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| WASP-165 , the SIMBAD biblio (20 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST11:36:45 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2013AJ....146..134K |
15 | D | 1 | 419759 | 301 | The radial velocity experiment (RAVE): fourth data release. | KORDOPATIS G., GILMORE G., STEINMETZ M., et al. | ||
|
2014AJ....148...81M |
15 | D | 1 | 329182 | 108 | APASS Landolt-Sloan BVgri photometry of RAVE stars. I. Data, effective temperatures, and reddenings. | MUNARI U., HENDEN A., FRIGO A., et al. | ||
|
2017AJ....153...75K |
16 | D | 1 | 451448 | 394 | The Radial Velocity Experiment (RAVE): fifth data release. | KUNDER A., KORDOPATIS G., STEINMETZ M., et al. | ||
|
2019MNRAS.482..301L |
893 | A | D | S X C F | 20 | 14 | 5 | WASP-147b, 160Bb, 164b, and 165b: two hot Saturns and two Jupiters, including two planets with metal-rich hosts. | LENDL M., ANDERSON D.R., BONFANTI A., 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. | ||
|
2020AJ....159..194V |
16 | D | 1 | 288 | ~ | A statistical search for star-planet interaction in the ultraviolet using GALEX. | VISWANATH G., NARANG M., MANOJ P., et al. | ||
|
2020AJ....160...83S |
16 | D | 1 | 451375 | 83 | The sixth Data Release of the Radial Velocity Experiment (RAVE). II. Stellar atmospheric parameters, chemical abundances, and distances. | STEINMETZ M., GUIGLION G., McMILLAN P.J., et al. | ||
|
2020MNRAS.498.1726M |
16 | D | 1 | 337 | 26 | A search for transiting planets around FGKM dwarfs and subgiants in the TESS full frame images of the Southern ecliptic hemisphere. | MONTALTO M., BORSATO L., GRANATA V., 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.509.3339K | 43 | X | 1 | 16 | 5 | Discovery of an inflated hot Jupiter around a slightly evolved star TOI-1789. | KHANDELWAL A., CHATURVEDI P., CHAKRABORTY A., 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. | ||
|
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. | ||
|
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. |