HATS-18 , the SIMBAD biblio

HATS-18 , the SIMBAD biblio (32 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST23:58:41

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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
2016AJ....152..127P viz 2209   K A D     X C       55 19 24
HATS-18b: an extreme short-period massive transiting planet spinning up its star. 		PENEV K., HARTMAN J.D., BAKOS G.A., et al.
2017A&A...601A..53E 43           X         1 17 39 The GAPS Programme with HARPS-N at TNG. XIII. The orbital obliquity of three close-in massive planets hosted by dwarf K-type stars: WASP-43, HAT-P-20 and Qatar-2. ESPOSITO M., COVINO E., DESIDERA 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 41           X         1 115 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 99       D       C       7 149 5 Giant planets: good neighbors for habitable worlds? GEORGAKARAKOS N., EGGL S. and DOBBS-DIXON I.
2018AJ....155..165P viz 247     A D     X C       6 83 54 Empirical tidal dissipation in exoplanet hosts from tidal spin-up. PENEV K., BOUMA L.G., WINN J.N., et al.
2018A&A...612L...2K viz 16       D               1 220 7 Signature of non-isotropic distribution of stellar rotation inclination angles in the Praesepe cluster. KOVACS G.
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.
2019MNRAS.482.1872B 43           X         1 6 11 Understanding WASP-12b. BAILEY A. and GOODMAN J.
2019AJ....158...39C 43   K                 1 15 29 Precise photometric transit follow-up observations of five close-in exoplanets: update on their physical properties. CHAKRABARTY A. and SENGUPTA S.
2019AJ....158...59S viz 17       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 17       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 17       D               1 4935 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..150P viz 214     A D     X         6 33 51 The continuing search for evidence of tidal orbital decay of hot Jupiters. PATRA K.C., WINN J.N., HOLMAN M.J., et al.
2020AJ....159..194V viz 17       D               1 288 ~ A statistical search for star-planet interaction in the ultraviolet using GALEX. VISWANATH G., NARANG M., MANOJ P., et al.
2020MNRAS.493..126M 43           X         1 25 19 NGTS-10b: the shortest period hot Jupiter yet discovered. McCORMAC J., GILLEN E., JACKMAN J.A.G., et al.
2020MNRAS.497.3911L 17       D               1 18 ~ Orbital period modulation in hot Jupiter systems. LANZA A.F.
2020A&A...641A..38G 17       D               4 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 2175 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.
2021ApJ...912..123J viz 17       D               1 757 22 Temperature and distance dependence of tidal circularization in close binaries: a catalog of eclipsing binaries in the southern hemisphere observed by the TESS satellite. JUSTESEN A.B. and ALBRECHT S.
2021ApJ...914...56A 192       D     X C       4 55 13 On a possible solution to the tidal realignment problem for hot Jupiters. ANDERSON K.R., WINN J.N. and PENEV K.
2021MNRAS.506.2247A 44           X         1 11 6 The impact of tidal friction evolution on the orbital decay of ultra-short-period planets. ALVARADO-MONTES J.A., SUCERQUIA M., GARCIA-CARMONA C., 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.
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.509.1447M viz 90               F     3 48 5 The ultra-hot-Jupiter KELT-16 b: dynamical evolution and atmospheric properties. MANCINI L., SOUTHWORTH J., NAPONIELLO L., et al.
2022ApJS..258...16P viz 18       D               1 4579 43 TESS Eclipsing Binary stars. I. Short-cadence observations of 4584 eclipsing binaries in sectors 1-26. PRSA A., KOCHOSKA A., CONROY K.E., et al.
2022ApJS..259...62I viz 18       D               1 395 24 TESS Transit Timing of Hundreds of Hot Jupiters. IVSHINA E.S. and WINN J.N.
2022AJ....163..228P viz 45           X         1 73 20 Empirical Limb-darkening Coefficients and Transit Parameters of Known Exoplanets from TESS. PATEL J.A. and ESPINOZA N.
2022MNRAS.515.3212S viz 1837 T K A D S   X C F     38 7 1 A search for transit timing variations in the
HATS-18 planetary system. 		SOUTHWORTH J., BARKER A.J., HINSE T.C., et al.
2022A&A...668A.114R 45           X         1 17 2 Measuring the orbit shrinkage rate of hot Jupiters due to tides. ROSARIO N.M., BARROS S.C.C., DEMANGEON O.D.S., et al.
2024ApJ...960...50W 20       D               1 46 ~ Orbital Decay of Hot Jupiters due to Weakly Nonlinear Tidal Dissipation. WEINBERG N.N., DAVACHI N., ESSICK R., et al.

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