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| WASP-89 , the SIMBAD biblio (22 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST21:59:07 |
| 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 | 1132 | K A | D | S X C | 28 | 10 | 20 |
Three WASP-south transiting exoplanets: WASP-74b, WASP-83b, and WASP-89b. |
HELLIER C., ANDERSON D.R., COLLIER CAMERON A., et al. |
|
2017MNRAS.465.3693H |
79 | X | 2 | 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...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. | ||
|
2018ApJ...856..155G |
96 | D | C | 9 | 149 | 5 | Giant planets: good neighbors for habitable worlds? | GEORGAKARAKOS N., EGGL S. and DOBBS-DIXON I. | |
|
2018A&A...612L...2K |
16 | D | 1 | 220 | 7 | Signature of non-isotropic distribution of stellar rotation inclination angles in the Praesepe cluster. | KOVACS G. | ||
| 2018MNRAS.477..175O | 177 | D | X C | 4 | 42 | 2 | Constraining planetary migration and tidal dissipation with coeval hot Jupiters. | O'CONNOR C.E. and HANSEN B.M.S. | |
|
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. | ||
|
2020A&A...636A..74T |
16 | D | 1 | 2918 | 90 | Public HARPS radial velocity database corrected for systematic errors. | TRIFONOV T., TAL-OR L., ZECHMEISTER M., et al. | ||
|
2020Natur.586..528W |
85 | X | 2 | 14 | 53 | Stellar clustering shapes the architecture of planetary systems. | WINTER A.J., KRUIJSSEN J.M.D., LONGMORE S.N., 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. | ||
|
2022ApJS..259...62I |
17 | D | 1 | 395 | 24 | TESS Transit Timing of Hundreds of Hot Jupiters. | IVSHINA E.S. and WINN J.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. | ||
| 2022MNRAS.516.6145P | 85 | X | 2 | 57 | 1 | Comprehensive Bayesian modelling of tidal circularization in open cluster binaries part I: M 35, NGC 6819, and NGC 188. | PENEV K.M. and SCHUSSLER J.A. | ||
|
2024A&A...683A.125P |
18 | D | 1 | 3561 | ~ | Analysis of the public HARPS/ESO spectroscopic archive Ca II H&K time series for the HARPS radial velocity database. | PERDELWITZ V., TRIFONOV T., TEKLU J.T., 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. | ||
| 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...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. |