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 ☉ , 1.51 M ☉ , and 1.51 M ☉ , 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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Hartman et al. (2012) studied this question.
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