WISEA J033515.07+431044.7 , the SIMBAD biblio

WISEA J033515.07+431044.7 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST23:37:31


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Title First 3 Authors
2012ApJ...753..156K viz 15       D               1 485 288 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.
2012AJ....144..148G viz 15       D               1 188 15 Spitzer photometry of WISE-selected brown dwarf and hyper-luminous infrared galaxy candidates. GRIFFITH R.L., KIRKPATRICK J.D., EISENHARDT P.R.M., et al.
2013ApJS..205....6M viz 15       D               1 307 112 A study of the diverse T dwarf population revealed by WISE. MACE G.N., KIRKPATRICK J.D., CUSHING M.C., et al.
2014ApJ...783...68B 557       D     X C       14 27 47 WISE y dwarfs as probes of the brown dwarf-exoplanet connection. BEICHMAN C., GELINO C.R., KIRKPATRICK J.D., et al.
2014yCat.5144....0M viz 15       D               1 103 ~ Investigating low-mass binary stars and brown dwarfs with near-infrared spectroscopy (Thesis, University of California, Los Angeles (2014)). MACE G.N.
2014ApJ...796...39T 15       D               1 63 38 The luminosities of the coldest brown dwarfs. TINNEY C.G., FAHERTY J.K., KIRKPATRICK J.D., et al.
2015ApJ...799...37L 133       D     X         4 34 32 Near-infrared photometry of Y dwarfs: low ammonia abundance and the onset of water clouds. LEGGETT S.K., MORLEY C.V., MARLEY M.S., et al.
2015ApJ...803..102D 39           X         1 22 19 Discovery of a low-luminosity, tight substellar binary at the T/Y transition. DUPUY T.J., LIU M.C. and LEGGETT S.K.
2015ApJ...804...92S 212       D     X         6 29 58 Hubble Space Telescope spectroscopy of brown dwarfs discovered with the wide-field infrared survey explorer. SCHNEIDER A.C., CUSHING M.C., KIRKPATRICK J.D., et al.
2017ApJ...838...73M viz 16       D               1 233 40 Surface gravities for 228 M, L, and T dwarfs in the NIRSPEC Brown Dwarf Spectroscopic Survey. MARTIN E.C., MACE G.N., McLEAN I.S., et al.
2017ApJ...842..118L viz 135       D     X         4 107 55 The Y-type brown dwarfs: estimates of mass and age from new astrometry, homogenized photometry, and near-infrared spectroscopy. LEGGETT S.K., TREMBLIN P., ESPLIN T.L., et al.
2018MNRAS.479.2702F 377       D     X C F     8 56 46 Constraining the multiplicity statistics of the coolest brown dwarfs: binary fraction continues to decrease with spectral type. FONTANIVE C., BILLER B., BONAVITA M., et al.
2019ApJS..240...19K viz 16       D               2 240 80 Preliminary trigonometric parallaxes of 184 late-T and Y dwarfs and an analysis of the field substellar mass function into the "planetary" mass regime. KIRKPATRICK J.D., MARTIN E.C., SMART R.L., et al.
2019AJ....157..101M viz 16       D               2 93 30 Cloud Atlas: Hubble Space Telescope near-infrared spectral library of brown dwarfs, planetary-mass companions, and hot Jupiters. MANJAVACAS E., APAI D., ZHOU Y., et al.
2019ApJ...877...24Z 222       D     X         6 14 46 A uniform retrieval analysis of ultra-cool dwarfs. III. Properties of Y- dwarfs. ZALESKY J.A., LINE M.R., SCHNEIDER A.C., et al.
2021ApJS..253....7K viz 17       D               3 726 76 The field substellar mass function based on the full-sky 20 pc census of 525 L, T, and Y dwarfs. KIRKPATRICK J.D., GELINO C.R., FAHERTY J.K., et al.
2023A&A...670A..19G viz 17       D               1 5915 6 The Fifth Catalogue of Nearby Stars (CNS5). GOLOVIN A., REFFERT S., JUST A., et al.
2023AJ....165..232B 17       D               1 146 1 Long-term 4.6 μm Variability in Brown Dwarfs and a New Technique for Identifying Brown Dwarf Binary Candidates. BROOKS H., KIRKPATRICK J.D., MEISNER A.M., et al.
2023AJ....166..103S viz 17       D               1 997 ~ Astrometry and Photometry for ≈1000 L, T, and Y Dwarfs from the UKIRT Hemisphere Survey. SCHNEIDER A.C., MUNN J.A., VRBA F.J., et al.
2025ApJ...991..193L 19       D               2 65 ~ Exploration of the Near-infrared Colors of Cold Y Dwarfs from the Ground and Space. LEGGETT S.K., PHILLIPS M.W. and TREMBLIN P.

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