Journal
ASTRONOMICAL JOURNAL
Volume 144, Issue 5, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0004-6256/144/5/139
Keywords
planetary systems; stars: individual (GSC 1364-01424, GSC 3607-01028, GSC 0488-02442); techniques: photometric; techniques: spectroscopic
Categories
Funding
- NOAO [A201Hr, A289Hr, A284Hr]
- NASA [N049Hr, N018Hr, N167Hr, N029Hr, N108Hr, N154Hr, NNG04GN74G, NNX08AF23G, NNX09AB29G, NNX09AF59G]
- NOAO Gemini/Keck time-exchange program [G329Hr]
- SAO IRD grants
- NSF [AST-1108686]
- Kepler mission under NASA [NCC2-1390]
- Hungarian Scientific Research Foundation (OTKA) [K-81373]
- Direct For Mathematical & Physical Scien
- Division Of Astronomical Sciences [1108686] Funding Source: National Science Foundation
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We report the discovery of three new transiting extrasolar planets orbiting moderately bright (V = 11.1, 11.7, and 12.4) F stars. The planets HAT-P-39b through HAT-P-41b have periods of P = 3.5439 days, 4.4572 days, and 2.6940 days, masses of 0.60 M-J, 0.62 M-J, and 0.80 M-J, and radii of 1.57 R-J, 1.73 R-J, and 1.68 R-J, respectively. They orbit stars with masses of 1.40 M-circle dot, 1.51 M-circle dot, and 1.51 M-circle dot, respectively. The three planets are members of an emerging population of highly inflated Jupiters with 0.4 M-J < M < 1.5 M-J and R > 1.5 R-J.
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