A Study of the Diverse T Dwarf Population Revealed by WISE
A Uniform Retrieval Analysis of Ultra-cool Dwarfs. III. Properties of Y Dwarfs
Further Defining Spectral Type Y and Exploring the Low-mass End of the Field Brown Dwarf Mass Function
Hubble Space Telescope Spectroscopy of Brown Dwarfs Discovered with the Wide-field Infrared Survey Explorer
Near-infrared Spectroscopy of the Y0 WISEP J173835.52+273258.9 and the Y1 WISE J035000.32-565830.2: The Importance of Non-equilibrium Chemistry
Parallaxes and Proper Motions of Ultracool Brown Dwarfs of Spectral Types Y and Late T
The Coldest Brown Dwarf (or Free-floating Planet)?: The Y Dwarf WISE 1828+2650
The Discovery of Y Dwarfs using Data from the Wide-field Infrared Survey Explorer (WISE)
The First Hundred Brown Dwarfs Discovered by the Wide-field Infrared Survey Explorer (WISE)
The missing light of the Hubble Ultra Deep Field
WISE Y Dwarfs as Probes of the Brown Dwarf-Exoplanet Connection
Instrument
WFC3, WFC3/IR
Temporal Coverage
2011-03-14T11:52:51Z/2012-03-04T23:24:58Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Kirkpatrick comma J. Davy, 2013, 'Spitzer Verification of the Coldest WISE?selected Brown Dwarfs', 1.0, European Space Agency, https://doi.org/10.5270/esa-rqtbplb