The distribution of transit durations for Kepler planet candidates and implications for their orbital eccentricities

Astrophysical Journal, Supplement Series

Volumn 197, Issue 1, 2011, Pages

  Moorhead, Althea V ^a   Ford, Eric B ^a   Morehead, Robert C ^a   Rowe, Jason ^b,c   Borucki, William J ^c   Batalha, Natalie M ^d   Bryson, Stephen T ^c   Caldwell, Douglas A ^b,c   Fabrycky, Daniel C ^e   Gautier, Thomas N ^f   Koch, David G ^c   Holman, Matthew J ^g   Jenkins, Jon M ^b,c   Li, Jie ^b,c   Lissauer, Jack J ^c   Lucas, Philip ^h   Marcy, Geoffrey W ⁱ   Quinn, Samuel N ^g   Quintana, Elisa ^b,c   Ragozzine, Darin ^g   Shporer, Avi ^i,j   Still, Martin ^c,i   Torres, Guillermo ^g   more..

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

^b SETI INSTITUTE   (United States)

^c NASA AMES RESEARCH CENTER   (United States)

^d SAN JOSE STATE UNIVERSITY   (United States)

^e University of California Santa Cruz   (United States)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^g HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^h UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

ⁱ UNIVERSITY OF CALIFORNIA   (United States)

^j LAS CUMBRES OBSERVATORY GLOBAL TELESCOPE NETWORK   (United States)

more..

Author keywords

fundamental parameters; planets and satellites

Indexed keywords

EID: 80655124830     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1088/0067-0049/197/1/1     Document Type: Article

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