ULAS J082707.67-020408.2 , the SIMBAD biblio

ULAS J082707.67-020408.2 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST23:13:22


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Title First 3 Authors
2007MNRAS.379.1423L 275       D     X C F     6 17 67 Eight new T4.5-T7.5 dwarfs discovered in the UKIDSS Large Area Survey Data Release 1. LODIEU N., PINFIELD D.J., LEGGETT S.K., et al.
2010ApJ...710.1627L viz 15       D               1 226 150 Mid-infrared photometry of cold brown dwarfs: diversity in age, mass, and metallicity. LEGGETT S.K., BURNINGHAM B., SAUMON D., et al.
2010A&A...524A..38M 16       D               1 16 55 Parallaxes and physical properties of 11 mid-to-late T dwarfs. MAROCCO F., SMART R.L., JONES H.R.A., et al.
2011ApJS..197...19K viz 15       D               1 573 330 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.
2012ApJ...752...56F viz 15       D               1 187 209 The Brown Dwarf Kinematics Project (BDKP). III. Parallaxes for 70 ultracool dwarfs. FAHERTY J.K., BURGASSER A.J., WALTER F.M., et al.
2012A&A...541A.163S 168       D     X C       4 21 13 UKIDSS detections of cool brown dwarfs. Proper motions of 14 known >T5 dwarfs and discovery of three new T5.5-T6 dwarfs. SCHOLZ R.-D., BIHAIN G., SCHNURR O., et al.
2012ApJ...753..156K viz 15       D               2 485 288 Further defining spectral type "Y" and exploring the low-mass end of the field brown dwarf mass function. KIRKPATRICK J.D., GELINO C.R., CUSHING M.C., 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.
2013MNRAS.433..457B viz 15       D               2 176 69 76 T dwarfs from the UKIDSS LAS: benchmarks, kinematics and an updated space density. BURNINGHAM B., CARDOSO C.V., SMITH L., 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.

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