A C II 158 mm emitter associated with an O I absorber at the end of the reionization epoch
Do the Most Massive Black Holes at z = 2 Grow via Major Mergers?
Infrared emission of z ~ 6 galaxies: AGN imprints
Limits to Rest-frame Ultraviolet Emission from Far-infrared-luminous z 6 Quasar Hosts
Searching for C II Emission from the First Sample of z 6 O I Absorption-associated Galaxies with the Atacama Large Millimeter/submillimeter Array
Instrument
WFC3, WFC3/IR
Temporal Coverage
2013-06-22T18:09:48Z/2014-07-15T03:05:42Z
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, Mechtley comma Matthew, 2015, 'WFC3IR Imaging of UV-Faint z=6 Quasars: Star-Forming Host Galaxies of AGN in the Early Universe', 1.0, European Space Agency, https://doi.org/10.5270/esa-qhp5qfx