BD+21 55B , the SIMBAD biblio

BD+21 55B , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST19:30:03


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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.
2019MNRAS.485.4423S viz 16       D               1 737 39 The Gaia ultracool dwarf sample - II. Structure at the end of the main sequence. SMART R.L., MAROCCO F., SARRO L.M., et al.
2021A&A...645A.100S viz 17       D               2 1696 44 SPECULOOS: Ultracool dwarf transit survey. Target list and strategy. SEBASTIAN D., GILLON M., DUCROT E., et al.
2021A&A...649A...6G viz 17       D               1 227180 168 Gaia Early Data Release 3. The Gaia Catalogue of Nearby Stars. GAIA COLLABORATION, SMART R.L., SARRO L.M., et al.
2022AJ....163..253T viz 17       D               2 397 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.
2022AJ....164..252T viz 17       D               1 129 3 The Perkins INfrared Exosatellite Survey (PINES). II. Transit Candidates and Implications for Planet Occurrence around L and T Dwarfs. TAMBURO P., MUIRHEAD P.S., McCARTHY A.M., 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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