WASP-182 , the SIMBAD biblio

WASP-182 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST14:18:15

Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
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
2017AJ....153..257O viz 16       D               1 10625 142 Comoving stars in Gaia DR1: an abundance of very wide separation comoving pairs. OH S., PRICE-WHELAN A.M., HOGG D.W., et al.
2018AJ....155..149B viz 16       D               1 9764 5 Fundamental properties of co-moving stars observed by Gaia. BOCHANSKI J.J., FAHERTY J.K., GAGNE J., et al.
2018MNRAS.478.4513B viz 16       D               1 342691 271 The GALAH Survey: second data release. BUDER S., ASPLUND M., DUONG L., et al.
2019MNRAS.482.5302S viz 16       D               1 54 8 The GALAH survey: co-orbiting stars and chemical tagging. SIMPSON J.D., MARTELL S.L., DA COSTA G., et al.
2019MNRAS.489.2478N 869 T     D     X C       20 11 2 WASP-169, WASP-171, WASP-175, and
WASP-182: three hot Jupiters and one bloated sub-Saturn mass planet discovered by WASP-South. 		NIELSEN L.D., BOUCHY F., TURNER O.D., et al.
2020A&A...636A..74T viz 16       D               1 2918 90 Public HARPS radial velocity database corrected for systematic errors. TRIFONOV T., TAL-OR L., ZECHMEISTER M., et al.
2021ApJ...909..115C viz 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.
2021MNRAS.504.4968C 226       D     X         6 35 13 The GALAH Survey: using galactic archaeology to refine our knowledge of TESS target stars. CLARK J.T., CLERTE M., HINKEL N.R., et al.
2021MNRAS.506..150B viz 17       D               1 588596 276 The GALAH+ survey: Third data release. BUDER S., SHARMA S., KOS J., et al.
2022MNRAS.510.2041C viz 17       D               1 315 3 The GALAH Survey: improving our understanding of confirmed and candidate planetary systems with large stellar surveys. CLARK J.T., WRIGHT D.J., WITTENMYER R.A., et al.
2022MNRAS.512L..60H viz 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 viz 60       D     X         2 395 24 TESS Transit Timing of Hundreds of Hot Jupiters. IVSHINA E.S. and WINN J.N.
2022AJ....163..228P viz 17       D               1 354 20 Empirical Limb-darkening Coefficients and Transit Parameters of Known Exoplanets from TESS. PATEL J.A. and ESPINOZA N.
2022MNRAS.517.5325H viz 17       D               1 214414 23 The GALAH survey: chemical clocks. HAYDEN M.R., SHARMA S., BLAND-HAWTHORN J., et al.
2024A&A...683A.125P viz 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.
2024MNRAS.532.4752D 45           X         1 130 ~ The SHERLOCK pipeline: new exoplanet candidates in the WASP-16, HAT-P-27, HAT-P-26, and TOI-2411 systems. DEVORA-PAJARES M., POZUELOS F.J., THUILLIER A., 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 viz 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 viz 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 viz 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.

goto View the references in ADS