HAT-P-37 , the SIMBAD biblio

HAT-P-37 , the SIMBAD biblio (31 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST15:03:26

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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
2012AJ....144...19B viz 1199       D S   X C       30 23 70 HAT-P-34b-HAT-P-37b: four transiting planets more massive than Jupiter orbiting moderately bright stars. BAKOS G.A., HARTMAN J.D., TORRES G., et al.
2013A&A...552A.119S viz 15       D               1 1487 118 Magnetic energy fluxes in sub-Alfvenic planet star and moon planet interactions. SAUR J., GRAMBUSCH T., DULING S., et al.
2013A&A...556A.150S viz 15       D               1 635 211 SWEET-Cat: a catalogue of parameters for Stars With ExoplanETs. I. New atmospheric parameters and masses for 48 stars with planets. SANTOS N.C., SOUSA S.G., MORTIER A., et al.
2013A&A...558A..55M viz 38           X         1 20 36 HATS-2b: a transiting extrasolar planet orbiting a K-type star showing starspot activity. MOHLER-FISCHER M., MANCINI L., HARTMAN J.D., et al.
2014A&A...562A.108S viz 15       D               1 196 44 Search for 150 MHz radio emission from extrasolar planets in the TIFR GMRT Sky Survey. SIROTHIA S.K., LECAVELIER DES ETANGS A., GOPAL-KRISHNA, et al.
2014MNRAS.440.1982H viz 40           X         1 23 77 Transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b. HELLIER C., ANDERSON D.R., COLLIER CAMERON A., et al.
2015A&A...574A..39D viz 16       D               1 113 33 Evolution of angular-momentum-losing exoplanetary systems. Revisiting Darwin stability. DAMIANI C. and LANZA A.F.
2015ApJ...806...97K 16       D               1 93 15 Polarization in exoplanetary systems caused by transits, grazing transits, and starspots. KOSTOGRYZ N.M., YAKOBCHUK T.M. and BERDYUGINA S.V.
2016ApJ...827....8N 17       D               2 43 105 Friends of hot jupiters. IV. Stellar companions beyond 50 au might facilitate giant planet formation, but most are unlikely to cause Kozai-Lidov migration. NGO H., KNUTSON H.A., HINKLEY S., et al.
2016AJ....152..181H viz 16       D               1 9279 22 SETI observations of exoplanets with the Allen Telescope Array. HARP G.R., RICHARDS J., TARTER J.C., 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.
2017MNRAS.472.3871T 40           X         1 41 12 Investigating the physical properties of transiting hot Jupiters with the 1.5-m Kuiper Telescope. TURNER J.D., LEITER R.M., BIDDLE L.I., et al.
2016AcA....66...55M 158           X C       3 12 27 New Transit Observations for HAT-P-30 b, HAT-P-37 b, TrES-5 b, WASP-28 b, WASP-36 b and WASP-39 b. MACIEJEWSKI G., DIMITROV D., MANCINI L., 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.
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.
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.
2020A&A...641A..38G 16       D               3 44 ~ TATOO: Tidal-chronology standalone tool to estimate the age of massive close-in planetary systems. GALLET F.
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.
2021ApJS..255...15W 59       D     X         2 82 15 Transiting exoplanet monitoring project (TEMP). VI. The homogeneous refinement of system parameters for 39 transiting hot Jupiters with 127 new light curves. WANG X.-Y., WANG Y.-H., WANG S., 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.
2022AJ....163...77A viz 298           X C       6 6 1 The transit timing and atmosphere of hot Jupiter HAT-P-37b. A-THANO N., JIANG I.-G., AWIPHAN S., 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.
2022MNRAS.512.2062B viz 656   K   D S   X C F     13 21 5 Homogeneous transit timing analyses of 10 exoplanet systems. BASTURK O., ESMER E.M., YALCINKAYA S., 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.
2023NatAs...7..900C viz 17       D               1 1054 ~ On the behaviour of spin-orbit connection of exoplanets. CANTO MARTINS B.L., MESSIAS Y.S., ARRUDA GONCALVES M.I., 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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