HAT-P-65 , the SIMBAD biblio

HAT-P-65 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST09:39:17

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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
2016AJ....152..182H viz 2612   K   D     X C       66 205 26
HAT-P-65b and HAT-P-66b: two transiting inflated hot Jupiters and observational evidence for the reinflation of close-in giant planets. 		HARTMAN J.D., BAKOS G.A., BHATTI W., 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.
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.
2019MNRAS.486.3963A 81           X         2 3 ~ Orbital decay of short-period gas giants under evolving tides. ALVARADO-MONTES J.A. and GARCIA-CARMONA C.
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               2 288 ~ 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.
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...913L..16C 460           X C       10 6 ~ Evidence for TiO in the atmosphere of the hot Jupiter HAT-P-65 b. CHEN G., PALLE E., PARVIAINEN H., et al.
2021A&A...653A.147M 42           X         1 16 4 TOI-1296b and TOI-1298b observed with TESS and SOPHIE: two hot Saturn-mass exoplanets with different densities around metal-rich stars. MOUTOU C., ALMENARA J.M., HEBRARD G., 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.
2022MNRAS.509.1447M viz 85               F     1 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.
2023A&A...672A..78M 87           X         2 15 ~ Pathways of survival for exomoons and inner exoplanets. MAKAROV V.V. and EFROIMSKY M.
2024MNRAS.528.1930K viz 779       D     X C       17 10 ~ Simultaneous multicolour transit photometry of hot Jupiters HAT-P-19b, HAT-P-51b, HAT-P-55b, and HAT-P-65b. KANG H., CHEN G., PALLE E., 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...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...697A.102T viz 65       D     X         2 176 ~ Ariel stellar characterisation III. Fast rotators and new FGK stars in the Ariel mission candidate sample. TSANTAKI M., MAGRINI L., DANIELSKI C., 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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