A Survey of Far Ultraviolet Spectroscopic Explorer and Hubble Space Telescope Sight Lines through High-Velocity Cloud Complex C
Broad Lya Emission from Three Nearby BL Lacertae Objects
Characterizing Transition Temperature Gas in the Galactic Corona
Cross-correlation of Lyman a absorbers with gas-rich galaxies
High-Velocity Cloud Complex C: Galactic Fuel or Galactic Waste?
Intergalactic Hydrogen Clouds OT Low Redshift: Connections to Voids and Dwarf Galaxies
Linking the power sources of emission-line galaxy nuclei from the highest to the lowest redshifts
Lya Absorption Systems and the Nearby Galaxy Distribution
Metallicity and Ionization in High-Velocity Cloud Complex C
O VI, N V, and C IV in the Galactic Halo. II. Velocity-Resolved Observations with the Hubble Space Telescope and Far Ultraviolet Spectroscopic Explorer
Probing the chemical composition of the Z < 1 intergalactic medium with observations and simulations
The Galaxy Environment of O VI Absorption Systems
The Last Eight-Billion Years of Intergalactic C IV Evolution
The Local LY alpha Forest: Association of Clouds with Superclusters and Voids
The Local Lya Forest. II. Distribution of H I Absorbers,Doppler Widths, and Baryon Content
The Local Lya Forest. I. Observations with the GHRS/G160M on the Hubble Space Telescope
The Low-redshift Intergalactic Medium
The Search for Intergalactic Hydrogen Clouds in Voids
Ultraviolet and Optical Properties of Narrow-Line Seyfert 1 Galaxies
X-Ray Absorption by the Warm-hot Intergalactic Medium in the Hercules Supercluster
Instrument
HRS, HRS/2
Temporal Coverage
1993-02-26T13:46:48Z/1993-09-09T08:21:47Z
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.
