A Giant Intragroup Nebula Hosting a Damped {Ly}\alpha Absorber at z = 0.313
A Hubble Space Telescope Study of Lyman Limit Systems: Census and Evolution
An improved measurement of the flux distribution of the Lya forest in QSO absorption spectra: the effect of continuum fitting, metal contamination and noise properties
A Relation between Supermassive Black Hole Mass and Quasar Metallicity?
A successful search for intervening 21 cm H I absorption in galaxies at 0.4 < z <1.0 with the Australian square kilometre array pathfinder (ASKAP)
A Uniform Analysis of the Lya Forest at z = 0-5. III. Hubble Space Telescope Faint Object Spectrograph Spectral Atlas
A Uniform Analysis of the Lya Forest at z = 0-5. IV. The Clustering and Evolution of Clouds at z <= 1.7
Chandra Detection of X-Ray Absorption Associated with a Damped Lya System
Classical and MgII-selected damped Lyman a absorbers: impact on OHI at z < 1.7
Damped Lya Gas Metallicities at Redshifts z=0.9-2.0 from Sloan Digital Sky Survey Spectra
Damped Lya Systems at z<1.65: The Expanded Sloan Digital Sky Survey Hubble Space Telescope Sample
Discovery of DampedLya Systems at Redshifts Less than 1.65 and Results on Their Incidence and Cosmological Mass Density
Discovery of z = 0.0912 and z = 0.2212 Damped Lya Absorption-Line Systems Toward the Quasar OI 363: Limits on the Nature of Damped Lya Galaxies
Dust depletion and abundance pattern in damped Lyalpha systems: A sample of Mn and Ti abundances at z < 2.2
Elemental Abundances in Two High Column Density Damped Lya Systems at z < 1.5
Emission Line Properties of Active Galactic Nuclei from a Post-COSTAR Hubble Space Telescope Faint Object Spectrograph Spectral Atlas
Energy Distribution of Individual Quasars from Far-Ultraviolet to X-Rays. I. Intrinsic Ultraviolet Hardness and Dust Opacities
GALEX Far-ultraviolet Color Selection of UV-bright High-redshift Quasars
H i 21 Centimeter Absorption in Two Low-Redshift Damped Lyalpha Systems
Imprints of the first billion years: Lyman limit systems at z ~ 5
Low- and High-Ionization Absorption Properties of Mg II Absorption-selected Galaxies at Intermediate Redshifts. I. General Properties
Metal Abundances at z<1.5: Fresh Clues to the Chemical Enrichment History of Damped Lya Systems
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
Si and Mn Abundances in Damped Lya Systems with Low Dust Content
The evolution of H I and C IV quasar absorption line systems at 1.9 < z < 3.2
The evolution of neutral hydrogen over the past 11 Gyr via H I 21 cm absorption
The Extreme Ultraviolet Variability of Quasars
The H I Content of the Universe Over the Past 10 GYRS
The Population of Weak Mg II Absorbers. II. The Properties of Single-Cloud Systems
The statistical properties of neutral gas at z < 1.65 from UV measurements of Damped Lyman Alpha systems
Instrument
FOS/BL, FOS/RD
Temporal Coverage
1996-05-15T02:54:10Z/1997-01-12T22:40:15Z
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., 1998, 'An Expanded Survey for Study of the LyAlpha Line in QSO MgII Absorption Systems', 1.0, European Space Agency, https://doi.org/10.5270/esa-phmfzwn
