HATS-14 , the SIMBAD biblio

HATS-14 , the SIMBAD biblio (32 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST19:52:18

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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
2015A&A...580A..63M viz 1560   K A D     X C       40 7 9 HATS-13b and
HATS-14b: two transiting hot Jupiters from the HATSouth survey. 		MANCINI L., HARTMAN J.D., PENEV K., et al.
2015ApJ...814L..16Z 312           X         8 18 9 A high obliquity orbit for the Hot-Jupiter HATS-14b transiting a 5400K star. ZHOU G., BAYLISS D., HARTMAN J.D., et al.
2016ApJ...823...29A 16       D               1 117 7 Spin-orbit alignment for three transiting hot jupiters: WASP-103b, WASP-87b, and WASP-66b. ADDISON B.C., TINNEY C.G., WRIGHT D.J., 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.
2018A&A...610A..20E viz 80           X         2 115 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.
2018A&A...613A..41M viz 43           X         1 13 47 The GAPS programme with HARPS-N at TNG. XVI. Measurement of the Rossiter-McLaughlin effect of transiting planetary systems HAT-P-3, HAT-P-12, HAT-P-22, WASP-39, and WASP-60. MANCINI L., ESPOSITO M., COVINO E., 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...59S viz 16       D               1 109 ~ Autoregressive planet search: feasibility study for irregular time series. STUHR A.M., FEIGELSON E.D., CACERES 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.
2019AJ....158..243P viz 16       D               1 160 18 A search for multiplanet systems with TESS using a Bayesian N-body retrieval and machine learning. PEARSON K.A.
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.
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.
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....161..164H viz 100       D       C       2 192 26 Speckle observations of TESS exoplanet host stars: understanding the binary exoplanet host star orbital period distribution. HOWELL S.B., MATSON R.A., CIARDI D.R., et al.
2021AJ....162...75L viz 17       D               1 517 28 Speckle observations of TESS exoplanet host stars. II. Stellar companions at 1-1000 au and implications for small planet detection. LESTER K.V., MATSON R.A., HOWELL S.B., 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.
2022AJ....164..104R viz 17       D               1 105 10 A Tendency Toward Alignment in Single-star Warm-Jupiter Systems. RICE M., WANG S., WANG X.-Y., et al.
2022PASP..134h2001A viz 43           X         1 366 39 Stellar Obliquities in Exoplanetary Systems. ALBRECHT S.H., DAWSON R.I. and WINN J.N.
2024ApJ...973L..21W 45           X         1 46 ~ Single-star Warm-Jupiter Systems Tend to Be Aligned, Even around Hot Stellar Hosts: No Teff-λ Dependency. WANG X.-Y., RICE M., WANG S., 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.
2025AJ....170...70E 47           X         1 38 ~ The Spin-Orbit Alignment of Eight Warm Gas Giant Systems. ESPINOZA-RETAMAL J.I., JORDAN A., BRAHM R., et al.
2025PASP..137g4401G 47           X         1 13 ~ A Hot Jupiter with a Retrograde Orbit Around A Sun-like Star and a Toy Model of Hot Jupiters in Wide Binary Star Systems. GIACALONE S., HOWARD A.W., RUBENZAHL R.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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