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Development of the Far-ultraviolet Imaging Spectrograph on KAISTSAT-4
Published online by Cambridge University Press: 12 April 2016
The Far-ultraviolet IMaging Spectrograph (FIMS) is a small spectrograph optimized for the observations of diffuse hot interstellar medium in far-ultraviolet wavebands (900–1150Å and 1335–1750Å). The instrument is expected to be sensitive to emission line fluxes an order of magnitude fainter than any previous missions. FIMS is currently under development and is scheduled for launch in 2002.
- III. New Trends in Small-Telescope Technology
- International Astronomical Union Colloquium , Volume 183: Small-Telescope Astronomy on Global Scales , 2001 , pp. 113 - 114
- Copyright © Astronomical Society of the Pacific 2001