SIMBAD references

2014AJ....147..144Z - Astron. J., 147, 144 (2014/June-0)

HATS-5b: a transiting hot Saturn from the HATSouth survey.

ZHOU G., BAYLISS D., PENEV K., BAKOS G.A., HARTMAN J.D., JORDAN A., MANCINI L., MOHLER M., CSUBRY Z., CICERI S., BRAHM R., RABUS M., BUCHHAVE L., HENNING T., SUC V., ESPINOZA N., BEKY B., NOYES R.W., SCHMIDT B., BUTLER R.P., SHECTMAN S., THOMPSON I., CRANE J., SATO B., CSAK B., LAZAR J., PAPP I., SARI P. and NIKOLOV N.

Abstract (from CDS):

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 M_p~ 0.24 M_J, radius of R_p~ 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.

Abstract Copyright: ∼

Journal keyword(s): stars: individual: (HATS-5, GSC 5897-00933) - techniques: photometric - techniques: spectroscopic

VizieR on-line data: <Available at CDS (J/AJ/147/144): table3.dat table4.dat>

Simbad objects: 3

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