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
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
Highly Ionized High-Velocity Clouds: Hot Intergalactic Medium or Galactic Halo?
HST/STIS Spectroscopy of 3C 273
Measuring Turbulence in the Interstellar Medium by Comparing N(H I; Lya) and N(H I; 21 cm)
Multiwavelength study of the distribution of neutral gas in and around galaxies and groups of galaxies
Probing the Intergalactic Medium/Galaxy Connection. V. On the Origin of Lya and O VI Absorption at z < 0.2
The Heavy-Element Enrichment of Lya Clouds in the Virgo Supercluster
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-redshift Lya forest towards 3C 273
The Low-z Intergalactic Medium. III. H I and Metal Absorbers at z < 0.4
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
Thermal Pressures in the Interstellar Medium away from Stellar Environments
Warm Gas in the Virgo Cluster. I. Distribution of Lya Absorbers
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2000-05-02T07:42:19Z/2000-06-22T05:36:40Z
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, Heap comma Sara Ridgway, 2006, 'Lyman-alpha Absorption in Low-z QSO's', 1.0, European Space Agency, https://doi.org/10.5270/esa-5ymy319