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

Authors :
Béky, Bence
Bakos, Gáspár Á.
Hartman, Joel
Torres, Guillermo
Latham, David W.
Jordán, Andres
Arriagada, Pamela
Bayliss, Daniel
Kiss, László L.
Kovács, Géza
Quinn, Sam N.
Marcy, Geoffrey W.
Howard, Andrew W.
Fischer, Debra A.
Johnson, John A.
Esquerdo, Gilbert A.
Noyes, Robert W.
Buchhave, Lars A.
Sasselov, Dimitar D.
Stefanik, Robert P.
Perumpilly, Gopakumar
Lázár, József
Papp, István
Sári, Pál
Source :
B\'eky, B., et al. 2011, ApJ, 734, 109
Publication Year :
2011

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 d, the reference epoch of transit is 2455186.01879 +/- 0.00054 (BJD), and the transit duration is 0.0705 +/- 0.0019 d. 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 Msun and radius is 0.90 +/- 0.04 Rsun. For the planetary companion we determine a mass of 0.660 +/- 0.033 MJ and radius of 1.038 +0.077 -0.058 RJ. For the 30 known transiting exoplanets between 0.3 MJ and 0.8 MJ, 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.<br />Comment: Submitted to ApJ on 2011-01-18. 12 pages, 7 figures, 7 tables

Details

Database :
arXiv
Journal :
B\'eky, B., et al. 2011, ApJ, 734, 109
Publication Type :
Report
Accession number :
edsarx.1101.3511
Document Type :
Working Paper
Full Text :
https://doi.org/10.1088/0004-637X/734/2/109