Planetary Candidates Observed By Kepler Iv: Planet Sample from Q1-Q8 (22 Months)

dc.contributor.utaustinauthorCochran, William D.en_US
dc.creatorBurke, Christopher J.en_US
dc.creatorBryson, Stephen T.en_US
dc.creatorMullally, F.en_US
dc.creatorRowe, Jason F.en_US
dc.creatorChristiansen, Jessie L.en_US
dc.creatorThompson, Susan E.en_US
dc.creatorCoughlin, Jeffrey L.en_US
dc.creatorHaas, Michael R.en_US
dc.creatorBatalha, Natalie M.en_US
dc.creatorCaldwell, Douglas A.en_US
dc.creatorJenkins, Jon M.en_US
dc.creatorStill, Martinen_US
dc.creatorBarclay, Thomasen_US
dc.creatorBorucki, William J.en_US
dc.creatorChaplin, William J.en_US
dc.creatorCiardi, David R.en_US
dc.creatorClarke, Bruce D.en_US
dc.creatorCochran, William D.en_US
dc.creatorDemory, Brice-Olivieren_US
dc.creatorEsquerdo, Gilbert A.en_US
dc.creatorGautier, Thomas N., IIIen_US
dc.creatorGilliland, Ronald L.en_US
dc.creatorGirouard, Forrest R.en_US
dc.creatorHavel, Mathieuen_US
dc.creatorHenze, Christopher E.en_US
dc.creatorHowell, Steve B.en_US
dc.creatorHuber, Danielen_US
dc.creatorLatham, David W.en_US
dc.creatorLi, Jieen_US
dc.creatorMorehead, Robert C.en_US
dc.creatorMorton, Timothy D.en_US
dc.creatorPepper, Joshuaen_US
dc.creatorQuintana, Elisaen_US
dc.creatorRagozzine, Darinen_US
dc.creatorSeader, Shawn E.en_US
dc.creatorShah, Yashen_US
dc.creatorShporer, Avien_US
dc.creatorTenenbaum, Peteren_US
dc.creatorTwicken, Joseph D.en_US
dc.creatorWolfgang, Angieen_US
dc.date.accessioned2016-10-28T19:35:27Z
dc.date.available2016-10-28T19:35:27Z
dc.date.issued2014-02en_US
dc.description.abstractWe provide updates to the Kepler planet candidate sample based upon nearly two years of high-precision photometry (i.e., Q1-Q8). From an initial list of nearly 13,400 threshold crossing events, 480 new host stars are identified from their flux time series as consistent with hosting transiting planets. Potential transit signals are subjected to further analysis using the pixel-level data, which allows background eclipsing binaries to be identified through small image position shifts during transit. We also re-evaluate Kepler Objects of Interest (KOIs) 1-1609, which were identified early in the mission, using substantially more data to test for background false positives and to find additional multiple systems. Combining the new and previous KOI samples, we provide updated parameters for 2738 Kepler planet candidates distributed across 2017 host stars. From the combined Kepler planet candidates, 472 are new from the Q1-Q8 data examined in this study. The new Kepler planet candidates represent similar to 40% of the sample with R-P similar to 1R(circle plus) and represent similar to 40% of the low equilibrium temperature (T-eq < 300 K) sample. We review the known biases in the current sample of Kepler planet candidates relevant to evaluating planet population statistics with the current Kepler planet candidate sample.en_US
dc.description.departmentAstronomyen_US
dc.description.sponsorshipNASA Postdoctoral Program at Ames Research Centeren_US
dc.identifierdoi:10.15781/T27S7HV83
dc.identifier.citationBurke, Christopher J., Stephen T. Bryson, F. Mullally, Jason F. Rowe, Jessie L. Christiansen, Susan E. Thompson, Jeffrey L. Coughlin et al. "Planetary candidates observed by Kepler IV: Planet sample from Q1-Q8 (22 Months)." The Astrophysical Journal Supplement Series, Vol. 210, No. 2 (Feb., 2014): 19.en_US
dc.identifier.doi10.1088/0067-0049/210/2/19en_US
dc.identifier.issn0067-0049en_US
dc.identifier.urihttp://hdl.handle.net/2152/42973
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.subjectspace vehiclesen_US
dc.subjecttransit timing observationsen_US
dc.subjectsun-like staren_US
dc.subject1st 4 monthsen_US
dc.subjecthabitableen_US
dc.subjectzoneen_US
dc.subjectlight curvesen_US
dc.subjecteclipsing binariesen_US
dc.subjecterror-correctionen_US
dc.subjectfalseen_US
dc.subjectpositivesen_US
dc.subjectblend scenariosen_US
dc.subjectmultiple systemen_US
dc.subjectastronomy & astrophysicsen_US
dc.titlePlanetary Candidates Observed By Kepler Iv: Planet Sample from Q1-Q8 (22 Months)en_US
dc.typeArticleen_US

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