Transit timing observations from Kepler. VI. Potentially interesting candidate systems from fourier-based statistical tests

Astrophysical Journal

Volumn 756, Issue 2, 2012, Pages

  Steffen, Jason H ^a   Ford, Eric B ^b   Rowe, Jason F ^c,d   Fabrycky, Daniel C ^e   Holman, Matthew J ^f   Welsh, William F ^g   Batalha, Natalie M ^h   Borucki, William J ^c   Bryson, Steve ^c   Caldwell, Douglas A ^c,d   Ciardi, David R ⁱ   Jenkins, Jon M ^c,d   Kjeldsen, Hans ^j   Koch, David G ^c   Prša, Andrej ^k   Sanderfer, Dwight T ^c   Seader, Shawn ^c   Twicken, Joseph D ^c,d  

^a NASA FERMILAB ASTROPHYSICS CENTER   (United States)

^b University of Florida   (United States)

^c NASA AMES RESEARCH CENTER   (United States)

^d SETI INSTITUTE   (United States)

^e University of California at Santa Cruz   (United States)

^f HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^g SAN DIEGO STATE UNIVERSITY   (United States)

^h SAN JOSE STATE UNIVERSITY   (United States)

ⁱ CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^j AARHUS UNIVERSITY   (Denmark)

^k VILLANOVA UNIVERSITY   (United States)

more..

Author keywords

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

Indexed keywords

EID: 84865608513     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/756/2/186     Document Type: Article

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