Edward L. Wright

TL;DR: Spitzer 3.6$$5$\mu$m and 4.5$$$m follow-up of 170 candidate extremely cool brown dwarfs newly discovered via the combination of WISE and NEOWISE imaging at 3$-$5$

TL;DR: In this article, the spectral energy distributions of brown dwarfs with decreasing effective temperature were examined. But the spectral properties of the Y dwarfs were not investigated. And the authors also presented the discovery of 6 new late-T dwarfs, updated spectra of two T dwarfs and the reclassification of a new Y dwarf, WISE J033605.04$-$014351.0, based on Keck/NIRSPEC $J$-band spectroscopy.

TL;DR: In this paper, the authors present a preliminary analysis of the images, which provide a characterization of the dust environment at heliocentric distances similar to those planned for the initial spacecraft encounter, but on the outbound leg of its orbit rather than the inbound.

TL;DR: In this article, the authors identify new Y- and T-type brown dwarfs from the WISE All Sky data release using images obtained in filters that divide the traditional near-infrared H and J bands into two halves.

TL;DR: In this paper, the authors presented the results of an extragalactic point source search using the five-year Wilkinson Microwave Anisotropy Probe (WMAP) 41, 61, and 94 GHz (Q, V, and W bands) temperature maps.