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| WASP-83 , the SIMBAD biblio (25 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST17:46:49 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2015AJ....150...18H | 602 | K | D | S X C | 14 | 10 | 20 |
Three WASP-south transiting exoplanets: WASP-74b, WASP-83b, and WASP-89b. |
HELLIER C., ANDERSON D.R., COLLIER CAMERON A., et al. |
|
2017AJ....153..136S |
16 | D | 1 | 525 | 287 | Accurate empirical radii and masses of planets and their host stars with Gaia parallaxes. | STASSUN K.G., COLLINS K.A. and GAUDI B.S. | ||
|
2017A&A...602A.107B |
16 | D | 2 | 476 | 185 | The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets. | BONOMO A.S., DESIDERA S., BENATTI S., 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. | ||
|
2018A&A...610A..20E |
40 | X | 1 | 115 | 9 | High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP). II. Lucky Imaging results from 2015 and 2016. | EVANS D.F., SOUTHWORTH J., SMALLEY B., et al. | ||
|
2018ApJ...856..155G |
96 | D | C | 7 | 149 | 5 | Giant planets: good neighbors for habitable worlds? | GEORGAKARAKOS N., EGGL S. and DOBBS-DIXON I. | |
|
2018MNRAS.474.5158G |
16 | D | 1 | 131 | 85 | A library of ATMO forward model transmission spectra for hot Jupiter exoplanets. | GOYAL J.M., MAYNE N., SING D.K., 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. | ||
| 2018PASP..130k4503P | 247 | S X C | 4 | 1 | 6 | TESS in the solar system. | PAL A., MOLNAR L. and KISS C. | ||
|
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. | ||
|
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. | ||
|
2021AJ....162..192Z |
17 | D | 1 | 713 | 29 | SOAR TESS survey. II. The impact of stellar companions on planetary populations. | ZIEGLER C., TOKOVININ A., LATIOLAIS M., 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 |
102 | D | X | 3 | 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. | ||
|
2022ApJS..261...26S |
17 | D | 1 | 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. | ||
|
2024AJ....167..203M |
108 | D | X | 3 | 805 | ~ | DIAmante TESS AutoRegressive Planet Search (DTARPS). II. Hundreds of New TESS Candidate Exoplanets. | MELTON E.J., FEIGELSON E.D., MONTALTO M., 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. | ||
|
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. | ||
|
2025A&A...699A.100D |
19 | D | 1 | 2580 | ~ | The Gaia spectroscopic catalogue of exoplanets and host stars. | DE LAVERNY P., LIGI R., CRIDA A., 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. |