Characterizing the Circumgalactic Medium of Nearby Galaxies with HST/COS and HST/STIS Absorption-line Spectroscopy
Characterizing Transition Temperature Gas in the Galactic Corona
Cosmic Voids and Void Properties
Exploring the Origin and Fate of the Magellanic Stream with Ultraviolet and Optical Absorption
Intrinsic Absorption in the Spectrum of NGC 7469: Simultaneous Chandra, FUSE, and STIS Observations
Measuring Turbulence in the Interstellar Medium by Comparing N(H I; Lya) and N(H I; 21 cm)
Multi-wavelength campaign on NGC 7469. V. Analysis of the HST/COS observations: Super solar metallicity, distance, and trough variation models
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 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
The Rise of an Ionized Wind in the Narrow-line Seyfert 1 Galaxy Mrk 335 Observed by XMM-Newton and HST
Tracking the year-to-year variation in the spectral energy distribution of the narrow-line Seyfert 1 galaxy Mrk 335
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2004-06-21T17:40:45Z/2004-07-01T21:44:44Z
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 comma Kenneth, 2007, 'The Properties of Highly Ionized High Velocity Gas in the Distant Galactic Corona and Local Group', 1.0, European Space Agency, https://doi.org/10.5270/esa-bslwezx
