A census of quasar-intrinsic absorption in the Hubble Space Telescope archive: systems from high-resolution echelle spectra
A Population of Weak Metal-Line Absorbers Surrounding the Milky Way
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 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
Discovery of an Ultraviolet Counterpart to an Ultrafast X-Ray Outflow in the Quasar PG 1211+143
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 Chemical Properties of Low-redshift QSOs
The Hot Intergalactic Medium-Galaxy Connection: Two Strong O VI Absorbers in the Sight Line toward PG 1211+143
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
Temporal Coverage
2002-02-04T21:54:50Z/2002-02-08T23:22:15Z
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, Shull et al., 2007, 'Metallicity and D/H abundance in Low-z LyAlpha Absorbers towards PG 1211+143', 1.0, European Space Agency, https://doi.org/10.57780/esa-k2rni6o