HATS-4b: A dense hot Jupiter transiting a super metal-rich G star

Andrés Jordán; Rafael Brahm; G. Á Bakos; D. Bayliss; K. Penev; J. D. Hartman; G. Zhou; L. Mancini; M. Mohler-Fischer; S. Ciceri; B. Sato; Z. Csubry; M. Rabus; V. Suc; N. Espinoza; W. Bhatti; M. De Val Borro; L. Buchhave; B. Csák; T. Henning; B. Schmidt; T. G. Tan; R. W. Noyes; B. Béky; R. P. Butler; S. Shectman; J. Crane; I. Thompson; A. Williams; R. Martin; C. Contreras; J. Lázár; I. Papp; P. Sári

doi:10.1088/0004-6256/148/2/29

HATS-4b: A dense hot Jupiter transiting a super metal-rich G star

Andrés Jordán, Rafael Brahm, G. Á Bakos, D. Bayliss, K. Penev, J. D. Hartman, G. Zhou, L. Mancini, M. Mohler-Fischer, S. Ciceri, B. Sato, Z. Csubry, M. Rabus, V. Suc, N. Espinoza, W. Bhatti, M. De Val Borro, L. Buchhave, B. Csák, T. HenningB. Schmidt, T. G. Tan, R. W. Noyes, B. Béky, R. P. Butler, S. Shectman, J. Crane, I. Thompson, A. Williams, R. Martin, C. Contreras, J. Lázár, I. Papp, P. Sári

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64 Citas (Scopus)

Resumen

We report the discovery by the HATSouth survey of HATS-4b, an extrasolar planet transiting a V = 13.46 mag G star. HATS-4b has a period of P ≈ 2.5167 days, mass of M_p ≈ 1.32 M_Jup, radius of R_p ≈ 1.02 R_Jup, and density of ρ_p = 1.55 ± 0.16 g cm^-3 ≈ 1.24 ρ_Jup. The host star has a mass of 1.00 M_⊙, a radius of 0.92 R_⊙, and a very high metallicity [Fe/H]=0.43 ± 0.08. HATS-4b is among the densest known planets with masses between 1 and 2 M_J and is thus likely to have a significant content of heavy elements of the order of 75 M_⊕. In this paper we present the data reduction, radial velocity measurements, and stellar classification techniques adopted by the HATSouth survey for the CORALIE spectrograph. We also detail a technique for simultaneously estimating vsin i and macroturbulence using high resolution spectra.

Idioma original	Inglés
Número de artículo	29
Publicación	Astronomical Journal
Volumen	148
N.º	2
DOI	https://doi.org/10.1088/0004-6256/148/2/29
Estado	Publicada - ago. 2014
Publicado de forma externa	Sí

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Jordán, A., Brahm, R., Bakos, G. Á., Bayliss, D., Penev, K., Hartman, J. D., Zhou, G., Mancini, L., Mohler-Fischer, M., Ciceri, S., Sato, B., Csubry, Z., Rabus, M., Suc, V., Espinoza, N., Bhatti, W., De Val Borro, M., Buchhave, L., Csák, B., ... Sári, P. (2014). HATS-4b: A dense hot Jupiter transiting a super metal-rich G star. Astronomical Journal, 148(2), Artículo 29. https://doi.org/10.1088/0004-6256/148/2/29

@article{2e4955b82f8943c58aefc49555c294dc,

title = "HATS-4b: A dense hot Jupiter transiting a super metal-rich G star",

abstract = "We report the discovery by the HATSouth survey of HATS-4b, an extrasolar planet transiting a V = 13.46 mag G star. HATS-4b has a period of P ≈ 2.5167 days, mass of Mp ≈ 1.32 MJup, radius of Rp ≈ 1.02 RJup, and density of ρp = 1.55 ± 0.16 g cm-3 ≈ 1.24 ρJup. The host star has a mass of 1.00 M⊙, a radius of 0.92 R⊙, and a very high metallicity [Fe/H]=0.43 ± 0.08. HATS-4b is among the densest known planets with masses between 1 and 2 MJ and is thus likely to have a significant content of heavy elements of the order of 75 M⊕. In this paper we present the data reduction, radial velocity measurements, and stellar classification techniques adopted by the HATSouth survey for the CORALIE spectrograph. We also detail a technique for simultaneously estimating vsin i and macroturbulence using high resolution spectra.",

keywords = "planetary systems, stars: individual (HATS-4, GSC 6505-00217), techniques: photometric, techniques: spectroscopic",

author = "Andr{\'e}s Jord{\'a}n and Rafael Brahm and Bakos, {G. {\'A}} and D. Bayliss and K. Penev and Hartman, {J. D.} and G. Zhou and L. Mancini and M. Mohler-Fischer and S. Ciceri and B. Sato and Z. Csubry and M. Rabus and V. Suc and N. Espinoza and W. Bhatti and {De Val Borro}, M. and L. Buchhave and B. Cs{\'a}k and T. Henning and B. Schmidt and Tan, {T. G.} and Noyes, {R. W.} and B. B{\'e}ky and Butler, {R. P.} and S. Shectman and J. Crane and I. Thompson and A. Williams and R. Martin and C. Contreras and J. L{\'a}z{\'a}r and I. Papp and P. S{\'a}ri",

year = "2014",

month = aug,

doi = "10.1088/0004-6256/148/2/29",

language = "English",

volume = "148",

journal = "Astronomical Journal",

issn = "0004-6256",

publisher = "American Astronomical Society",

number = "2",

}

Jordán, A , Brahm, R, Bakos, GÁ, Bayliss, D, Penev, K, Hartman, JD, Zhou, G, Mancini, L, Mohler-Fischer, M, Ciceri, S, Sato, B, Csubry, Z, Rabus, M, Suc, V, Espinoza, N, Bhatti, W, De Val Borro, M, Buchhave, L, Csák, B, Henning, T, Schmidt, B, Tan, TG, Noyes, RW, Béky, B, Butler, RP, Shectman, S, Crane, J, Thompson, I, Williams, A, Martin, R, Contreras, C, Lázár, J, Papp, I & Sári, P 2014, 'HATS-4b: A dense hot Jupiter transiting a super metal-rich G star', Astronomical Journal, vol. 148, n.º 2, 29. https://doi.org/10.1088/0004-6256/148/2/29

TY - JOUR

T1 - HATS-4b

T2 - A dense hot Jupiter transiting a super metal-rich G star

AU - Jordán, Andrés

AU - Brahm, Rafael

AU - Bakos, G. Á

AU - Bayliss, D.

AU - Penev, K.

AU - Hartman, J. D.

AU - Zhou, G.

AU - Mancini, L.

AU - Mohler-Fischer, M.

AU - Ciceri, S.

AU - Sato, B.

AU - Csubry, Z.

AU - Rabus, M.

AU - Suc, V.

AU - Espinoza, N.

AU - Bhatti, W.

AU - De Val Borro, M.

AU - Buchhave, L.

AU - Csák, B.

AU - Henning, T.

AU - Schmidt, B.

AU - Tan, T. G.

AU - Noyes, R. W.

AU - Béky, B.

AU - Butler, R. P.

AU - Shectman, S.

AU - Crane, J.

AU - Thompson, I.

AU - Williams, A.

AU - Martin, R.

AU - Contreras, C.

AU - Lázár, J.

AU - Papp, I.

AU - Sári, P.

PY - 2014/8

Y1 - 2014/8

N2 - We report the discovery by the HATSouth survey of HATS-4b, an extrasolar planet transiting a V = 13.46 mag G star. HATS-4b has a period of P ≈ 2.5167 days, mass of Mp ≈ 1.32 MJup, radius of Rp ≈ 1.02 RJup, and density of ρp = 1.55 ± 0.16 g cm-3 ≈ 1.24 ρJup. The host star has a mass of 1.00 M⊙, a radius of 0.92 R⊙, and a very high metallicity [Fe/H]=0.43 ± 0.08. HATS-4b is among the densest known planets with masses between 1 and 2 MJ and is thus likely to have a significant content of heavy elements of the order of 75 M⊕. In this paper we present the data reduction, radial velocity measurements, and stellar classification techniques adopted by the HATSouth survey for the CORALIE spectrograph. We also detail a technique for simultaneously estimating vsin i and macroturbulence using high resolution spectra.

AB - We report the discovery by the HATSouth survey of HATS-4b, an extrasolar planet transiting a V = 13.46 mag G star. HATS-4b has a period of P ≈ 2.5167 days, mass of Mp ≈ 1.32 MJup, radius of Rp ≈ 1.02 RJup, and density of ρp = 1.55 ± 0.16 g cm-3 ≈ 1.24 ρJup. The host star has a mass of 1.00 M⊙, a radius of 0.92 R⊙, and a very high metallicity [Fe/H]=0.43 ± 0.08. HATS-4b is among the densest known planets with masses between 1 and 2 MJ and is thus likely to have a significant content of heavy elements of the order of 75 M⊕. In this paper we present the data reduction, radial velocity measurements, and stellar classification techniques adopted by the HATSouth survey for the CORALIE spectrograph. We also detail a technique for simultaneously estimating vsin i and macroturbulence using high resolution spectra.

KW - planetary systems

KW - stars: individual (HATS-4, GSC 6505-00217)

KW - techniques: photometric

KW - techniques: spectroscopic

UR - http://www.scopus.com/inward/record.url?scp=84903991906&partnerID=8YFLogxK

U2 - 10.1088/0004-6256/148/2/29

DO - 10.1088/0004-6256/148/2/29

M3 - Article

AN - SCOPUS:84903991906

SN - 0004-6256

VL - 148

JO - Astronomical Journal

JF - Astronomical Journal

IS - 2

M1 - 29

ER -

HATS-4b: A dense hot Jupiter transiting a super metal-rich G star

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