TVLM 262-111511 , the SIMBAD biblio

TVLM 262-111511 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.28CEST00:41:45


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Title First 3 Authors
1993ApJ...414..279T viz 432 72 The fainstest stars : the luminosity and mass functions at the bottom of the main sequence. TINNEY C.G.
1995AJ....110.3014T 36 79 Trigonometric parallaxes and the HR diagram at the bottom of the main sequence. TINNEY C.G., REID I.N., GIZIS J., et al.
2008AJ....135..785W viz 15       D               43982 487 Constraining the age-activity relation for cool stars: the Sloan Digital Sky Survey Data Release 5 low-mass star spectroscopic sample. WEST A.A., HAWLEY S.L., BOCHANSKI J.J., et al.
2011AJ....141...97W viz 15       D               1 70845 269 The Sloan Digital Sky Survey Data Release 7 spectroscopic M dwarf catalog. I. Data. WEST A.A., MORGAN D.P., BOCHANSKI J.J., et al.
2011ApJS..197...19K viz 15       D               1 575 330 The first hundred brown dwarfs discovered by the Wide-field Infrared Survey Explorer (WISE). KIRKPATRICK J.D., CUSHING M.C., GELINO C.R., et al.
2012ApJS..201...19D viz 15       D               1 267 460 The Hawaii infrared parallax program. I. Ultracool binaries and the L/T transition. DUPUY T.J. and LIU M.C.
2016ApJS..224...36K viz 16       D               1 45305 70 The AllWISE motion survey, part 2. KIRKPATRICK J.D., KELLOGG K., SCHNEIDER A.C., et al.
2017MNRAS.468.3499D viz 16       D               1 278 6 Identification of partially resolved binaries in Pan-STARRS 1 data. DEACON N.R., MAGNIER E.A., BEST W.M.J., et al.
2019AJ....157..231K viz 17       D               1 74143 43 Exploring the age-dependent properties of M and L dwarfs using Gaia and SDSS. KIMAN R., SCHMIDT S.J., ANGUS R., et al.
2021A&A...649A...6G viz 17       D               1 89188 168 Gaia Early Data Release 3. The Gaia Catalogue of Nearby Stars. GAIA COLLABORATION, SMART R.L., SARRO L.M., et al.
2023ApJ...959...63S 19       D               1 137 ~ 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.

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