HATS-46 , the SIMBAD biblio

HATS-46 , the SIMBAD biblio (16 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST16:36:14

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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
2018AJ....155..112B viz 1019   K   D     X C       25 26 5 HATS-43b, HATS-44b, HATS-45b, and
HATS-46b: four short-period transiting giant planets in the Neptune-Jupiter mass range. 		BRAHM R., HARTMAN J.D., JORDAN 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.
2019AJ....158..243P viz 16       D               1 160 18 A search for multiplanet systems with TESS using a Bayesian N-body retrieval and machine learning. PEARSON K.A.
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.
2021MNRAS.501.5393L 2048   K A D S   X C F     47 5 ~ HATS-34b and
HATS-46b: re-characterization using TESS and Gaia. 		LOUDEN E.M. and HARTMAN J.D.
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...912..123J viz 17       D               1 757 22 Temperature and distance dependence of tidal circularization in close binaries: a catalog of eclipsing binaries in the southern hemisphere observed by the TESS satellite. JUSTESEN A.B. and ALBRECHT S.
2021ApJ...921...24S viz 17       D               2 328 1 The occurrence-weighted median planets discovered by transit surveys orbiting solar-type stars and their implications for planet formation and evolution. SCHLAUFMAN K.C. and HALPERN N.D.
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 60       D     X         2 354 20 Empirical Limb-darkening Coefficients and Transit Parameters of Known Exoplanets from TESS. PATEL J.A. and ESPINOZA N.
2023MNRAS.521.5636A viz 322       D     X C F     6 10 ~ LRG-BEASTS: evidence for clouds in the transmission spectrum of HATS-46 b. AHRER E., WHEATLEY P.J., GANDHI S., 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.
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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