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
Associated Absorption Lines in the Radio-loud Quasar 3C 351: Far-Ultraviolet Echelle Spectroscopy from the Hubble Space Telescope
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. II. Methods and Models
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
Complex C: A Low-Metallicity, High-Velocity Cloud Plunging into the Milky Way
Cosmic Voids and Void Properties
Halo Mass Dependence of H I and O VI Absorption: Evidence for Differential Kinematics
Measuring Turbulence in the Interstellar Medium by Comparing N(H I; Lya) and N(H I; 21 cm)
Mining circumgalactic baryons in the low-redshift universe
Multiwavelength study of the distribution of neutral gas in and around galaxies and groups of galaxies
Nearby Galaxy Filaments and the Ly-alpha Forest: Confronting Simulations and the UV Background with Observations
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
Relationship between the Metallicity of the Circumgalactic Medium and Galaxy Orientation
The Azimuthal Dependence of Outflows and Accretion Detected Using O VI Absorption
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 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
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, WFPC2, WFPC2/PC
Temporal Coverage
1999-06-27T07:37:36Z/2000-07-25T13:18:53Z
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, Jenkins comma Edward B., 2006, 'PROPERTIES OF THE LYMAN-ALPHA FOREST AND METAL-LINE SYSTEMS AT LOW Z', 1.0, European Space Agency, https://doi.org/10.5270/esa-du2sckd
