Absorption-selected galaxies trace the low-mass, late-type, star-forming population at z 2-3
ALMA observations of a metal-rich damped Ly a absorber at z = 2.5832: evidence for strong galactic winds in a galaxy group
Characterizing the circum-galactic medium of damped Lyman-a absorbing galaxies
Comprehensive study of a z = 2.35 DLA Galaxy: mass, metallicity, age, morphology and SFR from HST and VLT
On the two high-metallicity DLAs at z = 2.412 and 2.583 towards Q 0918+1636
The impact of satellite trails on Hubble Space Telescope observations
The missing light of the Hubble Ultra Deep Field
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2011-11-09T20:51:38Z/2012-09-15T16:19:47Z
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, Fynbo comma Johan P. U., 2013, 'Detecting the stellar continuum of the galaxy counterparts of three z>2 Damped Lyman-alpha Absorbers', 1.0, European Space Agency, https://doi.org/10.5270/esa-auybo1p