HATS-41 , the SIMBAD biblio

HATS-41 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST14:16:12

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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
2018MNRAS.477.3406B viz 1501   K   D     X C       37 11 4 HATS-39b, HATS-40b,
HATS-41b, and HATS-42b: three inflated hot Jupiters and a super-Jupiter transiting F stars. 		BENTO J., HARTMAN J.D., BAKOS G.A., 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.
2020MNRAS.496.4442C 41           X         1 33 26 The Transit and Light Curve Modeller. CSIZMADIA S.
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.
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.
2021AJ....162..263H viz 17       D               1 346 17 A uniform search for nearby planetary companions to hot Jupiters in TESS data reveals hot Jupiters are still lonely. HORD B.J., COLON K.D., KOSTOV V., et al.
2022MNRAS.512L..60H viz 17       D               1 1974 9 The flaring TESS Objects of Interest: flare rates for all two-minute cadence TESS planet candidates. HOWARD W.S.
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....163..228P viz 17       D               1 354 20 Empirical Limb-darkening Coefficients and Transit Parameters of Known Exoplanets from TESS. PATEL J.A. and ESPINOZA N.
2022MNRAS.513..102C viz 17       D               1 961 6 The TESS Triple-9 Catalog: 999 uniformly vetted exoplanet candidates. CACCIAPUOTI L., KOSTOV V.B., KUCHNER M., et al.
2022A&A...663A.161M viz 85           X         2 213 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.529.2893G 358           X C F     6 9 ~ Long-term double synchronization in close-in gas giant planets. GUO S., GUO J., SU J., et al.
2024AJ....167..203M viz 152       D     X         4 805 ~ DIAmante TESS AutoRegressive Planet Search (DTARPS). II. Hundreds of New TESS Candidate Exoplanets. MELTON E.J., FEIGELSON E.D., MONTALTO M., 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.535.1778E 18       D               1 139 ~ Viewing the PLATO LOPS2 field through the lenses of TESS. ESCHEN Y.N.E., BAYLISS D., WILSON T.G., 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 19       D               1 176 ~ Ariel stellar characterisation III. Fast rotators and new FGK stars in the Ariel mission candidate sample. TSANTAKI M., MAGRINI L., DANIELSKI C., et al.
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.
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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