HAT-P-49b: A 1.7 MJ planet transiting a bright 1.5 M⊙F-star

A. Bieryla; J. D. Hartman; G. Á Bakos; W. Bhatti; G. Kovács; I. Boisse; D. W. Latham; L. A. Buchhave; Z. Csubry; K. Penev; M. De Val-Borro; B. Béky; E. Falco; G. Torres; R. W. Noyes; P. Berlind; M. C. Calkins; G. A. Esquerdo; J. Lázár; I. Papp; P. Sári

doi:10.1088/0004-6256/147/4/84

HAT-P-49b: A 1.7 M_J planet transiting a bright 1.5 M⊙F-star

A. Bieryla, J. D. Hartman, G. Á Bakos, W. Bhatti, G. Kovács, I. Boisse, D. W. Latham, L. A. Buchhave, Z. Csubry, K. Penev, M. De Val-Borro, B. Béky, E. Falco, G. Torres, R. W. Noyes, P. Berlind, M. C. Calkins, G. A. Esquerdo, J. Lázár, I. PappP. Sári

Astrophysical Sciences

Research output: Contribution to journal › Article › peer-review

24 Scopus citations

Abstract

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 1.54 M⊙and a radius of 1.83 R ⊙ . 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 host star's fast rotation, 16 km s^-1. The planetary companion has a period of 2.6915 days, 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.

Original language	English (US)
Article number	84
Journal	Astronomical Journal
Volume	147
Issue number	4
DOIs	https://doi.org/10.1088/0004-6256/147/4/84
State	Published - Apr 2014

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

HD 340099)techniques
individual (HAT-P-49
photometrictechniques
planetary systems stars
spectroscopic

Access to Document

10.1088/0004-6256/147/4/84

Cite this

Bieryla, A., Hartman, J. D., Bakos, G. Á., Bhatti, W., Kovács, G., Boisse, I., Latham, D. W., Buchhave, L. A., Csubry, Z., Penev, K., De Val-Borro, M., Béky, B., Falco, E., Torres, G., Noyes, R. W., Berlind, P., Calkins, M. C., Esquerdo, G. A., Lázár, J., ... Sári, P. (2014). HAT-P-49b: A 1.7 M_J planet transiting a bright 1.5 M⊙F-star. Astronomical Journal, 147(4), Article 84. https://doi.org/10.1088/0004-6256/147/4/84

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title = "HAT-P-49b: A 1.7 MJ planet transiting a bright 1.5 M⊙F-star",

abstract = "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 1.54 M⊙and a radius of 1.83 R ⊙ . 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 host star's fast rotation, 16 km s-1. The planetary companion has a period of 2.6915 days, 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 Mp and Rp well determined.",

keywords = "HD 340099)techniques, individual (HAT-P-49, photometrictechniques, planetary systems stars, spectroscopic",

author = "A. Bieryla and Hartman, {J. D.} and Bakos, {G. {\'A}} and W. Bhatti and G. Kov{\'a}cs and I. Boisse and Latham, {D. W.} and Buchhave, {L. A.} and Z. Csubry and K. Penev and {De Val-Borro}, M. and B. B{\'e}ky and E. Falco and G. Torres and Noyes, {R. W.} and P. Berlind and Calkins, {M. C.} and Esquerdo, {G. A.} and J. L{\'a}z{\'a}r and I. Papp and P. S{\'a}ri",

year = "2014",

month = apr,

doi = "10.1088/0004-6256/147/4/84",

language = "English (US)",

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Bieryla, A, Hartman, JD , Bakos, GÁ, Bhatti, W, Kovács, G, Boisse, I, Latham, DW, Buchhave, LA, Csubry, Z, Penev, K, De Val-Borro, M, Béky, B, Falco, E, Torres, G, Noyes, RW, Berlind, P, Calkins, MC, Esquerdo, GA, Lázár, J, Papp, I & Sári, P 2014, 'HAT-P-49b: A 1.7 M_J planet transiting a bright 1.5 M⊙F-star', Astronomical Journal, vol. 147, no. 4, 84. https://doi.org/10.1088/0004-6256/147/4/84

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T2 - A 1.7 MJ planet transiting a bright 1.5 M⊙F-star

AU - Bieryla, A.

AU - Hartman, J. D.

AU - Bakos, G. Á

AU - Bhatti, W.

AU - Kovács, G.

AU - Boisse, I.

AU - Latham, D. W.

AU - Buchhave, L. A.

AU - Csubry, Z.

AU - Penev, K.

AU - De Val-Borro, M.

AU - Béky, B.

AU - Falco, E.

AU - Torres, G.

AU - Noyes, R. W.

AU - Berlind, P.

AU - Calkins, M. C.

AU - Esquerdo, G. A.

AU - Lázár, J.

AU - Papp, I.

AU - Sári, P.

PY - 2014/4

Y1 - 2014/4

N2 - 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 1.54 M⊙and a radius of 1.83 R ⊙ . 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 host star's fast rotation, 16 km s-1. The planetary companion has a period of 2.6915 days, 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 Mp and Rp well determined.

AB - 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 1.54 M⊙and a radius of 1.83 R ⊙ . 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 host star's fast rotation, 16 km s-1. The planetary companion has a period of 2.6915 days, 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 Mp and Rp well determined.

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KW - individual (HAT-P-49

KW - photometrictechniques

KW - planetary systems stars

KW - spectroscopic

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