WISE J163645.56-074325.1 , the SIMBAD biblio

WISE J163645.56-074325.1 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST05:21:01


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Title First 3 Authors
2013ApJS..205....6M viz 15       D               1 307 112 A study of the diverse T dwarf population revealed by WISE. MACE G.N., KIRKPATRICK J.D., CUSHING M.C., et al.
2014yCat.5144....0M viz 15       D               1 103 ~ Investigating low-mass binary stars and brown dwarfs with near-infrared spectroscopy (Thesis, University of California, Los Angeles (2014)). MACE G.N.
2020AJ....159..257B viz 16       D               2 378 38 The Hawaii infrared parallax program. IV. A comprehensive parallax survey of L0-T8 dwarfs with UKIRT. BEST W.M.J., LIU M.C., MAGNIER E.A., et al.
2021ApJ...911....7Z 393       D     X         10 63 21 The Hawaii infrared parallax program. V. New T-dwarf members and candidate members of nearby young moving groups. ZHANG Z., LIU M.C., BEST W.M.J., et al.
2023A&A...670A..19G viz 17       D               1 5915 6 The Fifth Catalogue of Nearby Stars (CNS5). GOLOVIN A., REFFERT S., JUST A., et al.
2023ApJ...959...63S 17       D               1 177 ~ The Hawaii Infrared Parallax Program. VI. The Fundamental Properties of 1000+ Ultracool Dwarfs and Planetary-mass Objects Using Optical to Mid-infrared Spectral Energy Distributions and Comparison to BT-Settl and ATMO 2020 Model Atmospheres. SANGHI A., LIU M.C., BEST W.M.J., et al.
2024MNRAS.527.6624L 197       D       C F     11 98 ~ A near-infrared variability survey of young planetary-mass objects. LIU P., BILLER B.A., VOS J.M., et al.
2024A&A...684A..69G viz 18       D               1 159 ~ Implications of the discovery of AF Lep b The mass-luminosity relation for planets in the β Pic Moving Group and the L-T transition for young companions and free-floating planets. GRATTON R., BONAVITA M., MESA D., et al.
2026AJ....171..198M 20       D               4 144 ~ Uniform Forward-modeling Analysis of Ultracool Dwarfs. IV. Benchmarking the Sonora Diamondback and D. Saumon & M. S. Marley () Atmospheric Models Across Late M, L, and T Types with Low-resolution 0.8-2.5 μm Spectroscopy. MADER E., ZHANG Z., FORTNEY J.J., et al.

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