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

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    Date
    2015-04
    Author
    Mullally, F.
    Coughlin, Jeffrey L.
    Thompson, Susan E.
    Rowe, Jason
    Burke, Christopher
    Latham, David W.
    Batalha, Natalie M.
    Bryson, Stephen T.
    Christiansen, Jessie
    Henze, Christopher E.
    Ofir, Aviv
    Quarles, Billy
    Shporer, Avi
    Van Eylen, Vincent
    Van Laerhoven, Christa
    Shah, Yash
    Wolfgang, Angie
    Chaplin, W. J.
    Xie, Ji-Wei
    Akeson, Rachel
    Argabright, Vic
    Bachtell, Eric
    Barclay, Thomas
    Borucki, William J.
    Caldwell, Douglas A.
    Campbell, Jennifer R.
    Catanzarite, Joseph H.
    Cochran, William D.
    Duren, Riley M.
    Fleming, Scott W.
    Fraquelli, Dorothy
    Girouard, Forrest R.
    Haas, Michael R.
    Helminiak, Krzysztof G.
    Howell, Steve B.
    Huber, Daniel
    Larson, Kipp
    Gautier, Thomas N., III
    Jenkins, Jon M.
    Li, Jie
    Lissauer, Jack J.
    McArthur, Scot
    Miller, Chris
    Morris, Robert L.
    Patil-Sabale, Anima
    Plavchan, Peter
    Putnam, Dustin
    Quintana, Elisa V.
    Ramirez, Solange
    Aguirre, V. Silva
    Seader, Shawn
    Smith, Jeffrey C.
    Steffen, Jason H.
    Stewart, Chris
    Stober, Jeremy
    Still, Martin
    Tenenbaum, Peter
    Troeltzsch, John
    Twicken, Joseph D.
    Zamudio, Khadeejah A.
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    Abstract
    We 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.
    Department
    McDonald Observatory
    Subject
    catalogs
    eclipses
    planetary systems
    systematic-error correction
    potential transit signals
    main-sequence
    stars
    earth-sized planet
    solar-type stars
    1st 12 quarters
    eclipsing
    binaries
    light-curve
    habitable zone
    input catalog
    astronomy & astrophysics
    URI
    http://hdl.handle.net/2152/42977
    Citation
    Mullally, 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. Harvard
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    • facebook
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    • CONTACT US
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    • Adobe Reader
    Subscribe to our NewsletterGive to the Libraries

    © The University of Texas at Austin