ULAS J004757.40+154641.4 , the SIMBAD biblio

ULAS J004757.40+154641.4 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST18:11:32


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Title First 3 Authors
2013MNRAS.430.1171D viz 15       D               1 101 37 The sub-stellar birth rate from UKIDSS. DAY-JONES A.C., MAROCCO F., PINFIELD D.J., et al.
2014ApJ...794..143B viz 15       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.
2015MNRAS.449.3651M viz 16       D               6 271 33 A large spectroscopic sample of L and T dwarfs from UKIDSS LAS: peculiar objects, binaries, and space density. MAROCCO F., JONES H.R.A., DAY-JONES A.C., et al.
2020ApJ...889..176F viz 16       D               1 189 24 WISE 2150-7520AB: a very low-mass, wide comoving brown dwarf system discovered through the citizen science project Backyard Worlds: Planet 9. FAHERTY J.K., GOODMAN S., CASELDEN D., et al.
2021ApJ...911....7Z 351       D     X         9 63 21 The Hawaii infrared parallax program. V. New T-dwarf members and candidate members of nearby young moving groups. ZHANG Z., LIU M.C., BEST W.M.J., et al.
2021ApJ...918L..25L 17       D               1 71 14 On the detection of exomoons transiting isolated planetary-mass objects. LIMBACH M.A., VOS J.M., WINN J.N., et al.
2024A&A...684A..69G viz 18       D               1 159 ~ 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.
2024A&A...686A..37P viz 18       D               1 71 ~ Spectral characterization of young LT dwarfs. PISCARRETA L., MUZIC K., ALMENDROS-ABAD V., et al.
2025A&A...701A.208P viz 19       D               2 61 ~ X-SHYNE: X-Shooter spectra of young exoplanet analogs II. Presentation and analysis of the full library. PETRUS S., CHAUVIN G., BONNEFOY M., et al.

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