Transit timing observations from Kepler. V. Transit timing variation candidates in the first sixteen months from polynomial models

Astrophysical Journal

Volumn 756, Issue 2, 2012, Pages

  Ford, Eric B ^a   Ragozzine, Darin ^b   Rowe, Jason F ^c,d   Steffen, Jason H ^e   Barclay, Thomas ^c,f   Batalha, Natalie M ^g   Borucki, William J ^c   Bryson, Stephen T ^c   Caldwell, Douglas A ^c,d   Fabrycky, Daniel C ^h   Gautier, Thomas N ⁱ   Holman, Matthew J ^b   Ibrahim, Khadeejah A ^c   Kjeldsen, Hans ^j   Kinemuchi, Karen ^c,f   Koch, David G ^c   Lissauer, Jack J ^c   Still, Martin ^c,f   Tenenbaum, Peter ^c,d   Uddin, Kamal ^c   Welsh, William ^k   more..

^a 211 Bryant Space Sciences Center ^*  (United States)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c NASA AMES RESEARCH CENTER   (United States)

^d SETI INSTITUTE   (United States)

^e NASA FERMILAB ASTROPHYSICS CENTER   (United States)

^f BAY AREA ENVIRONMENTAL RESEARCH INSTITUTE   (United States)

^g SAN JOSE STATE UNIVERSITY   (United States)

^h University of California Santa Cruz   (United States)

ⁱ CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^j AARHUS UNIVERSITY   (Denmark)

^k SAN DIEGO STATE UNIVERSITY   (United States)

more..

Author keywords

planetary systems; planets and satellites: detection; planets and satellites: dynamical evolution and stability; techniques: miscellaneous

Indexed keywords

EID: 84865609542     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/756/2/185     Document Type: Article

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