HATS-45 , the SIMBAD biblio

HATS-45 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST12:15:31


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Title First 3 Authors
2018AJ....155..112B viz 1169   K   D     X C       28 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 17       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 17       D               1 4935 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.
2021ApJ...909..115C viz 17       D               1 2175 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.
2021AJ....162..192Z viz 17       D               1 713 29 SOAR TESS survey. II. The impact of stellar companions on planetary populations. ZIEGLER C., TOKOVININ A., LATIOLAIS M., 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.
2021ApJS..257...53L 45           X         1 7 8 TESS Data for Asteroseismology: light-curve systematics correction. LUND M.N., HANDBERG R., BUZASI D.L., et al.
2022ApJS..259...62I viz 18       D               1 395 24 TESS Transit Timing of Hundreds of Hot Jupiters. IVSHINA E.S. and WINN J.N.
2022A&A...663A.161M viz 18       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.

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