Absorption-Line Systems and Galaxies in Front of the Second-brightest Quasar, PHL 1811
Cloud-by-cloud, multiphase, Bayesian modelling: application to four weak, low-ionization absorbers
Highly Ionized High-Velocity Clouds: Hot Intergalactic Medium or Galactic Halo?
Probing the chemical composition of the Z < 1 intergalactic medium with observations and simulations
Probing the Intergalactic Medium/Galaxy Connection. V. On the Origin of Lya and O VI Absorption at z < 0.2
The Last Eight-Billion Years of Intergalactic C IV Evolution
The Properties of Low Redshift Intergalactic O VI Absorbers Determined from High S/N Observations of 14 QSOs with the Cosmic Origins Spectrograph
The spectral energy distributions of active galactic nuclei
Instrument
STIS, STIS/CCD
Temporal Coverage
2001-08-20T01:50:18Z/2002-02-21T22:28:09Z
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, 'A SNAPshot Survey of Absorption Lines from High Velocity Clouds in the Milky Way', 1.0, European Space Agency, https://doi.org/10.5270/esa-8r2wywz