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| HATS-53 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST20:03:56 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2018AJ....155...79H |
1084 | K A | D | X C | 27 | 25 | 7 |
HATS-50b through HATS-53b: four transiting hot Jupiters orbiting G-type stars discovered by the HATSouth survey. |
HENNING T., MANCINI L., SARKIS P., et al. |
|
2018ApJS..239...14J |
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..190H |
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. | ||
|
2020ApJ...890...23L |
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. | ||
|
2021ApJ...909..115C |
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. | ||
|
2021ApJ...919..138T |
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 |
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 |
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 |
17 | D | 1 | 395 | 24 | TESS Transit Timing of Hundreds of Hot Jupiters. | IVSHINA E.S. and WINN J.N. | ||
|
2024A&A...691A..53S |
18 | D | 1 | 4078 | ~ | SWEET-Cat: A view on the planetary mass-radius relation. | SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., et al. | ||
| 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. |