PLANETARY CANDIDATES OBSERVED BY KEPLER. V. PLANET SAMPLE FROM Q1-Q12 (36 MONTHS)

被引：142

作者：

Rowe, Jason F. ^{[1
,2
]}

Coughlin, Jeffrey L. ^{[1
]}

Antoci, Victoria ^{[3
]}

Barclay, Thomas ^{[2
,4
]}

Batalha, Natalie M. ^{[2
]}

Borucki, William J. ^{[2
]}

Burke, Christopher J. ^{[1
,2
]}

Bryson, Steven T. ^{[2
]}

Caldwell, Douglas A. ^{[1
,2
]}

Campbell, Jennifer R. ^{[2
,5
]}

Catanzarite, Joseph H. ^{[1
]}

Christiansen, Jessie L. ^{[6
]}

Cochran, William ^{[7
]}

Gilliland, Ronald L. ^{[8
]}

Girouard, Forrest R. ^{[9
]}

Haas, Michael R. ^{[2
]}

Helminiak, Krzysztof G. ^{[10
]}

Henze, Christopher E. ^{[2
]}

Hoffman, Kelsey L. ^{[1
,2
]}

Howell, Steve B. ^{[2
]}

Huber, Daniel ^{[1
,2
,11
]}

Hunter, Roger C. ^{[2
]}

Jang-Condell, Hannah ^{[12
]}

Jenkins, Jon M. ^{[2
]}

Klaus, Todd C. ^{[13
]}

Latham, David W. ^{[14
]}

Li, Jie ^{[1
]}

Lissauer, Jack J. ^{[2
]}

McCauliff, Sean D. ^{[5
]}

Morris, Robert L. ^{[1
]}

Mullally, F. ^{[2
]}

Ofir, Aviv ^{[15
,16
]}

Quarles, Billy ^{[2
]}

Quintana, Elisa ^{[2
]}

Sabale, Anima ^{[5
]}

Seader, Shawn ^{[1
,2
]}

Shporer, Avi ^{[17
]}

Smith, Jeffrey C. ^{[1
,2
]}

Steffen, Jason H. ^{[18
]}

Still, Martin ^{[2
,4
]}

Tenenbaum, Peter ^{[1
,2
]}

Thompson, Susan E. ^{[1
,2
]}

Twicken, Joseph D. ^{[1
]}

Van Laerhoven, Christa ^{[19
,20
]}

Wolfgang, Angie ^{[21
]}

Zamudio, Khadeejah A. ^{[2
,5
]}

机构：

[1] SETI Inst, Mountain View, CA 94043 USA

[2] NASA Ames Res Ctr, Moffett Field, CA 94035 USA

[3] Aarhus Univ, Stellar Astrophys Ctr, DK-8000 Aarhus C, Denmark

[4] Bay Area Environm Res Inst, Sonoma, CA 95476 USA

[5] Wyle Labs, Moffett Field, CA 94035 USA

[6] CALTECH, NASA Exoplanet Sci Inst, Pasadena, CA 91106 USA

[7] Univ Texas Austin, Dept Astron & McDonald Observ, Austin, TX 78712 USA

[8] Penn State Univ, Ctr Exoplanets & Habitable Words, University Pk, PA 16802 USA

[9] Logyx LLC, Mountain View, CA 94043 USA

[10] Natl Inst Nat Sci, Natl Astron Observ Japan, Subaru Telescope, Hilo, HI 96720 USA

[11] Univ Sydney, Sch Phys, Sydney Inst Astron SIfA, Sydney, NSW 2006, Australia

[12] Univ Wyoming, Dept Phys & Astron, Laramie, WY 82071 USA

[13] Moon Express Inc, Moffett Field, CA 94035 USA

[14] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

[15] Weizmann Inst Sci, IL-76100 Rehovot, Israel

[16] Univ Gottingen, Inst Astrophys, D-37077 Gottingen, Germany

[17] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

[18] Northwestern Univ, CIERA, Evanston, IL 60208 USA

[19] Univ Arizona, Tucson, AZ USA

[20] Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada

[21] Univ Calif Santa Cruz, Santa Cruz, CA 95064 USA

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2015年 / 217卷 / 01期

基金：

澳大利亚研究理事会; 欧洲研究理事会; 新加坡国家研究基金会;

关键词：

catalogs; planets and satellites: fundamental parameters; TRANSIT TIMING OBSERVATIONS; FALSE-POSITIVE RATE; M-DWARF STARS; ECLIPSING BINARIES; DATA RELEASE; HABITABLE ZONE; LIGHT CURVES; EXOPLANET; II; SYSTEMS;

D O I：

10.1088/0067-0049/217/1/16

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Kepler mission discovered 2842 exoplanet candidates with 2 yr of data. We provide updates to the Kepler planet candidate sample based upon 3 yr (Q1-Q12) of data. Through a series of tests to exclude false-positives, primarily caused by eclipsing binary stars and instrumental systematics, 855 additional planetary candidates have been discovered, bringing the total number known to 3697. We provide revised transit parameters and accompanying posterior distributions based on a Markov Chain Monte Carlo algorithm for the cumulative catalog of Kepler Objects of Interest. There are now 130 candidates in the cumulative catalog that receive less than twice the flux the Earth receives and more than 1100 have a radius less than 1.5 R-circle plus. There are now a dozen candidates meeting both criteria, roughly doubling the number of candidate Earth analogs. A majority of planetary candidates have a high probability of being bonafide planets, however, there are populations of likely false-positives. We discuss and suggest additional cuts that can be easily applied to the catalog to produce a set of planetary candidates with good fidelity. The full catalog is publicly available at the NASA Exoplanet Archive.

引用

页数：22

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