HD 12051B , the SIMBAD biblio

HD 12051B , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST14:44:53


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Title First 3 Authors
2014ApJ...792..119D viz 15       D               1 184 63 Wide cool and ultracool companions to nearby stars from Pan-STARRS 1. DEACON N.R., LIU M.C., MAGNIER E.A., et al.
2020AJ....159..257B viz 16       D               3 378 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.
2021AJ....161...42B viz 17       D               1 398 43 A volume-limited sample of ultracool dwarfs. I. Construction, space density, and a gap in the L/T transition. BEST W.M.J., LIU M.C., MAGNIER E.A., et al.
2022AJ....163..253T viz 17       D               1 397 8 The Perkins INfrared Exosatellite Survey (PINES) I. Survey Overview, Reduction Pipeline, and Early Results. TAMBURO P., MUIRHEAD P.S., McCARTHY A.M., et al.
2022ApJ...935...15Z 85             C       1 61 ~ COol Companions ON Ultrawide orbiTS (COCONUTS). III. A Very Red L6 Benchmark Brown Dwarf around a Young M5 Dwarf. ZHANG Z., LIU M.C., MORLEY C.V., 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.
2023AJ....166..103S viz 17       D               1 997 ~ Astrometry and Photometry for ≈1000 L, T, and Y Dwarfs from the UKIRT Hemisphere Survey. SCHNEIDER A.C., MUNN J.A., VRBA F.J., et al.
2024ApJ...960..105Z 18       D               1 129 ~ A Possible Correlation between Metallicity and Near-IR Color for Late-M and L Dwarfs. ZHANG R., LIU M.C. and ZHANG Z.
2024ApJ...963...67C 18       D               2 117 ~ Predicting Cloud Conditions in Substellar Mass Objects Using Ultracool Dwarf Companions. CALAMARI E., FAHERTY J.K., VISSCHER C., 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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