WASP-133 , the SIMBAD biblio

WASP-133 , the SIMBAD biblio (18 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST21:03:51

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2016A&A...591A..55M viz 300     A     X         8 13 27 Five transiting hot Jupiters discovered using WASP-South, Euler, and TRAPPIST: WASP-119 b, WASP-124 b, WASP-126 b, WASP-129 b, and
WASP-133 b. 		MAXTED P.F.L., ANDERSON D.R., COLLIER CAMERON A., et al.
2017A&A...603A..30S viz 16       D               2 2500 58 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al.
2018A&A...610A..20E viz 161           X         4 115 9 High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP). II. Lucky Imaging results from 2015 and 2016. EVANS D.F., SOUTHWORTH J., SMALLEY B., et al.
2018AJ....155..165P viz 16       D               1 83 54 Empirical tidal dissipation in exoplanet hosts from tidal spin-up. PENEV K., BOUMA L.G., WINN J.N., et al.
2018ApJS..239...14J viz 16       D               1 1561 6 Revised exoplanet radii and habitability using Gaia data release 2. JOHNS D., MARTI C., HUFF M., et al.
2019AJ....158..190H viz 16       D               1 343 61 Hot Jupiters are destroyed by tides while their host stars are on the main sequence. HAMER J.H. and SCHLAUFMAN K.C.
2020ApJ...890...23L viz 16       D               1 4936 35 Current population statistics do not favor photoevaporation over core-powered mass loss as the dominant cause of the exoplanet radius gap. LOYD R.O.P., SHKOLNIK E.L., SCHNEIDER A.C., et al.
2021A&A...645A...7K viz 17       D               1 1569 17 Determining the true mass of radial-velocity exoplanets with Gaia. Nine planet candidates in the brown dwarf or stellar regime and 27 confirmed planets. KIEFER F., HEBRARD G., LECAVELIER DES ETANGS A., et al.
2021ApJ...909..115C viz 17       D               1 2176 13 Planets Across Space and Time (PAST). I. Characterizing the memberships of Galactic components and stellar ages: revisiting the kinematic methods and applying to planet host stars. CHEN D.-C., XIE J.-W., ZHOU J.-L., et al.
2021ApJ...919..138T viz 17       D               1 531 12 Further evidence for tidal spin-up of hot Jupiter host stars. TEJADA AREVALO R.A., WINN J.N. and ANDERSON K.R.
2022ApJS..259...62I viz 17       D               1 395 24 TESS Transit Timing of Hundreds of Hot Jupiters. IVSHINA E.S. and WINN J.N.
2022A&A...663A...4S viz 17       D               1 14206 7 Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. SOUBIRAN C., BROUILLET N. and CASAMIQUELA L.
2022A&A...663A.161M viz 17       D               1 213 8 Ariel stellar characterisation. I. Homogeneous stellar parameters of 187 FGK planet host stars: Description and validation of the method. MAGRINI L., DANIELSKI C., BOSSINI D., et al.
2024MNRAS.532.4752D 45           X         1 130 ~ The SHERLOCK pipeline: new exoplanet candidates in the WASP-16, HAT-P-27, HAT-P-26, and TOI-2411 systems. DEVORA-PAJARES M., POZUELOS F.J., THUILLIER A., et al.
2024A&A...688A.193D viz 18       D               1 182 ~ Ariel stellar characterisation II. Chemical abundances of carbon, nitrogen, and oxygen for 181 planet-host FGK dwarf stars. DA SILVA R., DANIELSKI C., DELGADO MENA E., et al.
2024MNRAS.534..843G 18       D               1 182 ~ Do anomalously dense hot Jupiters orbit stealth binary stars? GOSWAMY T., COLLIER CAMERON A. and WILSON T.G.
2024A&A...691A..53S viz 18       D               1 4078 ~ SWEET-Cat: A view on the planetary mass-radius relation. SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., et al.
2026AJ....171..157S 20       D               2 480 ~ Most Hot Jupiters Were Cool Giant Planets for More Than 1 Gyr. SCHMIDT S.P. and SCHLAUFMAN K.C.

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