dc.subjectsystematic-error correctionen_US
dc.subjectpotential transit signalsen_US
dc.subjectmain-sequenceen_US
dc.subjectstarsen_US
dc.subjectearth-sized planeten_US
dc.subjectsolar-type starsen_US
dc.subject1st 12 quartersen_US
dc.subjecteclipsingen_US
dc.subjectbinariesen_US
dc.subjectlight-curveen_US
dc.subjecthabitable zoneen_US
dc.subjectinput catalogen_US
dc.subjectastronomy & astrophysicsen_US
dc.titlePlanetary Candidates Observed By Kepler. Vi. Planet Sample from Q1-Q16 (47 Months)en_US
dc.typeArticleen_US

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