other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Help |
HATS-22 , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2023.09.24CEST13:38:07 |
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 |
---|---|---|---|---|---|---|---|---|---|
2017MNRAS.468..835B | 1786 | K | D | X C F | 42 | 10 | 7 |
HATS-22b, HATS-23b and HATS-24b: three new transiting super-Jupiters from the HATSouth project. |
BENTO J., SCHMIDT B., HARTMAN J.D., 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. | ||
2018MNRAS.478.4513B ![]() |
17 | D | 1 | 342691 | 271 | The GALAH Survey: second data release. | BUDER S., ASPLUND M., DUONG L., 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. | ||
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. | ||
2021MNRAS.506..150B ![]() |
18 | D | 1 | 588596 | 276 | The GALAH+ survey: Third data release. | BUDER S., SHARMA S., KOS J., et al. | ||
2021AJ....162..263H ![]() |
18 | 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. | ||
2022ApJS..259...62I ![]() |
19 | D | 1 | 395 | 24 | TESS Transit Timing of Hundreds of Hot Jupiters. | IVSHINA E.S. and WINN J.N. | ||
2022A&A...663A.161M ![]() |
47 | X | 1 | 32 | 8 | Ariel stellar characterisation. I. Homogeneous stellar parameters of 187 FGK planet host stars: Description and validation of the method. | MAGRINI L., DANIELSKI C., BOSSINI D., et al. |
© Université de Strasbourg/CNRS
• Contact