A census of quasar-intrinsic absorption in the Hubble Space Telescope archive: systems from high-resolution echelle spectra
Discovery of a new quadruply lensed QSO: HS 0810+2554 - A brighter twin to PG 1115+080
Metal-enriched halo gas across galaxy overdensities over the last 10 billion years
Observations of radio-quiet quasars at 10-mas resolution by use of gravitational lensing
Spectral shape of the UV ionizing background and O VI absorbers at z ~ 1.5 towards HS 0747+4259
Strange quasar candidates with abnormal astrometric characteristics from Gaia EDR3 and SDSS (SQUAB-II): optical identifications
The evolution of Lyman a absorbers in the redshift range 0.5 < z < 1.9
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
2001-09-06T19:12:49Z/2001-11-11T16:30:30Z
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 comma Dieter, 2002, 'Baryons in intermediate redshift {z > 1} OVI absorbers', 1.0, European Space Agency, https://doi.org/10.5270/esa-ddel7ow
