WASP-114 , the SIMBAD biblio

WASP-114 , the SIMBAD biblio (24 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST07:55:17


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Title First 3 Authors
2016A&A...593A.113B 1755   K A S   X C       43 4 5 WASP-113b and
WASP-114b, two inflated hot Jupiters with contrasting densities.
BARROS S.C.C., BROWN D.J.A., HEBRARD G., 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.
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..237...38B viz 16       D               1 1111 42 Spectral properties of cool stars: extended abundance analysis of Kepler Objects of Interest. BREWER J.M. and FISCHER D.A.
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.
2019MNRAS.490.5088M viz 16       D               2 214 32 Search for stellar companions of exoplanet host stars by exploring the second ESA-Gaia data release. MUGRAUER M.
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..150P viz 166     A D     X         5 33 51 The continuing search for evidence of tidal orbital decay of hot Jupiters. PATRA K.C., WINN J.N., HOLMAN M.J., et al.
2020MNRAS.497.3911L 16       D               1 18 ~ Orbital period modulation in hot Jupiter systems. LANZA A.F.
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...914...56A 59       D     X         2 55 13 On a possible solution to the tidal realignment problem for hot Jupiters. ANDERSON K.R., WINN J.N. and PENEV K.
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.
2022MNRAS.509.1447M viz 85               F     2 48 5 The ultra-hot-Jupiter KELT-16 b: dynamical evolution and atmospheric properties. MANCINI L., SOUTHWORTH J., NAPONIELLO 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.
2022AJ....164...60S viz 17       D               1 854 2 Galactic Chemical Evolution of Exoplanet Hosting Stars: Are High-mass Planetary Systems Young? SWASTIK C., BANYAL R.K., NARANG M., et al.
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.
2024ApJ...960...50W 18       D               1 46 ~ Orbital Decay of Hot Jupiters due to Weakly Nonlinear Tidal Dissipation. WEINBERG N.N., DAVACHI N., ESSICK R., 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.
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...993...78S 205       D     X         5 63 ~ In Search of Decay: An Analysis of Transit Times of Hot Jupiters in Main-sequence and Post-main-sequence Systems. SODICKSON N. and GRUNBLATT S.
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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