CD-34 8618 , the SIMBAD biblio

CD-34 8618 , the SIMBAD biblio (31 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST09:21:19


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Title First 3 Authors
2017MNRAS.471.2743T 1056     A     X C       26 23 35
WASP-167b/
KELT-13b: joint discovery of a hot Jupiter transiting a rapidly rotating F1V star.
TEMPLE L.Y., HELLIER C., ALBROW M.D., 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.
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...636A..74T viz 16       D               1 2918 90 Public HARPS radial velocity database corrected for systematic errors. TRIFONOV T., TAL-OR L., ZECHMEISTER M., et al.
2020MNRAS.496..504N 44           X         1 16 55 Searching for thermal inversion agents in the transmission spectrum of KELT-20b/MASCARA-2b: detection of neutral iron and ionised calcium H&K lines. NUGROHO S.K., GIBSON N.P., DE MOOIJ E.J.W., et al.
2020ApJS..250...20C viz 16       D               1 141 41 A search for rotation periods in 1000 TESS objects of interest. CANTO MARTINS B.L., GOMES R.L., MESSIAS Y.S., 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.
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.
2021A&A...647A..49S viz 351       D     X C       8 41 12 Chemical analysis of early-type stars with planets. SAFFE C., MIQUELARENA P., ALACORIA J., et al.
2021ApJ...916L...1A 17       D               1 57 40 A preponderance of perpendicular planets. ALBRECHT S.H., MARCUSSEN M.L., WINN J.N., 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.
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.
2022PASP..134h2001A viz 17       D               1 366 39 Stellar Obliquities in Exoplanetary Systems. ALBRECHT S.H., DAWSON R.I. and WINN J.N.
2022MNRAS.516...75B 17       D               1 115 9 Exploring the dependence of hot Jupiter occurrence rates on stellar mass with TESS. BELEZNAY M. and KUNIMOTO M.
2022A&A...668A.157S 187       D     X         5 48 1 Are Am stars and hot-Jupiter planets related? SAFFE C., ALACORIA J., MIQUELARENA P., et al.
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.
2024AJ....167...48M 18       D               2 72 ~ Signs of Similar Stellar Obliquity Distributions for Hot and Warm Jupiters Orbiting Cool Stars. MORGAN M., BOWLER B.P., TRAN Q.H., et al.
2024AJ....167..126R 18       D               2 141 ~ The Orbital Geometries and Stellar Obliquities of Exoplanet-hosting Multistar Systems. RICE M., GERBIG K. and VANDERBURG A.
2024A&A...686L...1M 18       D               3 48 ~ Gas, not dust: Migration of TESS/Gaia hot Jupiters possibly halted by the magnetospheres of protoplanetary disks. MENDIGUTIA I., LILLO-BOX J., VIOQUE M., et al.
2024A&A...687A.144K 1012     A     X C       22 16 ~ The phase curve of the ultra-hot Jupiter
WASP-167b as seen by TESS.
KALMAN S., DEREKAS A., CSIZMADIA S., 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.
2025RNAAS...9...33K 280           X C       5 4 ~ Detection of a Peculiar Noise Type in the TESS “Fast” Light Curves. KALMAN S., CSIZMADIA S., PAL A., et al.
2025A&A...695A..27M viz 19       D               1 132 ~ Intermediate-mass stars and the origin of the gas-giant planet-metallicity correlation. MALDONADO J., MIROUH G.M., MENDIGUTIA I., et al.
2025ApJ...983L..42R 47           X         1 32 ~ From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest Mp/M* Systems Exhibit Low Obliquities, Even around Hot Stars. RUSZNAK J., WANG X.-Y., RICE M., et al.
2025A&A...697A.102T viz 19       D               1 176 ~ Ariel stellar characterisation III. Fast rotators and new FGK stars in the Ariel mission candidate sample. TSANTAKI M., MAGRINI L., DANIELSKI C., 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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