FIRE Spectroscopy of Five Late-type T Dwarfs Discovered with the Wide-field Infrared Survey Explorer
Adam J. Burgasser (UCSD/MIT), Michael C. Cushing (NASA JPL), J. Davy, Kirkpatrick (Caltech/IPAC), Christopher R. Gelino (Caltech/IPAC), Roger L., Griffith (Caltech/IPAC), Dagny L. Looper (U. Hawaii), Christopher Tinney (U., New South Wales), Robert A. Simcoe (MIT)

TL;DR
This study reports the discovery and spectral analysis of five late-type T dwarfs using WISE data, revealing diverse atmospheric properties and providing insights into their temperatures, ages, and compositions.
Contribution
First spectroscopic characterization of five late-type T dwarfs discovered with WISE, including atmospheric modeling and implications for brown dwarf diversity.
Findings
Spectral types range from T5.5 to T8.5.
Effective temperatures between 600 K and 930 K.
Evidence of low gravity and cloudy atmospheres in some objects.
Abstract
We present the discovery of five late-type T dwarfs identified with the Wide-field Infrared Survey Explorer (WISE). Low-resolution near-infrared spectroscopy obtained with the Magellan Folded-port InfraRed Echellette (FIRE) reveal strong water and methane absorption in all five sources, and spectral indices and comparison to spectral templates indicate classifications ranging from T5.5 to T8.5:. The spectrum of the latest-type source, WISE J1812+2721, is an excellent match to that of the T8.5 companion brown dwarf Wolf 940B. WISE-based spectrophotometric distance estimates place these T dwarfs at 12-13 pc from the Sun, assuming they are single. Preliminary fits of the spectral data to the atmosphere models of Saumon & Marley indicate effective temperatures ranging from 600 K to 930 K, both cloudy and cloud-free atmospheres, and a broad range of ages and masses. In particular, two…
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