Observations of local ISM emission with the Berkeley EUV/FUV shuttle telescope

Details Observations of local ISM emission with the Berkeley EUV/FUV shuttle telescope Observations of local ISM emission with the Berkeley EUV/FUV shuttle telescope

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2345..344m&link_type=abstract

In NASA. Goddard Space Flight Center Local Interstellar Medium, No. 81 p 344-347 (SEE N85-15539 06-90)

Astronomy and Astrophysics

Astronomy

3

Background Radiation, Diffuse Radiation, Interstellar Matter, Spaceborne Astronomy, Ultraviolet Astronomy, Ultraviolet Telescopes, Cosmic Rays, Extreme Ultraviolet Radiation, Far Ultraviolet Radiation, Payloads

Scientific paper

The Berkeley Extreme Ultraviolet/Far Ultraviolet Shuttle Telescope (BEST) will be launched on the Space Shuttle in November, 1984, as part of the NASA UVX project. The Berkeley spectrometer will make observations of the cosmic diffuse background in the 600 - 1900 Å band, with a spectral resolution of 10 Å. The sensitivity and spectral resolution of the instrument make it ideal for the study of components of the interstellar medium in the 104 - 106K range.

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