HAT-P-27b: A hot jupiter transiting a G star on A 3 day orbit

B. Béky; G. Á Bakos; J. Hartman; G. Torres; D. W. Latham; A. Jordán; P. Arriagada; D. Bayliss; L. L. Kiss; Géza Kovács; S. N. Quinn; G. W. Marcy; A. W. Howard; D. A. Fischer; J. A. Johnson; G. A. Esquerdo; R. W. Noyes; L. A. Buchhave; D. D. Sasselov; R. P. Stefanik; G. Perumpilly; J. Lázár; I. Papp; P. Sári

doi:10.1088/0004-637X/734/2/109

HAT-P-27b: A hot jupiter transiting a G star on A 3 day orbit

B. Béky
, G. Á Bakos
, J. Hartman
, G. Torres
, D. W. Latham
, A. Jordán
, P. Arriagada
, D. Bayliss
, L. L. Kiss
, Géza Kovács
, S. N. Quinn
, G. W. Marcy
, A. W. Howard
, D. A. Fischer
, J. A. Johnson
, G. A. Esquerdo
, R. W. Noyes
, L. A. Buchhave
, D. D. Sasselov
, R. P. Stefanik

G. Perumpilly, J. Lázár, I. Papp, P. Sári

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

39 Scopus citations

Abstract

We report the discovery of HAT-P-27b, an exoplanet transiting the moderately bright G8 dwarf star GSC 0333-00351 (V = 12.214). The orbital period is 3.039586 ± 0.000012 days, the reference epoch of transit is 2455186.01879 ± 0.00054 (BJD), and the transit duration is 0.0705 ± 0.0019 days. The host star with its effective temperature 5300 ± 90 K is somewhat cooler than the Sun and is more metal-rich with a metallicity of +0.29 ± 0.10. Its mass is 0.94 ± 0.04 M_⊙ and radius is 0.90^+0.05 _{- 0.04} R_⊙. For the planetary companion we determine a mass of 0.660 ± 0.033 M _J and radius of 1.038^+0.077 _{- 0.058} R _J. For the 30 known transiting exoplanets between 0.3 M _J and 0.8 M _J, a negative correlation between host star metallicity and planetary radius and an additional dependence of planetary radius on equilibrium temperature are confirmed at a high level of statistical significance.

Original language	English
Article number	109
Journal	Astrophysical Journal
Volume	734
Issue number	2
DOIs	https://doi.org/10.1088/0004-637X/734/2/109
State	Published - 10 Jun 2011
Externally published	Yes

Keywords

planetary systems
stars: individual (HAT-P-27, GSC 0333-00351)
techniques: photometric
techniques: spectroscopic

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10.1088/0004-637X/734/2/109

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Béky, B., Bakos, G. Á., Hartman, J., Torres, G., Latham, D. W., Jordán, A., Arriagada, P., Bayliss, D., Kiss, L. L., Kovács, G., Quinn, S. N., Marcy, G. W., Howard, A. W., Fischer, D. A., Johnson, J. A., Esquerdo, G. A., Noyes, R. W., Buchhave, L. A., Sasselov, D. D., ... Sári, P. (2011). HAT-P-27b: A hot jupiter transiting a G star on A 3 day orbit. Astrophysical Journal, 734(2), Article 109. https://doi.org/10.1088/0004-637X/734/2/109

@article{cdaf0b784cab40cba23b397ec467a0bf,

title = "HAT-P-27b: A hot jupiter transiting a G star on A 3 day orbit",

abstract = "We report the discovery of HAT-P-27b, an exoplanet transiting the moderately bright G8 dwarf star GSC 0333-00351 (V = 12.214). The orbital period is 3.039586 ± 0.000012 days, the reference epoch of transit is 2455186.01879 ± 0.00054 (BJD), and the transit duration is 0.0705 ± 0.0019 days. The host star with its effective temperature 5300 ± 90 K is somewhat cooler than the Sun and is more metal-rich with a metallicity of +0.29 ± 0.10. Its mass is 0.94 ± 0.04 M⊙ and radius is 0.90+0.05 - 0.04 R⊙. For the planetary companion we determine a mass of 0.660 ± 0.033 M J and radius of 1.038+0.077 - 0.058 R J. For the 30 known transiting exoplanets between 0.3 M J and 0.8 M J, a negative correlation between host star metallicity and planetary radius and an additional dependence of planetary radius on equilibrium temperature are confirmed at a high level of statistical significance.",

keywords = "planetary systems, stars: individual (HAT-P-27, GSC 0333-00351), techniques: photometric, techniques: spectroscopic",

author = "B. B{\'e}ky and Bakos, \{G. {\'A}\} and J. Hartman and G. Torres and Latham, \{D. W.\} and A. Jord{\'a}n and P. Arriagada and D. Bayliss and Kiss, \{L. L.\} and G{\'e}za Kov{\'a}cs and Quinn, \{S. N.\} and Marcy, \{G. W.\} and Howard, \{A. W.\} and Fischer, \{D. A.\} and Johnson, \{J. A.\} and Esquerdo, \{G. A.\} and Noyes, \{R. W.\} and Buchhave, \{L. A.\} and Sasselov, \{D. D.\} and Stefanik, \{R. P.\} and G. Perumpilly and J. L{\'a}z{\'a}r and I. Papp and P. S{\'a}ri",

year = "2011",

month = jun,

day = "10",

doi = "10.1088/0004-637X/734/2/109",

language = "English",

volume = "734",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "2",

}

Béky, B, Bakos, GÁ, Hartman, J, Torres, G, Latham, DW, Jordán, A, Arriagada, P, Bayliss, D, Kiss, LL, Kovács, G, Quinn, SN, Marcy, GW, Howard, AW, Fischer, DA, Johnson, JA, Esquerdo, GA, Noyes, RW, Buchhave, LA, Sasselov, DD, Stefanik, RP, Perumpilly, G, Lázár, J, Papp, I & Sári, P 2011, 'HAT-P-27b: A hot jupiter transiting a G star on A 3 day orbit', Astrophysical Journal, vol. 734, no. 2, 109. https://doi.org/10.1088/0004-637X/734/2/109

TY - JOUR

T1 - HAT-P-27b

T2 - A hot jupiter transiting a G star on A 3 day orbit

AU - Béky, B.

AU - Bakos, G. Á

AU - Hartman, J.

AU - Torres, G.

AU - Latham, D. W.

AU - Jordán, A.

AU - Arriagada, P.

AU - Bayliss, D.

AU - Kiss, L. L.

AU - Kovács, Géza

AU - Quinn, S. N.

AU - Marcy, G. W.

AU - Howard, A. W.

AU - Fischer, D. A.

AU - Johnson, J. A.

AU - Esquerdo, G. A.

AU - Noyes, R. W.

AU - Buchhave, L. A.

AU - Sasselov, D. D.

AU - Stefanik, R. P.

AU - Perumpilly, G.

AU - Lázár, J.

AU - Papp, I.

AU - Sári, P.

PY - 2011/6/10

Y1 - 2011/6/10

N2 - We report the discovery of HAT-P-27b, an exoplanet transiting the moderately bright G8 dwarf star GSC 0333-00351 (V = 12.214). The orbital period is 3.039586 ± 0.000012 days, the reference epoch of transit is 2455186.01879 ± 0.00054 (BJD), and the transit duration is 0.0705 ± 0.0019 days. The host star with its effective temperature 5300 ± 90 K is somewhat cooler than the Sun and is more metal-rich with a metallicity of +0.29 ± 0.10. Its mass is 0.94 ± 0.04 M⊙ and radius is 0.90+0.05 - 0.04 R⊙. For the planetary companion we determine a mass of 0.660 ± 0.033 M J and radius of 1.038+0.077 - 0.058 R J. For the 30 known transiting exoplanets between 0.3 M J and 0.8 M J, a negative correlation between host star metallicity and planetary radius and an additional dependence of planetary radius on equilibrium temperature are confirmed at a high level of statistical significance.

AB - We report the discovery of HAT-P-27b, an exoplanet transiting the moderately bright G8 dwarf star GSC 0333-00351 (V = 12.214). The orbital period is 3.039586 ± 0.000012 days, the reference epoch of transit is 2455186.01879 ± 0.00054 (BJD), and the transit duration is 0.0705 ± 0.0019 days. The host star with its effective temperature 5300 ± 90 K is somewhat cooler than the Sun and is more metal-rich with a metallicity of +0.29 ± 0.10. Its mass is 0.94 ± 0.04 M⊙ and radius is 0.90+0.05 - 0.04 R⊙. For the planetary companion we determine a mass of 0.660 ± 0.033 M J and radius of 1.038+0.077 - 0.058 R J. For the 30 known transiting exoplanets between 0.3 M J and 0.8 M J, a negative correlation between host star metallicity and planetary radius and an additional dependence of planetary radius on equilibrium temperature are confirmed at a high level of statistical significance.

KW - planetary systems

KW - stars: individual (HAT-P-27, GSC 0333-00351)

KW - techniques: photometric

KW - techniques: spectroscopic

UR - https://www.scopus.com/pages/publications/79958280813

U2 - 10.1088/0004-637X/734/2/109

DO - 10.1088/0004-637X/734/2/109

M3 - Article

AN - SCOPUS:79958280813

SN - 0004-637X

VL - 734

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

M1 - 109

ER -

HAT-P-27b: A hot jupiter transiting a G star on A 3 day orbit

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Keywords

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