CD-46 1323 , the SIMBAD biblio

CD-46 1323 , the SIMBAD biblio (32 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:18:25

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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
2017ApJ...834...17C viz 16       D               1 290 454 Probabilistic forecasting of the masses and radii of other worlds. CHEN J. and KIPPING D.
2016PASP..128f4401T viz 1117       D S   X C       27 23 6 WASP-120 b, WASP-122 b, AND WASP-123 b: three newly discovered planets from the WASP-South survey. TURNER O.D., ANDERSON D.R., COLLIER CAMERON A., 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...609A.116R viz 16       D               1 143018 65 Empirical photometric calibration of the Gaia red clump: Colours, effective temperature, and absolute magnitude. RUIZ-DERN L., BABUSIAUX C., ARENOU F., 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.
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.
2018A&A...620A.172Z viz 16       D               1 127610 99 3D mapping of young stars in the solar neighbourhood with Gaia DR2. ZARI E., HASHEMI H., BROWN A.G.A., 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.
2020AJ....159...19Z viz 17       D               1 125 132 SOAR TESS Survey. I. Sculpting of TESS planetary systems by stellar companions. ZIEGLER C., TOKOVININ A., BRICENO C., et al.
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...635A..73B viz 535     A D S   X         13 73 22 A multiplicity study of transiting exoplanet host stars. I. High-contrast imaging with VLT/SPHERE. BOHN A.J., SOUTHWORTH J., GINSKI 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.
2020AJ....160..155W viz 82           X         2 61 45 Systematic phase curve study of known transiting systems from year one of the TESS mission. WONG I., SHPORER A., DAYLAN T., 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.
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 17       D               1 354 20 Empirical Limb-darkening Coefficients and Transit Parameters of Known Exoplanets from TESS. PATEL J.A. and ESPINOZA N.
2022MNRAS.513..102C viz 17       D               1 961 6 The TESS Triple-9 Catalog: 999 uniformly vetted exoplanet candidates. CACCIAPUOTI L., KOSTOV V.B., KUCHNER M., et al.
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.
2022AcA....72....1M viz 12 3 Search for planets in hot Jupiter systems with multi-sector TESS photometry. II. Constraints on planetary companions in 12 systems. MACIEJEWSKI G.
2024A&A...683A.125P viz 18       D               1 3561 ~ Analysis of the public HARPS/ESO spectroscopic archive Ca II H&K time series for the HARPS radial velocity database. PERDELWITZ V., TRIFONOV T., TEKLU J.T., et al.
2024A&A...686A.147Z 108       D         F     4 19 ~ Stellar obliquity measurements of six gas giants Orbital misalignment of WASP-101b and WASP-131b. ZAK J., BOCCHIERI A., SEDAGHATI E., et al.
2024A&A...688A.193D viz 63       D     X         2 182 ~ 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.
2024ApJS..274...20P 18       D               1 223 ~ Statistics and Habitability of F-type Star-Planet Systems. PATEL S.D., CUNTZ M. and WEINBERG N.N.
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.
2024MNRAS.535.1778E 18       D               1 139 ~ Viewing the PLATO LOPS2 field through the lenses of TESS. ESCHEN Y.N.E., BAYLISS D., WILSON T.G., 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.
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.
2026ApJ...996L...7W 50           X         1 48 ~ Unified Kraft Break at ∼6500 K: A Newly Identified Single-star Obliquity Transition Matches the Classical Rotation Break. WANG X.-Y., WANG S. and ONG J.M.J.
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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