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

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

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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{6ba056a344304a5c9f30f752339c8632,

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 (US)",

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journal = "Astrophysical Journal",

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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 - http://www.scopus.com/inward/record.url?scp=79958280813&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=79958280813&partnerID=8YFLogxK

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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