TY - JOUR
T1 - HATS-5b
T2 - A transiting hot saturn from the HATsouth survey
AU - Zhou, G.
AU - Bayliss, D.
AU - Penev, K.
AU - Bakos, G. Á
AU - Hartman, J. D.
AU - Jordán, A.
AU - Mancini, L.
AU - Mohler, M.
AU - Csubry, Z.
AU - Ciceri, S.
AU - Brahm, R.
AU - Rabus, M.
AU - Buchhave, L.
AU - Henning, T.
AU - Suc, V.
AU - Espinoza, N.
AU - Béky, B.
AU - Noyes, R. W.
AU - Schmidt, B.
AU - Butler, R. P.
AU - Shectman, S.
AU - Thompson, I.
AU - Crane, J.
AU - Sato, B.
AU - Csák, B.
AU - Lázár, J.
AU - Papp, I.
AU - Sári, P.
AU - Nikolov, N.
PY - 2014/6
Y1 - 2014/6
N2 - We report the discovery of HATS-5b, a transiting hot Saturn orbiting a G-type star, by the HATSouth survey. HATS-5b has a mass of Mp 0.24 MJ, radius of Rp 0.91 R J, and transits its host star with a period of P 4.7634 days. The radius of HATS-5b is consistent with both theoretical and empirical models. The host star has a V-band magnitude of 12.6, mass of 0.94 M ⊙, and radius of 0.87 R. The relatively high scale height of HATS-5b and the bright, photometrically quiet host star make this planet a favorable target for future transmission spectroscopy follow-up observations. We reexamine the correlations in radius, equilibrium temperature, and metallicity of the close-in gas giants and find hot Jupiter-mass planets to exhibit the strongest dependence between radius and equilibrium temperature. We find no significant dependence in radius and metallicity for the close-in gas giant population.
AB - We report the discovery of HATS-5b, a transiting hot Saturn orbiting a G-type star, by the HATSouth survey. HATS-5b has a mass of Mp 0.24 MJ, radius of Rp 0.91 R J, and transits its host star with a period of P 4.7634 days. The radius of HATS-5b is consistent with both theoretical and empirical models. The host star has a V-band magnitude of 12.6, mass of 0.94 M ⊙, and radius of 0.87 R. The relatively high scale height of HATS-5b and the bright, photometrically quiet host star make this planet a favorable target for future transmission spectroscopy follow-up observations. We reexamine the correlations in radius, equilibrium temperature, and metallicity of the close-in gas giants and find hot Jupiter-mass planets to exhibit the strongest dependence between radius and equilibrium temperature. We find no significant dependence in radius and metallicity for the close-in gas giant population.
KW - stars: individual (HATS-5, GSC 5897-00933)
KW - techniques: photometric
KW - techniques: spectroscopic
UR - https://www.scopus.com/pages/publications/84900815765
U2 - 10.1088/0004-6256/147/6/144
DO - 10.1088/0004-6256/147/6/144
M3 - Article
AN - SCOPUS:84900815765
SN - 0004-6256
VL - 147
JO - Astronomical Journal
JF - Astronomical Journal
IS - 6
M1 - 144
ER -