SIMBAD references

2020AJ....159..255C - Astron. J., 159, 255-255 (2020/June-0)

Two transiting hot Jupiters from the WASP survey: WASP-150b and WASP-176b.

COOKE B.F., POLLACCO D., ALMLEAKY Y., BARKAOUI K., BENKHALDOUN Z., BLAKE J.A., BOUCHY F., BOUMIS P., BROWN D.J.A., BRUNI I., BURDANOV A., CAMERON A.C., CHOTE P., DAASSOU A., D'AGO G., DALAL S., DAMASSO M., DELREZ L., DOYLE A.P., DUCROT E., GILLON M., HEBRARD G., HELLIER C., HENNING T., JEHIN E., KIEFER F., KING G.W., LIAKOS A., LOPEZ T., MANCINI L., MARDLING R., MAXTED P.F.L., McCORMAC J., MURRAY C., NIELSEN L.D., OSBORN H., PALLE E., PEPE F., POZUELOS F.J., PRIETO-ARRANZ J., QUELOZ D., SCHANCHE N., SEGRANSAN D., SMALLEY B., SOUTHWORTH J., THOMPSON S., TURNER O., UDRY S., VELASCO S., WEST R., WHEATLEY P. and ALIKAKOS J.

Abstract (from CDS):

We report the discovery of two transiting exoplanets from the WASP survey, WASP-150b and WASP-176b. WASP-150b is an eccentric (e = 0.38) hot Jupiter on a 5.6 day orbit around a V = 12.03, F8 main-sequence host. The host star has a mass and radius of 1.4 M_☉ and 1.7 R_☉ respectively. WASP-150b has a mass and radius of 8.5 M_J and 1.1 R_J, leading to a large planetary bulk density of 6.4 ρ_J. WASP-150b is found to be ∼3 Gyr old, well below its circularization timescale, supporting the eccentric nature of the planet. WASP-176b is a hot Jupiter planet on a 3.9 day orbit around a V = 12.01, F9 sub-giant host. The host star has a mass and radius of 1.3 M_☉ and 1.9 R_☉. WASP-176b has a mass and radius of 0.86 M_J and 1.5 R_J, respectively, leading to a planetary bulk density of 0.23 ρ_J.

Journal keyword(s): Exoplanet systems - Radial velocity - Exoplanet detection methods - Photometry

VizieR on-line data: <Available at CDS (J/AJ/159/255): table2.dat table3.dat fig1-3.dat fig5.dat fig7a-g.dat fig9a-g.dat>

Simbad objects: 12

Full paper

View the references in ADS

To bookmark this query, right click on this link: simbad:2020AJ....159..255C and select 'bookmark this link' or equivalent in the popup menu