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| HATS-66 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST00:01:19 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
2019AJ....157...55H 
|
812 | A | D | X C | 20 | 22 | 11 | HATS-60b-HATS-69b: 10 transiting planets from HATSouth. | HARTMAN J.D., BAKOS G.A., BAYLISS D., 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. | ||
|
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. | ||
|
2022AJ....163..228P
|
17 | D | 1 | 354 | 20 | Empirical Limb-darkening Coefficients and Transit Parameters of Known Exoplanets from TESS. | PATEL J.A. and ESPINOZA N. | ||
| 2024ApJS..274...20P | 18 | D | 1 | 223 | ~ | Statistics and Habitability of F-type Star-Planet Systems. | PATEL S.D., CUNTZ M. and WEINBERG N.N. | ||
| 2024MNRAS.535.1778E | 18 | D | 1 | 139 | ~ | Viewing the PLATO LOPS2 field through the lenses of TESS. | ESCHEN Y.N.E., BAYLISS D., WILSON T.G., et al. | ||
|
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. |
