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HAT-P-49b: A 1.7 M_J Planet Transiting a Bright 1.5 M_S F-Star

We report the discovery of the transiting extrasolar planet HAT-P-49b. The planet transits the bright (V = 10.3) slightly evolved F-star HD 340099 with a mass of 1.54M_S and a radius of 1.83 R_S. HAT-P-49b is orbiting one of the 25 brightest stars to host a transiting planet which makes this a favorable candidate for detailed follow-up. This system is an especially strong target for Rossiter- McLaughlin follow-up due to the fast rotation of the host star, 16 km/s. The planetary companion has a period of 2.6915 d, mass of 1.73 M_J and radius of 1.41 R_J. The planetary characteristics are consistent with that of a classical hot Jupiter but we note that this is the fourth most massive star to host a transiting planet with both M_p and R_p well determined.

preprint2014arXivOpen access
A. BierylaJ. D. HartmanG. A. BakosW. BhattiG. KovacsI. BoisseD. W. LathamL. A. BuchhaveZ. CsubryK. PenevM. de Val-BorroB. BekyE. FalcoG. TorresR. W. NoyesP. BerlindM. C. CalkinsG. A. EsquerdoJ. LazarI. PappP. Sari
astro-ph.EP
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A. BierylaJ. D. HartmanG. A. BakosW. BhattiG. KovacsI. BoisseD. W. LathamL. A. BuchhaveZ. CsubryK. PenevM. de Val-BorroB. BekyE. FalcoG. TorresR. W. NoyesP. BerlindM. C. CalkinsG. A. EsquerdoJ. LazarI. PappP. Sari

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