PLANETARY CANDIDATES OBSERVED BY KEPLER. VI. PLANET SAMPLE FROM Q1-Q16 (47 MONTHS)

被引：202

作者：

Mullally, F. ^{[1
]}

Coughlin, Jeffrey L. ^{[1
]}

Thompson, Susan E. ^{[1
]}

Rowe, Jason ^{[1
]}

Burke, Christopher ^{[1
]}

Latham, David W. ^{[2
]}

Batalha, Natalie M. ^{[3
]}

Bryson, Stephen T. ^{[3
]}

Christiansen, Jessie ^{[4
]}

Henze, Christopher E. ^{[3
]}

Ofir, Aviv ^{[5
,6
]}

Quarles, Billy ^{[7
]}

Shporer, Avi ^{[8
]}

Van Eylen, Vincent ^{[9
]}

Van Laerhoven, Christa ^{[10
]}

Shah, Yash ^{[11
]}

Wolfgang, Angie ^{[12
]}

Chaplin, W. J. ^{[9
,13
]}

Xie, Ji-Wei ^{[14
]}

Akeson, Rachel ^{[4
]}

Argabright, Vic ^{[15
]}

Bachtell, Eric ^{[15
]}

Barclay, Thomas ^{[16
]}

Borucki, William J. ^{[3
]}

Caldwell, Douglas A. ^{[1
]}

Campbell, Jennifer R.

Catanzarite, Joseph H. ^{[1
]}

Cochran, William D. ^{[18
,19
]}

Duren, Riley M. ^{[20
]}

Fleming, Scott W. ^{[21
]}

Fraquelli, Dorothy ^{[21
]}

Girouard, Forrest R. ^{[22
]}

Haas, Michael R. ^{[3
]}

Helminiak, Krzysztof G. ^{[23
]}

Howell, Steve B. ^{[3
]}

Huber, Daniel ^{[1
,24
]}

Larson, Kipp ^{[15
]}

Gautier, Thomas N., III

Jenkins, Jon M. ^{[1
]}

Li, Jie ^{[1
]}

Lissauer, Jack J. ^{[3
]}

McArthur, Scot

Miller, Chris ^{[15
]}

Morris, Robert L. ^{[1
]}

Patil-Sabale, Anima ^{[17
]}

Plavchan, Peter ^{[25
]}

Putnam, Dustin ^{[15
]}

Quintana, Elisa V. ^{[1
]}

Ramirez, Solange ^{[4
]}

Aguirre, V. Silva ^{[9
]}

机构：

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

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

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

[4] CALTECH, NASA, Exoplanet Sci Inst, Pasadena, CA 91125 USA

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

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

[7] NASA, Ames Res Ctr, Space Sci & Astrobiol Div, Moffett Field, CA 94035 USA

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

[9] Aarhus Univ, Dept Phys & Astron, Stellar Astrophys Ctr, DK-8000 Aarhus C, Denmark

[10] Dept Planetary Sci, Tucson, AZ USA

[11] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA

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

[13] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England

[14] Nanjing Univ, Minist Educ, Astron & Astrophys, Nanjing 210093, Jiangsu, Peoples R China

[15] Ball Aerosp & Technol Corp, Boulder, CO 80301 USA

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

[17] NASA, Ames Res Ctr, Wyle Labs, Moffett Field, CA 94035 USA

[18] Univ Texas Austin, McDonald Observ, Austin, TX 78712 USA

[19] Univ Texas Austin, Dept Astron, Austin, TX 78712 USA

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

[21] Space Telescope Sci Inst, Comp Sci Corp, Baltimore, MD 21218 USA

[22] NASA, Ames Res Ctr, Orbital Sci Corp, Moffett Field, CA 94035 USA

[23] Natl Astron Observ Japan, Subaru Telescope, Hilo, HI 96720 USA

[24] Univ Sydney, Sch Phys, SIfA, Sydney, NSW 2006, Australia

[25] Dept Phys Astron & Mat Sci, Springfield, MO 65897 USA

[26] Northwestern Univ, Ctr Interdisciplinary Res & Explorat Astron CIERA, Dept Phys & Astron, Evanston, IL 60208 USA

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2015年 / 217卷 / 02期

基金：

美国国家航空航天局; 欧洲研究理事会; 新加坡国家研究基金会;

关键词：

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;

D O I：

10.1088/0067-0049/217/2/31

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页数：16

共 9 条

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