2MASSI J0859254-194926 , the SIMBAD biblio

2MASSI J0859254-194926 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST11:31:33

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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
2003AJ....126.2421C viz 15       D               1 831 351 Meeting the cool neighbors. V. A 2MASS-Selected sample of ultracool dwarfs. CRUZ K.L., REID I.N., LIEBERT J., et al.
2007AJ....133..439C viz 15       D               307 255 Meeting the cool neighbors. IX. The luminosity function of M7-L8 ultracool dwarfs in the field. CRUZ K.L., REID I.N., KIRKPATRICK J.D., et al.
2008AJ....135..580R 15       D               1 46 33 L-dwarf binaries in the 20-Parsec sample. REID I.N., CRUZ K.L., BURGASSER A.J., et al.
2008MNRAS.390.1517C viz 15       D               142 17 Proper motions of field L and T dwarfs - II. CASEWELL S.L., JAMESON R.F. and BURLEIGH M.R.
2009AJ....137....1F viz 15       D               1 851 248 The brown dwarf kinematics project I. Proper motions and tangential velocities for a large sample of late-type M, L, and T dwarfs. FAHERTY J.K., BURGASSER A.J., CRUZ K.L., et al.
2011AJ....141...54A 15       D               2 144 40 Parallaxes of southern extremely cool objects. I. Targets, proper motions, and first results. ANDREI A.H., SMART R.L., PENNA J.L., et al.
2012ApJ...752...56F viz 15       D               3 187 209 The Brown Dwarf Kinematics Project (BDKP). III. Parallaxes for 70 ultracool dwarfs. FAHERTY J.K., BURGASSER A.J., WALTER F.M., et al.
2013ApJ...767..110P 16       D               1 84 16 Dancing in the dark: new brown dwarf binaries from kernel phase interferometry. POPE B., MARTINACHE F. and TUTHILL P.
2014AJ....147...34S viz 16       D               1 197 46 Discovery of the young L dwarf WISE J174102.78-464225.5. SCHNEIDER A.C., CUSHING M.C., KIRKPATRICK J.D., et al.
2014ApJ...794..143B viz 16       D               1 554 99 SpeX spectroscopy of unresolved very low mass binaries. II. Identification of 14 candidate binaries with late-M/early-L and T dwarf components. BARDALEZ GAGLIUFFI D.C., BURGASSER A.J., GELINO C.R., et al.
2013PASP..125..809T viz 16       D               6 160 39 Nearby M, L, and T dwarfs discovered by the Wide-field Infrared Survey Explorer (WISE). THOMPSON M.A., KIRKPATRICK J.D., MACE G.N., et al.
2015ApJ...810..158F viz 16       D               1 211 260 Fundamental parameters and spectral energy distributions of young and field age objects with masses spanning the stellar to planetary regime. FILIPPAZZO J.C., RICE E.L., FAHERTY J., et al.
2016ApJ...817..112S viz 16       D               1 20551 25 A proper motion survey using the first sky pass of NEOWISE-reactivation data. SCHNEIDER A.C., GRECO J., CUSHING M.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.
2018MNRAS.481.3548S viz 16       D               2 118 1 Parallaxes of Southern Extremely Cool objects III: 118 L and T dwarfs. SMART R.L., BUCCIARELLI B., JONES H.R.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.
2022MNRAS.513..516F 45           X         1 4 1 Using old and new approaches: determining physical properties of brown dwarfs with empirical relations and machine learning models. FEESER S.J. and BEST W.M.J.
2022ApJ...934..178A 18       D               1 157 5 Disentangling the Signatures of Blended-light Atmospheres in L/T Transition Brown Dwarfs. ASHRAF A., BARDALEZ GAGLIUFFI D.C., MANJAVACAS E., et al.
2022AJ....164..244F viz 18       D               4 115 2 NICMOS Kernel-phase Interferometry. I. Catalogue of Brown Dwarfs Observed in F110W and F170M. FACTOR S.M. and KRAUS A.L.
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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