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| WASP-183 , the SIMBAD biblio (14 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST12:58:18 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2019MNRAS.485.5790T |
869 | T | D | X C | 20 | 12 | 3 |
Three hot-Jupiters on the upper edge of the mass-radius distribution: WASP-177, WASP-181, and WASP-183. |
TURNER O.D., ANDERSON D.R., BARKAOUI K., et al. |
|
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. | ||
|
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. | ||
|
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. | ||
| 2024MNRAS.534..843G | 18 | D | 1 | 182 | ~ | Do anomalously dense hot Jupiters orbit stealth binary stars? | GOSWAMY T., COLLIER CAMERON A. and WILSON T.G. | ||
|
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. | ||
| 2025ApJS..277...15J | 19 | D | 2 | 136 | ~ | Half a Million Binary Stars Identified from the Low-resolution Spectra of LAMOST. | JING Y., MAO T.-X., WANG J., et al. | ||
|
2025A&A...697A.102T |
19 | D | 1 | 176 | ~ | Ariel stellar characterisation III. Fast rotators and new FGK stars in the Ariel mission candidate sample. | TSANTAKI M., MAGRINI L., DANIELSKI C., 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 | 120 | D | C | 3 | 480 | ~ | Most Hot Jupiters Were Cool Giant Planets for More Than 1 Gyr. | SCHMIDT S.P. and SCHLAUFMAN K.C. |