WASP-90 , the SIMBAD biblio

WASP-90 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST11:33:25

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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...585A.126W viz 356   K       X C       8 18 84 Three irradiated and bloated hot Jupiters: WASP-76b, WASP-82b, and
WASP-90b. 		WEST R.G., HELLIER C., ALMENARA J.-M., et al.
2016A&A...589A..58E viz 94       D     X         3 85 36 High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP). I. Lucky imaging observations of 101 systems in the southern hemisphere. EVANS D.F., SOUTHWORTH J., MAXTED P.F.L., 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.
2018MNRAS.474.5158G viz 16       D               1 131 85 A library of ATMO forward model transmission spectra for hot Jupiter exoplanets. GOYAL J.M., MAYNE N., SING D.K., 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.
2018A&A...620A..58S viz 16       D               1 164 10 SWEET-Cat updated. New homogenous spectroscopic parameters. SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., 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.
2020AJ....159..194V viz 16       D               1 288 ~ A statistical search for star-planet interaction in the ultraviolet using GALEX. VISWANATH G., NARANG M., MANOJ P., et al.
2020MNRAS.498.4680G viz 16       D               1 92 29 A library of self-consistent simulated exoplanet atmospheres. GOYAL J.M., MAYNE N., DRUMMOND B., 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.
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 108       D     X         3 182 ~ 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.
2024ApJS..274...20P 18       D               1 223 ~ Statistics and Habitability of F-type Star-Planet Systems. PATEL S.D., CUNTZ M. and WEINBERG N.N.
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.
2025A&A...699A.100D viz 19       D               1 2580 ~ The Gaia spectroscopic catalogue of exoplanets and host stars. DE LAVERNY P., LIGI R., CRIDA A., et al.
2025ApJ...990..113M 19       D               1 274 ~ OWLS. I. The Olin Wilson Legacy Survey. MORRIS B.M., HEBB L., HAWLEY S.L., 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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