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| WASP-142 , the SIMBAD biblio (21 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST19:04:33 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2017MNRAS.465.3693H |
532 | K | D | X C | 13 | 35 | 57 |
WASP-South transiting exoplanets: WASP-130b, WASP-131b, WASP-132b, WASP-139b, WASP-140b, WASP-141b and WASP-142b. |
HELLIER C., ANDERSON D.R., COLLIER CAMERON A., 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....160..155W |
181 | D | X | 5 | 61 | 45 | Systematic phase curve study of known transiting systems from year one of the TESS mission. | WONG I., SHPORER A., DAYLAN T., 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 | 3 | 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. | ||
|
2022ApJS..258...16P |
17 | D | 1 | 4582 | 43 | TESS Eclipsing Binary stars. I. Short-cadence observations of 4584 eclipsing binaries in sectors 1-26. | PRSA A., KOCHOSKA A., CONROY K.E., 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. | ||
|
2022A&A...663A.161M |
17 | D | 1 | 213 | 8 | Ariel stellar characterisation. I. Homogeneous stellar parameters of 187 FGK planet host stars: Description and validation of the method. | MAGRINI L., DANIELSKI C., BOSSINI D., et al. | ||
|
2024AJ....167..203M |
197 | D | X | 5 | 805 | ~ | DIAmante TESS AutoRegressive Planet Search (DTARPS). II. Hundreds of New TESS Candidate Exoplanets. | MELTON E.J., FEIGELSON E.D., MONTALTO M., et al. | |
|
2024A&A...688A.193D |
18 | D | 1 | 182 | ~ | Ariel stellar characterisation II. Chemical abundances of carbon, nitrogen, and oxygen for 181 planet-host FGK dwarf stars. | DA SILVA R., DANIELSKI C., DELGADO MENA E., 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. | ||
| 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. | ||
| 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. |