The Discovery of Y Dwarfs Using Data from the Wide-field Infrared Survey Explorer (WISE)
Michael C. Cushing, J. Davy Kirkpatrick, Christopher R. Gelino, Roger, L. Griffith, Michael F. Skrutskie, Amanda K. Mainzer, Kenneth A. Marsh,, Charles A. Beichman, Adam J. Burgasser, Lisa A. Prato, Robert A. Simcoe, Mark, S. Marley, D. Saumon, Richard S. Freedman

TL;DR
This paper reports the discovery of seven ultracool brown dwarfs, including the first identified Y dwarfs, using WISE data, and characterizes their spectra and temperatures, extending the classification of substellar objects.
Contribution
The study introduces the first Y dwarf spectral class, redefines T9 as a standard, and provides the coldest spectroscopically confirmed brown dwarfs to date.
Findings
Seven new ultracool brown dwarfs discovered with WISE.
Identification of the Y spectral class and new spectral standards.
Brown dwarfs have effective temperatures between 300 K and 500 K.
Abstract
We present the discovery of seven ultracool brown dwarfs identified with the Wide-field Infrared Survey Explorer (WISE). Near-infrared spectroscopy reveals deep absorption bands of H_2O and CH_4 that indicate all seven of the brown dwarfs have spectral types later than UGPS J072227.51-054031.2, the latest type T dwarf currently known. The spectrum of WISEP J182831.08+265037.8 is distinct in that the heights of the J- and H-band peaks are approximately equal in units of f_lambda, so we identify it as the archetypal member of the Y spectral class. The spectra of at least two of the other brown dwarfs exhibit absorption on the blue wing of the H-band peak that we tentatively ascribe to NH_3. These spectral morphological changes provide a clear transition between the T dwarfs and the Y dwarfs. In order to produce a smooth near-infrared spectral sequence across the T/Y dwarf transition, we…
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