A catalogue of absorption lines in eight Hubble Space Telescope/STIS E230M 1.0 < z < 1.7 quasar spectra
A census of quasar-intrinsic absorption in the Hubble Space Telescope archive: systems from high-resolution echelle spectra
A high-resolution study of the evolution of the Lyman alpha forest in the redshift interval 0.9 < z < 1.7
Detection of molecular hydrogen at z = 1.15 toward HE 0515-4414
HE 0515-4414: an unusual sub-damped Ly a system revisited
High-resolution O VI absorption line observations at 1.2 <= z <= 1.7 in the bright QSO HE 0515-4414
Metal-enriched halo gas across galaxy overdensities over the last 10 billion years
Photoionized O VI absorbers toward the bright QSO HE 0515-4414
Probing the intra-group medium of a z = 0.28 galaxy group
The baryon density at z = 0.9-1.9. Tracing the warm-hot intergalactic medium with broad Lyman a absorption
The evolution of Lyman a absorbers in the redshift range 0.5 < z < 1.9
The Last Eight-billion Years of Intergalactic Si IV Evolution
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
Instrument
STIS, STIS/CCD, STIS/NUV-MAMA
Temporal Coverage
2000-01-31T01:49:41Z/2000-02-02T06:04:39Z
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, Reimers et al., 2006, 'UV brightest known intermediate redshift QSO:, A z=1.15 DLA and metals in the Ly Alpha forest', 1.0, European Space Agency, https://doi.org/10.5270/esa-d6ipckp
