A census of quasar-intrinsic absorption in the Hubble Space Telescope archive: systems from high-resolution echelle spectra
A High-Resolution Survey of Low-Redshift QSO Absorption Lines: Statistics and Physical Conditions of O VI Absorbers
A Population of Weak Metal-Line Absorbers Surrounding the Milky Way
A Space Telescope Imaging Spectrograph Survey for O VI Absorption Systems at 0.12 < z lesssim 0.5. II. Physical Conditions of the Ionized Gas
A STIS Survey for O VI Absorption Systems at 0.12 < z lesssim 0.5. I. The Statistical Properties of Ionized Gas
A Survey of Analogs to Weak Mg II Absorbers in the Present
A Survey of Far Ultraviolet Spectroscopic Explorer and Hubble Space Telescope Sight Lines through High-Velocity Cloud Complex C
Broad H I Absorbers as Metallicity-independent Tracers of the Warm-Hot Intergalactic Medium
Characterizing the Circumgalactic Medium of Nearby Galaxies with HST/COS and HST/STIS Absorption-line Spectroscopy
Characterizing Transition Temperature Gas in the Galactic Corona
C II Radiative Cooling of the Diffuse Gas in the Milky Way
Cloud-by-cloud multiphase investigation of the circumgalactic medium of low-redshift galaxies
FUSE and STIS Observations of the Warm-hot Intergalactic Medium toward PG 1259+593
Highly Ionized Gas Surrounding High-Velocity Cloud Complex C
Measuring Turbulence in the Interstellar Medium by Comparing N(H I; Lya) and N(H I; 21 cm)
Metallicity and Ionization in High-Velocity Cloud Complex C
Mining circumgalactic baryons in the low-redshift universe
Origins of highly ionized gas in high-velocity clouds
Physical Properties, Baryon Content, and Evolution of the Lya Forest: New Insights from High-Resolution Observations at z <~ 0.4
The Deuterium-to-Hydrogen Ratio in a Low-Metallicity Cloud Falling onto the Milky Way
The Diversity of High- and Intermediate-Velocity Clouds: Complex C versus IV Arch
The Galaxy Environment of O VI Absorption Systems
The history of enrichment of the intergalactic medium using cosmological simulations
The Low-redshift Intergalactic Medium as Seen in Archival Legacy HST/STIS and FUSE Data
The Low-z Intergalactic Medium. III. H I and Metal Absorbers at z < 0.4
The Low-z Intergalactic Medium. II. Lyb, O VI, and C III Forest
The Milky Way halo as a QSO absorption-line system. New results from an HST/STIS absorption-line catalogue of Galactic high-velocity clouds
The Nature of Weak Mg II Absorbing Structures
The origins and evolution of weak low ionization quasar absorption line systems
The Properties of Low Redshift Intergalactic O VI Absorbers Determined from High S/N Observations of 14 QSOs with the Cosmic Origins Spectrograph
Tracing baryons in the warm-hot intergalactic medium with broad Ly a absorption
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2000-10-04T19:00:42Z/2001-12-19T20:32:38Z
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, Tripp comma Todd M., 2006, 'The Nature and Distribution of O VI Absorbers in the Vicinity of Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-ncj0p1d