HAT-P-51 , the SIMBAD biblio

HAT-P-51 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST13:05:31


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Title First 3 Authors
2015AJ....150..168H viz 1404   K A D     X C       36 12 9 HAT-P-50b,
HAT-P-51b, HAT-P-52b, and HAT-P-53b: three transiting hot Jupiters and a transiting hot Saturn from the HATNet survey.
HARTMAN J.D., BHATTI W., BAKOS G.A., et al.
2017A&A...602A.107B viz 16       D               2 476 185 The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets. BONOMO A.S., DESIDERA S., BENATTI S., 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.
2018ApJ...856..155G viz 96       D       C       7 149 5 Giant planets: good neighbors for habitable worlds? GEORGAKARAKOS N., EGGL S. and DOBBS-DIXON I.
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.
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.
2020AJ....159..194V viz 16       D               1 288 ~ A statistical search for star-planet interaction in the ultraviolet using GALEX. VISWANATH G., NARANG M., MANOJ P., 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...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.
2021RAA....21...44K 585   K A D S   X C       13 8 ~ New observations and transit solutions of the inflated exoplanets HAT-P-40b and
HAT-P-51b.
KJURKCHIEVA D.P., PETROV N.I. and POPOV V.A.
2022ApJS..259...33K viz 17       D               1 3171 19 The TESS Faint-star Search: 1617 TOIs from the TESS Primary Mission. KUNIMOTO M., DAYLAN T., GUERRERO N., 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.
2022ApJS..261...26S viz 17       D               2 1893 2 Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys. SU T., ZHANG L.-Y., LONG L., et al.
2024MNRAS.528.1930K viz 690       D     X C       15 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.
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.
2025ApJS..277...15J 19       D               4 136 ~ Half a Million Binary Stars Identified from the Low-resolution Spectra of LAMOST. JING Y., MAO T.-X., WANG J., 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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