HATS-8 , the SIMBAD biblio

HATS-8 , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.05.07CEST05:55:03


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Title First 3 Authors
2015AJ....150...49B viz 1884   K   D S   X C       46 10 26
HATS-8b: a low-density transiting Super-Neptune.
BAYLISS D., HARTMAN J.D., BAKOS G.A., et al.
2015ApJ...814L..16Z 40           X         1 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.
2017MNRAS.465.3693H viz 42           X         1 35 57 WASP-South transiting exoplanets: WASP-130b, WASP-131b, WASP-132b, WASP-139b, WASP-140b, WASP-141b and WASP-142b. HELLIER C., ANDERSON D.R., COLLIER CAMERON A., 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.
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.
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 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.
2020AJ....159....7M 358       D     X C       8 5 ~ MOPSS. II. Extreme optical scattering slope for the inflated super-Neptune HATS-8b. MAY E.M., GARDNER T., RAUSCHER E., et al.
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.
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.

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