2MASS J14482563+1031590 , the SIMBAD biblio

2MASS J14482563+1031590 , the SIMBAD biblio (31 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST17:12:01


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Title First 3 Authors
2003IAUS..211..197W 29 44 New M and L dwarfs confirmed with CorMass. WILSON J.C., MILLER N.A., GIZIS J.E., et al.
2006AJ....132..891R viz 15       D               56 93 A search for binary systems among the nearest L dwarfs. REID I.N., LEWITUS E., ALLEN P.R., et al.
2007AJ....133.2258S viz 15       D               154 169 Activity and kinematics of ultracool dwarfs, including an amazing flare observation. SCHMIDT S.J., CRUZ K.L., BONGIORNO B.J., et al.
2008MNRAS.384.1399J viz 15       D               162 32 Proper motions of field L and T dwarfs. JAMESON R.F., CASEWELL S.L., BANNISTER N.P., et al.
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.
2009MNRAS.394..857D viz 15       D               1 283 26 The UKIDSS-2MASS proper motion survey - I. Ultracool dwarfs from UKIDSS DR4. DEACON N.R., HAMBLY N.C., KING R.R., et al.
2008AJ....136.1290R viz 15       D               468 204 Meeting the cool neighbors. X. Ultracool dwarfs from the 2MASS all-sky data release. REID N.I., CRUZ K.L., KIRKPATRICK J.D., et al.
2010ApJ...710.1142B viz 15       D               2 210 205 SpeX spectroscopy of unresolved very low mass binaries. I. Identification of 17 candidate binaries straddling the L dwarf/T dwarf transition. BURGASSER A.J., CRUZ K.L., CUSHING M., et al.
2010AJ....139.1808S viz 15       D               2 579 150 Colors and kinematics of L dwarfs from the Sloan Digital Sky Survey. SCHMIDT S.J., WEST A.A., HAWLEY S.L., et al.
2010A&A...518A..10V viz 15       D               1 168913 597 A catalogue of quasars and active nuclei: 13th edition. VERON-CETTY M.-P. and VERON P.
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.
2014PASP..126..642S 16       D               1 141 22 Calibrating ultracool dwarfs : optical template spectra, bolometric corrections, and {Chi } values. SCHMIDT S.J., WEST A.A., BOCHANSKI J.J., et al.
2015AJ....149..158S viz 16       D               1 188 96 BOSS ultracool dwarfs. I. Colors and magnetic activity of M and l dwarfs. SCHMIDT S.J., HAWLEY S.L., WEST A.A., et al.
2015ApJ...805...90T viz 40           X         1 146 135 The most luminous galaxies discovered by WISE. TSAI C.-W., EISENHARDT P.R.M., WU J., et al.
2015ApJS..219...33G viz 16       D               2 430 153 BANYAN. VII. A new population of young substellar candidate members of nearby moving groups from the BASS survey. GAGNE J., FAHERTY J.K., CRUZ K.L., 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.
2016A&A...589A..49S viz 16       D               1 1371 27 Photometric brown-dwarf classification. II. A homogeneous sample of 1361 L and T dwarfs brighter than J = 17.5 with accurate spectral types. SKRZYPEK N., WARREN S.J. and FAHERTY J.K.
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.
2016ApJS..225...10F viz 16       D               3 212 193 Population properties of brown dwarf analogs to exoplanets. FAHERTY J.K., RIEDEL A.R., CRUZ K.L., et al.
2017AJ....154..147D viz 16       D               1 324 9 CCD parallaxes for 309 late-type dwarfs and subdwarfs. DAHN C.C., HARRIS H.C., SUBASAVAGE J.P., et al.
2019MNRAS.485.4423S viz 17       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.
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.
2019ApJ...883..205B viz 17       D               1 500 34 The ultracool SpeXtroscopic survey. I. Volume-limited spectroscopic sample and luminosity function of M7-L5 ultracool dwarfs. BARDALEZ GAGLIUFFI D.C., BURGASSER A.J., SCHMIDT S.J., et al.
2020AJ....159..257B viz 17       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.
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.
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.
2022MNRAS.513.5701S viz 108       D         F     7 132 9 Ultracool dwarfs observed with the Spitzer infrared spectrograph - II. Emergence and sedimentation of silicate clouds in L dwarfs, and analysis of the full M5-T9 field dwarf spectroscopic sample. SUAREZ G. and METCHEV S.
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.
2023MNRAS.523.4739S 19       D               2 28 ~ Ultracool dwarfs observed with the Spitzer Infrared Spectrograph - III. Dust grains in young L dwarf atmospheres are heavier. SUAREZ G. and METCHEV S.
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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