WISE J014807.25-720258.7 , the SIMBAD biblio

WISE J014807.25-720258.7 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST00:51:14

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2011ApJ...743...50C 511   K   D     X         14 36 281 The discovery of Y dwarfs using data from the Wide-field Infrared Survey Explorer (WISE). CUSHING M.C., KIRKPATRICK J.D., GELINO C.R., et al.
2011ApJS..197...19K viz 15       D               2 573 330 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...745...26B 38           X         1 15 11 Resolved spectroscopy of a brown dwarf binary at the T Dwarf/Y dwarf transition. BURGASSER A.J., GELINO C.R., CUSHING M.C., 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.
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.
2012ApJ...759...60T 16       D               1 21 43 WISE J163940.83-684738.6: a Y dwarf identified by methane imaging. TINNEY C.G., FAHERTY J.K., KIRKPATRICK J.D., et al.
2013ApJ...763..130L 16       D               1 23 46 A comparison of near-infrared photometry and spectra for y dwarfs with a new generation of cool cloudy models. LEGGETT S.K., MORLEY C.V., MARLEY M.S., 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.
2013MNRAS.433.2054S 15       D               1 88 22 NPARSEC: NTT Parallaxes of Southern Extremely Cool objects. Goals, targets, procedures and first results. SMART R.L., TINNEY C.G., BUCCIARELLI B., et al.
2014ApJ...796...39T 364       D     X         10 63 38 The luminosities of the coldest brown dwarfs. TINNEY C.G., FAHERTY J.K., KIRKPATRICK J.D., et al.
2015ApJ...799...37L 78           X         2 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 273           X C       6 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.
2017ApJ...842..118L viz 16       D               6 107 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.
2013Sci...341.1492D 2 33 141 Distances, luminosities, and temperatures of the coldest known substellar objects. DUPUY T.J. and KRAUS A.L.
2018ApJS..236...28T 16       D               6 64 4 New Y- and T dwarfs from WISE identified by methane imaging. TINNEY C.G., KIRKPATRICK J.D., FAHERTY J.K., et al.
2018MNRAS.479.2702F 177       D       C F     5 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               1 240 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.
2021ApJS..253....7K viz 17       D               2 726 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.
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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