2MASS J01245068-3844389 , the SIMBAD biblio

2MASS J01245068-3844389 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST08:09:56


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Title First 3 Authors
1997MNRAS.284..507T 11 19 Lithium detection in a field brown dwarf candidate. THACKRAH A., JONES H. and HAWKINS M.
1998AJ....115.1648P 73 17 The solar neighborhood. V. VRI photometry of southern nearby star candidates. PATTERSON R.J., IANNA P.A. and BEGAM M.C.
1999A&A...343..883N 105 91 Search for X-ray emission from bona-fide and candidate brown dwarfs. NEUHAEUSER R., BRICENO C., COMERON F., et al.
1999ApJ...519..802K 3 79 846 Dwarfs cooler than ``M'': the definition of spectral type ``L'' using discoveries from the 2 micron all-sky survey (2MASS). KIRKPATRICK J.D., REID I.N., LIEBERT J., et al.
1999ApJ...519..834K 2 12 103 An improved optical spectrum and new model fits of the likely brown dwarf GD 165B. KIRKPATRICK J.D., ALLARD F., BIDA T., et al.
2000ARA&A..38..485B 50 132 Observations of brown dwarfs. BASRI G.
2013ApJ...772...79A 289       D     X C       7 138 267 A near-infrared spectroscopic study of young field ultracool dwarfs. ALLERS K.N. and LIU M.C.
2014ApJ...783..121G viz 16       D               2 213 242 BANYAN. II. Very low mass and substellar candidate members to nearby, young kinematic groups with previously known signs of youth. GAGNE J., LAFRENIERE D., DOYON R., et al.
2015MNRAS.453.2378M 119           X   F     2 29 7 Discovery of a low-mass companion to the F7V star HD 984. MESHKAT T., BONNEFOY M., MAMAJEK E.E., et al.
2017AJ....153..190J 81             C       1 26 6 Integral field spectroscopy of the low-mass companion HD 984 B with the Gemini Planet Imager. JOHNSON-GROH M., MAROIS C., DE ROSA R.J., et al.
2019AJ....157..234S viz 17       D               3 355 40 ACRONYM. III. Radial velocities for 336 candidate young low-mass stars in the solar neighborhood, including 77 newly confirmed young moving group members. SCHNEIDER A.C., SHKOLNIK E.L., ALLERS K.N., 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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