Edward Wright
0000-0001-5058-1593
UCLA
56 papers found
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The CatWISE Preliminary Catalog: Motions from WISE and NEOWISE Data
Asteroid Diameters and Albedos from NEOWISE Reactivation Mission Years 4 and 5
Expanding the Y Dwarf Census with Spitzer Follow-up of the Coldest CatWISE Solar Neighborhood Discoveries
Spectral Classification and Ionized Gas Outflows in z ∼ 2 WISE-selected Hot Dust-obscured Galaxies
Improved Infrared Photometry and a Preliminary Parallax Measurement for the Extremely Cold Brown Dwarf CWISEP J144606.62-231717.8
The Contribution of Galaxies to the 3.4 μm Cosmic Infrared Background as Measured Using WISE
An Ongoing Mid-infrared Outburst in the White Dwarf 0145+234: Catching in Action the Tidal Disruption of an Exoasteroid?
CWISEP J193518.59–154620.3: An Extremely Cold Brown Dwarf in the Solar Neighborhood Discovered with CatWISE
Physical Characterization of Active Asteroid (6478) Gault
The Massive and Distant Clusters of WISE Survey. I. Survey Overview and a Catalog of >2000 Galaxy Clusters at z ≃ 1
Preliminary Trigonometric Parallaxes of 184 Late-T and Y Dwarfs and an Analysis of the Field Substellar Mass Function into the “Planetary” Mass Regime
Super-Eddington Accretion in the WISE-selected Extremely Luminous Infrared Galaxy W2246−0526
Y Dwarf Trigonometric Parallaxes from the Spitzer Space Telescope
Galaxy Ellipticity Measurements in the Near-infrared for Weak Lensing
The 2.4 μm Galaxy Luminosity Function as Measured Using WISE. II. Sample Selection
The 2.4 μm Galaxy Luminosity Function as Measured Using WISE. III. Measurement Results
A Secure W2 Detection of WD 0806-661B from CatWISE
Small and Nearby NEOs Observed by NEOWISE During the First Three Years of Survey: Physical Properties
A Family-based Method of Quantifying NEOWISE Diameter Errors
New Y and T Dwarfs from WISE Identified by Methane Imaging
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