Abundance Profiles and Kinematics of Damped Lya Absorbing Galaxies at z < 0.651,
A Hubble Space Telescope Study of Lyman Limit Systems: Census and Evolution
A SINFONI integral field spectroscopy survey for galaxy counterparts to damped Lyman a systems - I. New detections and limits for intervening and associated absorbers
Double-damped Lya Absorption: A Possible Large Neutral Hydrogen Gas Filament near Redshift z=1
Imprints of the first billion years: Lyman limit systems at z ~ 5
Magellan LDSS3 emission confirmation of galaxies hosting metal-rich Lyman a absorption systems
Metals and Dust in Intermediate-Redshift Damped Lya Galaxies
New Magellan Inamori Kyocera Echelle Observations of z < 1.5 sub-damped Lyman a systems
On the HI content, dust-to-gas ratio and nature of MgII absorbers
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2002-05-13T01:31:44Z/2004-07-16T13:41:36Z
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, Rao comma Sandhya M., 2007, 'A Large Targeted Survey for z < 1.6 Damped Lyman Alpha Lines in SDSS QSO MgII-FeII Systems', 1.0, European Space Agency, https://doi.org/10.5270/esa-2w6j5of