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 Sub-damped Lya Absorber with Unusual Abundances: Evidence of Gas Recycling in a Low-redshift Galaxy Group
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?
High-resolution ultraviolet spectroscopy of gas in galaxy halos and large-scale structures
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
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
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2001-03-16T10:51:54Z/2002-06-29T23:27:21Z
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, Bowen comma David V., 2006, 'The Metallicity of Gas in the Local Universe: Beyond the Milky Way', 1.0, European Space Agency, https://doi.org/10.5270/esa-8mtvr51
