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 Transition Temperature Gas in the Galactic Corona
Measuring Turbulence in the Interstellar Medium by Comparing N(H I; Lya) and N(H I; 21 cm)
Probing the chemical composition of the Z < 1 intergalactic medium with observations and simulations
The Last Eight-Billion Years of Intergalactic C IV Evolution
The Low-redshift Intergalactic Medium as Seen in Archival Legacy HST/STIS and FUSE Data
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, STIS/NUV-MAMA
Temporal Coverage
2003-06-30T03:01:16Z/2003-07-04T07:04:05Z
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, Sembach et al., 2004, 'Is the Compact HVC Toward Ton S210 Remnant Debris from the Formation of the Local Group?', 1.0, European Space Agency, https://doi.org/10.5270/esa-x58rlaj
