A Survey of Far Ultraviolet Spectroscopic Explorer and Hubble Space Telescope Sight Lines through High-Velocity Cloud Complex C
Characterizing Transition Temperature Gas in the Galactic Corona
Cosmic Voids and Void Properties
Highly Ionized Gas Surrounding High-Velocity Cloud Complex C
High-Velocity Cloud Complex C: Galactic Fuel or Galactic Waste?
Linking the power sources of emission-line galaxy nuclei from the highest to the lowest redshifts
Measuring Turbulence in the Interstellar Medium by Comparing N(H I; Lya) and N(H I; 21 cm)
Metallicity and Ionization in High-Velocity Cloud Complex C
Origins of highly ionized gas in high-velocity clouds
O VI, N V, and C IV in the Galactic Halo. II. Velocity-Resolved Observations with the Hubble Space Telescope and Far Ultraviolet Spectroscopic Explorer
Probing Halos of Galaxies at Very Large Radii Using Background QSOs
Ultraviolet and Optical Properties of Narrow-Line Seyfert 1 Galaxies
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
1998-02-22T15:52:06Z/1999-10-28T22:58:28Z
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, Cote et al., 2006, 'Galaxy Rotation Curves at Large Radius using Ly-alpha Absorption Lines', 1.0, European Space Agency, https://doi.org/10.5270/esa-o8jzlft