Absorption by Highly Ionized Interstellar Gas Along Extragalactic and Galactic Sight Lines
Cross-correlation of Lyman a absorbers with gas-rich galaxies
Discovery of Highly Ionized High-Velocity Clouds toward Markarian 509
Highly Ionized High-Velocity Clouds: Intergalactic Gas in the Local Group or Distant Gas in the Galactic Halo?
Hubble Space Telescope Observations of the Seyfert Galaxy NGC 3783: Discovery of Variable C IV Absorption
Intrinsic Absorption Lines in Seyfert 1 Galaxies. I. Ultraviolet Spectra from the Hubble Space Telescope
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 Galactic Disk and Halo. II. Hot Interstellar Gas toward the Inner Galaxy Star HD 156359
Probing the Galactic Disk and Halo. I. The NGC 3783 Sight Line
STIS Echelle Observations of the Intrinsic UV Absorption in the Seyfert 1 Galaxy NGC 3783
The Galaxy Environment of O VI Absorption Systems
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 Search for Intergalactic Hydrogen Clouds in Voids
Instrument
HRS, HRS/2
Temporal Coverage
1993-02-09T21:51:54Z/1993-05-22T19:45:29Z
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, Savage comma Blair D., 1994, 'HIGHLY IONIZED NITROGEN IN THE GALACTIC HALO', 1.0, European Space Agency, https://doi.org/10.5270/esa-o9wg9pz
