other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Help |
HATS-8 , the SIMBAD biblio (13 results) | C.D.S. - SIMBAD4 rel 1.8 - 2023.10.04CEST05:09:13 |
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 |
---|---|---|---|---|---|---|---|---|---|
2015AJ....150...49B ![]() |
1904 | 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 ![]() |
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 ![]() |
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 ![]() |
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 | 100 | D | C | 7 | 149 | 5 | Giant planets: good neighbors for habitable worlds? | GEORGAKARAKOS N., EGGL S. and DOBBS-DIXON I. | |
2018ApJS..239...14J | 17 | 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 ![]() |
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 ![]() |
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 | 366 | 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 ![]() |
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 ![]() |
18 | 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 ![]() |
18 | 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. |
© Université de Strasbourg/CNRS
• Contact