2MASS J00440332+0228112 , the SIMBAD biblio

2MASS J00440332+0228112 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST17:41:40


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Title First 3 Authors
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.
2017AJ....153..196S 413       D S   X         10 123 16 A 2MASS/AllWISE search for extremely red L dwarfs: the discovery of several likely L type members of β Pic, AB Dor, Tuc-Hor, Argus, and the Hyades. SCHNEIDER A.C., WINDSOR J., CUSHING M.C., et al.
2017AJ....154...69S viz 16       D               2 237 80 All-sky Co-moving Recovery Of Nearby Young Members (ACRONYM). II. The β Pictoris Moving Group. SHKOLNIK E.L., ALLERS K.N., KRAUS A.L., et al.
2017AJ....154..112K viz 334       D S   X         8 206 4 A statistical survey of peculiar L and T dwarfs in SDSS, 2MASS, and WISE. KELLOGG K., METCHEV S., MILES-PAEZ P.A., et al.
2018AJ....156...57D 16       D               1 73 14 The Hawaii Infrared Parallax Program. III. 2MASS J0249-0557 c: a wide planetary-mass companion to a low-mass binary in the β Pic moving group. DUPUY T.J., LIU M.C., ALLERS K.N., et al.
2022ApJ...934..178A viz 17       D               4 277 5 Disentangling the Signatures of Blended-light Atmospheres in L/T Transition Brown Dwarfs. ASHRAF A., BARDALEZ GAGLIUFFI D.C., MANJAVACAS E., et al.
2023ApJ...959...63S 61       D     X         2 177 ~ 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.
2024MNRAS.527.6624L 421       D     X C F     8 98 ~ A near-infrared variability survey of young planetary-mass objects. LIU P., BILLER B.A., VOS J.M., et al.
2024A&A...684A..69G viz 18       D               2 159 ~ Implications of the discovery of AF Lep b The mass-luminosity relation for planets in the β Pic Moving Group and the L-T transition for young companions and free-floating planets. GRATTON R., BONAVITA M., MESA D., et al.

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