WASP-104 , the SIMBAD biblio

WASP-104 , the SIMBAD biblio (32 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST19:31:00


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Title First 3 Authors
2014A&A...570A..64S viz 2205     A D S   X C       56 9 9
WASP-104b and WASP-106b: two transiting hot Jupiters in 1.75-day and 9.3-day orbits.
SMITH A.M.S., ANDERSON D.R., ARMSTRONG D.J., et al.
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.
2015A&A...579A.129W 16       D               1 71 19 A Lucky Imaging search for stellar sources near 74 transit hosts. WOELLERT M. and BRANDNER W.
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.
2018A&A...610A..20E viz 161           X         4 115 9 High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP). II. Lucky Imaging results from 2015 and 2016. EVANS D.F., SOUTHWORTH J., SMALLEY B., 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.
2018AJ....156...44M 586     A     X C       14 6 4
WASP-104b is darker than charcoal.
MOCNIK T., HELLIER C. and SOUTHWORTH J.
2018MNRAS.473.1801G 40           X         1 78 1 Exoplanet phase curves at large phase angles. Diagnostics for extended hazy atmospheres. GARCIA MUNOZ A. and CABRERA J.
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.
2018A&A...620A..58S viz 16       D               1 164 10 SWEET-Cat updated. New homogenous spectroscopic parameters. SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., 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.
2019MNRAS.490.5088M viz 16       D               2 214 32 Search for stellar companions of exoplanet host stars by exploring the second ESA-Gaia data release. MUGRAUER M.
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..137G 17       D               3 74 83 Statistical characterization of hot Jupiter atmospheres using Spitzer's secondary eclipses. GARHART E., DEMING D., MANDELL A., et al.
2021MNRAS.500.5420C viz 585           X C       13 16 14 An enhanced slope in the transmission spectrum of the hot Jupiter WASP-104b. CHEN G., PALLE E., PARVIAINEN H., 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.
2021ApJS..255...15W 17       D               1 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...923..242G 17       D               2 56 ~ Why is it so hot in here? Exploring population trends in Spitzer thermal emission observations of hot Jupiters using planet-specific, self-consistent atmospheric models. GOYAL J.M., LEWIS N.K., WAKEFORD H.R., et al.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL M., et al.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., 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.
2022A&A...663A...4S viz 17       D               1 14206 7 Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. SOUBIRAN C., BROUILLET N. and CASAMIQUELA L.
2022A&A...663A.161M viz 17       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.
2023AJ....165..262Z viz 17       D               1 314 ~ Scaling K2. VI. Reduced Small-planet Occurrence in High-galactic-amplitude Stars. ZINK J.K., HARDEGREE-ULLMAN K.K., CHRISTIANSEN J.L., et al.
2024A&A...688A.193D viz 18       D               1 182 ~ Ariel stellar characterisation II. Chemical abundances of carbon, nitrogen, and oxygen for 181 planet-host FGK dwarf stars. DA SILVA R., DANIELSKI C., DELGADO MENA E., et al.
2024MNRAS.534..843G 18       D               1 182 ~ Do anomalously dense hot Jupiters orbit stealth binary stars? GOSWAMY T., COLLIER CAMERON A. and WILSON T.G.
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...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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