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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. 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Bieryla, B. Beky, D. W. Latham, E. Falco, G. A. Bakos, G. A. Esquerdo, G. Kovacs, G. Torres, I. Boisse, I. Papp, J. D. Hartman, J. Lazar, K. Penev, L. A. Buchhave, M. C. Calkins, M. de Val-Borro, P. Berlind, P. Sari, R. W. Noyes, W. Bhatti, Z. Csubry","submitted_at":"2014-01-21T20:57:50Z","abstract_excerpt":"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. 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