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
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
Cosmic Voids and Void Properties
Far Ultraviolet Spectroscopic Explorer and Space Telescope Imaging Spectrograph Observations of Intervening O VI Absorption Line Systems in the Spectrum of PG 0953+415
Highly Ionized High-Velocity Clouds: Hot Intergalactic Medium or Galactic Halo?
Measuring Turbulence in the Interstellar Medium by Comparing N(H I; Lya) and N(H I; 21 cm)
Multiphase High-Velocity Clouds toward HE 0226-4110 and PG 0953+414
Origins of highly ionized gas in high-velocity clouds
O VI and Multicomponent H I Absorption Associated with a Galaxy Group in the Direction of PG 0953+415: Physical Conditions and Baryonic Content
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
Physical Properties, Baryon Content, and Evolution of the Lya Forest: New Insights from High-Resolution Observations at z <~ 0.4
The Galaxy Environment of O VI Absorption Systems
The history of enrichment of the intergalactic medium using cosmological simulations
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 O VI Absorbers toward PG 0953+415: High-Metallicity, Cosmic-Web Gas Far from Luminous Galaxies
The Properties of Low Redshift Intergalactic O VI Absorbers Determined from High S/N Observations of 14 QSOs with the Cosmic Origins Spectrograph
The Statistical and Physical Properties of the Low-Redshift LYa Forest Observed with the Hubble Space Telescope/STIS
Tracing baryons in the warm-hot intergalactic medium with broad Ly a absorption
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
1998-12-04T18:41:29Z/1998-12-11T19:11:23Z
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 et al., 2006, 'The Relationship Between Lyman-alpha Clouds and Galaxies at z<0.3', 1.0, European Space Agency, https://doi.org/10.5270/esa-ux68tac
