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| HAT-P-66 , the SIMBAD biblio (20 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST15:05:56 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2016AJ....152..182H |
2573 | K | D | X C | 65 | 205 | 26 |
HAT-P-65b and HAT-P-66b: two transiting inflated hot Jupiters and observational evidence for the reinflation of close-in giant planets. |
HARTMAN J.D., BAKOS G.A., BHATTI W., 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. | ||
|
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. | ||
|
2020AJ....159..194V |
16 | D | 2 | 288 | ~ | A statistical search for star-planet interaction in the ultraviolet using GALEX. | VISWANATH G., NARANG M., MANOJ P., et al. | ||
|
2021A&A...645A...7K |
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 |
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. | ||
| 2021A&A...653A.147M | 42 | X | 1 | 16 | 4 | TOI-1296b and TOI-1298b observed with TESS and SOPHIE: two hot Saturn-mass exoplanets with different densities around metal-rich stars. | MOUTOU C., ALMENARA J.M., HEBRARD G., et al. | ||
| 2022AJ....163..104F | 17 | D | 2 | 61 | 7 | The Breakthrough Listen search for intelligent life: technosignature search of Transiting TESS Targets of Interest. | FRANZ N., CROFT S., SIEMION A.P.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. | ||
|
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. | ||
|
2022MNRAS.513..102C |
17 | D | 1 | 961 | 6 | The TESS Triple-9 Catalog: 999 uniformly vetted exoplanet candidates. | CACCIAPUOTI L., KOSTOV V.B., KUCHNER M., et al. | ||
|
2022ApJS..261...26S |
17 | D | 2 | 1893 | 2 | Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys. | SU T., ZHANG L.-Y., LONG L., et al. | ||
|
2023ApJS..264...17Z |
17 | D | 3 | 31380 | 1 | Stellar Parameters and Spectroscopic Properties of TESS Objects Observed in the LAMOST Low- and Medium-resolution Spectral Survey. | ZHANG L.-Y., SU T., MISRA P., et al. | ||
| 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. | ||
|
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. | ||
| 2025RNAAS...9..275M | 19 | D | 1 | 365 | ~ | An In-depth Study of Brown Dwarfs with TESS. | MARCADON F. and PRSA A. | ||
| 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. |