PLANETARY CANDIDATES OBSERVED BY KEPLER . V. PLANET SAMPLE FROM Q1–Q12 (36 MONTHS)-Reference-Cited by-同舟云学术

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

Published:2015-03-24 Issue:1 Volume:217 Page:16
ISSN:1538-4365
Container-title:The Astrophysical Journal Supplement Series
language:
Short-container-title:ApJS

Author:

Rowe Jason F.,Coughlin Jeffrey L.,Antoci Victoria,Barclay Thomas^ORCID,Batalha Natalie M.,Borucki William J.,Burke Christopher J.,Bryson Steven T.,Caldwell Douglas A.,Campbell Jennifer R.,Catanzarite Joseph H.,Christiansen Jessie L.,Cochran William,Gilliland Ronald L.,Girouard Forrest R.,Haas Michael R.,Hełminiak Krzysztof G.,Henze Christopher E.,Hoffman Kelsey L.,Howell Steve B.,Huber Daniel,Hunter Roger C.,Jang-Condell Hannah,Jenkins Jon M.,Klaus Todd C.,Latham David W.,Li Jie,Lissauer Jack J.,McCauliff Sean D.,Morris Robert L.,Mullally F.,Ofir Aviv,Quarles Billy,Quintana Elisa,Sabale Anima,Seader Shawn,Shporer Avi^ORCID,Smith Jeffrey C.,Steffen Jason H.,Still Martin,Tenenbaum Peter,Thompson Susan E.,Twicken Joseph D.,Laerhoven Christa Van,Wolfgang Angie,Zamudio Khadeejah A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.1088/0067-0049/217/1/16/pdf

Reference74 articles.

1. ADAPTIVE OPTICS IMAGES OFKEPLEROBJECTS OF INTEREST

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3. Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458

4. A sub-Mercury-sized exoplanet

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