TYC 6411-312-1 , the SIMBAD biblio

2019MNRAS.482..301L - Mon. Not. R. Astron. Soc., 482, 301-312 (2019/January-1)

WASP-147b, 160Bb, 164b, and 165b: two hot Saturns and two Jupiters, including two planets with metal-rich hosts.

LENDL M., ANDERSON D.R., BONFANTI A., BOUCHY F., BURDANOV A., CAMERON A.C., DELREZ L., GILLON M., HELLIER C., JEHIN E., MAXTED P.F.L., NIELSEN L.D., PEPE F., POLLACCO D., QUELOZ D., SEGRANSAN D., SOUTHWORTH J., SMALLEY B., THOMPSON S., TURNER O., TRIAUD A.H.M.J., UDRY S. and WEST R.G.

Abstract (from CDS):

We report the discovery of four transiting hot Jupiters, WASP-147, WASP-160B, WASP-164, and WASP-165 from the WASP survey. WASP-147b is a near Saturn-mass (M_P = 0.28M_J) object with a radius of 1.11 R_J orbiting a G4 star with a period of 4.6 d. WASP-160Bb has a mass and radius (M_p=_0.28_MJ_, R_p=_1.09_RJ_) near-identical to WASP-147b, but is less irradiated, orbiting a metal-rich ([Fe/H]_* = 0.27) K0 star with a period of 3.8 d. WASP-160B is part of a near equal-mass visual binary with an on-sky separation of 28.5 arcsec. WASP-164b is a more massive (M_P=_2.13_MJ_, R_p=_1.13_RJ_) hot Jupiter, orbiting a G2 star on a close-in (P = 1.8 d), but tidally stable orbit. WASP-165b is a classical (M_p=_0.66_MJ_, R_P=_1.26_RJ_) hot Jupiter in a 3.5 d period orbit around a metal-rich ([Fe/H]_* = 0.33) star. WASP-147b and WASP-160Bb are promising targets for atmospheric characterization through transmission spectroscopy, while WASP-164b presents a good target for emission spectroscopy.

Journal keyword(s): planets and satellites: detection - planetary systems

Simbad objects: 14

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