The transit light curve project. IX. Evidence for a smaller radius of the exoplanet XO-3b

Astrophysical Journal

Volumn 683, Issue 2, 2008, Pages 1076-1084

  Winn, Joshua N ^a   Holman, Matthew J ^b   Torres, Guillermo ^b   Mccullough, Peter ^c   Johns Krull, Christopher ^d   Latham, David W ^b   Shporer, Avi ^e   Mazeh, Tsevi ^e   Garcia Melendo, Enrique ^f   Foote, Cindy ^g   Esquerdo, Gil ^b   Everett, Mark ^h  

^a MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c STScI   (United States)

^d RICE UNIVERSITY   (United States)

^e TEL AVIV UNIVERSITY   (Israel)

^f Esteve Duran Observatory   (Spain)

^g Vermillion Cliffs Observatory   (United States)

^h PLANETARY SCIENCE INSTITUTE   (United States)

Author keywords

Planetary systems; Stars: individual (GSC 03727 01064, XO 3)

Indexed keywords

EID: 51349168763     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/589737     Document Type: Article

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