A Relation between Supermassive Black Hole Mass and Quasar Metallicity?
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
Deep imaging of Q2112+059: A bright host galaxy but no DLA absorber
Dramatic X-Ray Spectral Variability of the Broad Absorption Line Quasar PG 2112+059
Emission Line Properties of Active Galactic Nuclei from a Post-COSTAR Hubble Space Telescope Faint Object Spectrograph Spectral Atlas
Heavy X-Ray Absorption in Soft X-Ray-weak Active Galactic Nuclei
Low- and High-Ionization Absorption Properties of Mg II Absorption-selected Galaxies at Intermediate Redshifts. I. General Properties
The Extreme Ultraviolet Variability of Quasars
The Nondamped Nature of 12 Low-Redshift Damped Lya Candidate Systems
The Population of Weak Mg II Absorbers. II. The Properties of Single-Cloud Systems
Instrument
FOS/BL, FOS/RD, HRS/1
Temporal Coverage
1995-07-11T17:46:59Z/1995-09-11T08:00:07Z
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, Lanzetta comma Kenneth M., 1996, 'DAMPED LYMAN-ALPHA ABSORPTION LINES FROM MODERATE-REDSHIFT GALAXIES', 1.0, European Space Agency, https://doi.org/10.5270/esa-3vem7nr