Hats-3b: An inflated hot jupiter transiting an F-type star*

D. Bayliss; G. Zhou; K. Penev; G. Á Bakos; J. D. Hartman; A. Jordán; L. Mancini; M. Mohler-Fischer; V. Suc; M. Rabus; B. Béky; Z. Csubry; L. Buchhave; T. Henning; N. Nikolov; B. Csák; R. Brahm; N. Espinoza; R. W. Noyes; B. Schmidt; P. Conroy; D. J. Wright; C. G. Tinney; B. C. Addison; P. D. Sackett; D. D. Sasselov; J. Lázár; I. Papp; P. Sári

doi:10.1088/0004-6256/146/5/113

P. Conroy, D. J. Wright, C. G. Tinney, B. C. Addison, P. D. Sackett, D. D. Sasselov, J. Lázár, I. Papp, P. Sári

Producción científica: Contribución a una revista › Artículo › revisión exhaustiva

58 Citas (Scopus)

Resumen

We report the discovery by the HATSouth survey of HATS-3b, a transiting extrasolar planet orbiting a V = 12.4 F dwarf star. HATS-3b has a period of P = 3.5479 days, mass of M_p = 1.07 M _J, and radius of R _p = 1.38 R _J. Given the radius of the planet, the brightness of the host star, and the stellar rotational velocity (vsin i = 9.0 km s^-1), this system will make an interesting target for future observations to measure the Rossiter-McLaughlin effect and determine its spin-orbit alignment. We detail the low-/medium-resolution reconnaissance spectroscopy that we are now using to deal with large numbers of transiting planet candidates produced by the HATSouth survey. We show that this important step in discovering planets produces log g and T _eff parameters at a precision suitable for efficient candidate vetting, as well as efficiently identifying stellar mass eclipsing binaries with radial velocity semi-amplitudes as low as 1 km s^-1.

Idioma original	Inglés
Número de artículo	113
Publicación	Astronomical Journal
Volumen	146
N.º	5
DOI	https://doi.org/10.1088/0004-6256/146/5/113
Estado	Publicada - nov 2013
Publicado de forma externa	Sí

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Bayliss, D., Zhou, G., Penev, K., Bakos, G. Á., Hartman, J. D., Jordán, A., Mancini, L., Mohler-Fischer, M., Suc, V., Rabus, M., Béky, B., Csubry, Z., Buchhave, L., Henning, T., Nikolov, N., Csák, B., Brahm, R., Espinoza, N., Noyes, R. W., ... Sári, P. (2013). Hats-3b: An inflated hot jupiter transiting an F-type star*. Astronomical Journal, 146(5), Artículo 113. https://doi.org/10.1088/0004-6256/146/5/113

@article{8b8ec6ee4c3f4657be3c02c69add21a4,

title = "Hats-3b: An inflated hot jupiter transiting an F-type star*",

abstract = "We report the discovery by the HATSouth survey of HATS-3b, a transiting extrasolar planet orbiting a V = 12.4 F dwarf star. HATS-3b has a period of P = 3.5479 days, mass of Mp = 1.07 M J, and radius of R p = 1.38 R J. Given the radius of the planet, the brightness of the host star, and the stellar rotational velocity (vsin i = 9.0 km s-1), this system will make an interesting target for future observations to measure the Rossiter-McLaughlin effect and determine its spin-orbit alignment. We detail the low-/medium-resolution reconnaissance spectroscopy that we are now using to deal with large numbers of transiting planet candidates produced by the HATSouth survey. We show that this important step in discovering planets produces log g and T eff parameters at a precision suitable for efficient candidate vetting, as well as efficiently identifying stellar mass eclipsing binaries with radial velocity semi-amplitudes as low as 1 km s-1.",

keywords = "planetary systems, stars: individual (HATS-3, GSC 6926?00454), techniques: photometric, techniques: spectroscopic",

author = "D. Bayliss and G. Zhou and K. Penev and Bakos, \{G. {\'A}\} and Hartman, \{J. D.\} and A. Jord{\'a}n and L. Mancini and M. Mohler-Fischer and V. Suc and M. Rabus and B. B{\'e}ky and Z. Csubry and L. Buchhave and T. Henning and N. Nikolov and B. Cs{\'a}k and R. Brahm and N. Espinoza and Noyes, \{R. W.\} and B. Schmidt and P. Conroy and Wright, \{D. J.\} and Tinney, \{C. G.\} and Addison, \{B. C.\} and Sackett, \{P. D.\} and Sasselov, \{D. D.\} and J. L{\'a}z{\'a}r and I. Papp and P. S{\'a}ri",

year = "2013",

month = nov,

doi = "10.1088/0004-6256/146/5/113",

language = "English",

volume = "146",

journal = "Astronomical Journal",

issn = "0004-6256",

publisher = "American Astronomical Society",

number = "5",

}

Bayliss, D, Zhou, G, Penev, K, Bakos, GÁ, Hartman, JD, Jordán, A, Mancini, L, Mohler-Fischer, M, Suc, V, Rabus, M, Béky, B, Csubry, Z, Buchhave, L, Henning, T, Nikolov, N, Csák, B, Brahm, R, Espinoza, N, Noyes, RW, Schmidt, B, Conroy, P, Wright, DJ, Tinney, CG, Addison, BC, Sackett, PD, Sasselov, DD, Lázár, J, Papp, I & Sári, P 2013, 'Hats-3b: An inflated hot jupiter transiting an F-type star*', Astronomical Journal, vol. 146, n.º 5, 113. https://doi.org/10.1088/0004-6256/146/5/113

TY - JOUR

T1 - Hats-3b

T2 - An inflated hot jupiter transiting an F-type star*

AU - Bayliss, D.

AU - Zhou, G.

AU - Penev, K.

AU - Bakos, G. Á

AU - Hartman, J. D.

AU - Jordán, A.

AU - Mancini, L.

AU - Mohler-Fischer, M.

AU - Suc, V.

AU - Rabus, M.

AU - Béky, B.

AU - Csubry, Z.

AU - Buchhave, L.

AU - Henning, T.

AU - Nikolov, N.

AU - Csák, B.

AU - Brahm, R.

AU - Espinoza, N.

AU - Noyes, R. W.

AU - Schmidt, B.

AU - Conroy, P.

AU - Wright, D. J.

AU - Tinney, C. G.

AU - Addison, B. C.

AU - Sackett, P. D.

AU - Sasselov, D. D.

AU - Lázár, J.

AU - Papp, I.

AU - Sári, P.

PY - 2013/11

Y1 - 2013/11

N2 - We report the discovery by the HATSouth survey of HATS-3b, a transiting extrasolar planet orbiting a V = 12.4 F dwarf star. HATS-3b has a period of P = 3.5479 days, mass of Mp = 1.07 M J, and radius of R p = 1.38 R J. Given the radius of the planet, the brightness of the host star, and the stellar rotational velocity (vsin i = 9.0 km s-1), this system will make an interesting target for future observations to measure the Rossiter-McLaughlin effect and determine its spin-orbit alignment. We detail the low-/medium-resolution reconnaissance spectroscopy that we are now using to deal with large numbers of transiting planet candidates produced by the HATSouth survey. We show that this important step in discovering planets produces log g and T eff parameters at a precision suitable for efficient candidate vetting, as well as efficiently identifying stellar mass eclipsing binaries with radial velocity semi-amplitudes as low as 1 km s-1.

AB - We report the discovery by the HATSouth survey of HATS-3b, a transiting extrasolar planet orbiting a V = 12.4 F dwarf star. HATS-3b has a period of P = 3.5479 days, mass of Mp = 1.07 M J, and radius of R p = 1.38 R J. Given the radius of the planet, the brightness of the host star, and the stellar rotational velocity (vsin i = 9.0 km s-1), this system will make an interesting target for future observations to measure the Rossiter-McLaughlin effect and determine its spin-orbit alignment. We detail the low-/medium-resolution reconnaissance spectroscopy that we are now using to deal with large numbers of transiting planet candidates produced by the HATSouth survey. We show that this important step in discovering planets produces log g and T eff parameters at a precision suitable for efficient candidate vetting, as well as efficiently identifying stellar mass eclipsing binaries with radial velocity semi-amplitudes as low as 1 km s-1.

KW - planetary systems

KW - stars: individual (HATS-3, GSC 6926?00454)

KW - techniques: photometric

KW - techniques: spectroscopic

UR - https://www.scopus.com/pages/publications/84886915019

U2 - 10.1088/0004-6256/146/5/113

DO - 10.1088/0004-6256/146/5/113

M3 - Article

AN - SCOPUS:84886915019

SN - 0004-6256

VL - 146

JO - Astronomical Journal

JF - Astronomical Journal

IS - 5

M1 - 113

ER -

Hats-3b: An inflated hot jupiter transiting an F-type star*

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