Detecting neutral hydrogen at z 3 in large spectroscopic surveys of quasars
Imprints of the first billion years: Lyman limit systems at z ~ 5
The Advanced Camera for Surveys+Wide Field Camera 3 Survey for Lyman Limit Systems. I. The Data
The beamed jet and quasar core of the distant blazar 4C 71.07
The first ultraviolet quasar-stacked spectrum at z 2.4 from WFC3
The HST/ACS+WFC3 Survey for Lyman Limit Systems. II. Science
Instrument
WFC3, WFC3/UVIS
Temporal Coverage
2009-08-28T09:58:41Z/2010-09-05T03:27:27Z
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, OMeara comma John M., 2011, 'A WFC3 Grism Survey for Lyman limit absorption at z=2', 1.0, European Space Agency, https://doi.org/10.5270/esa-j8siimz