Far ultraviolet astronomy using the FAUST telescope

Details Far ultraviolet astronomy using the FAUST telescope Far ultraviolet astronomy using the FAUST telescope

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981splb.reptr....b&link_type=abstract

In NASA. Marshall Space Flight Center Spacelab Mission 1 Expt. Descriptions 3 p (SEE N82-18234 09-12)

Astronomy and Astrophysics

Astronomy

Astronomical Observatories, Celestial Bodies, Spaceborne Telescopes, Ultraviolet Astronomy, Far Ultraviolet Radiation, Galaxies, Optical Equipment, Spaceborne Experiments, Spacelab Payloads, Ultraviolet Telescopes

Scientific paper

The Far Ultraviolet Space Telescope (FAUST) a compact, wide field-of-view, far ultraviolet instrument designed for astronomical observations of extended and point sources is discussed. The design and application of the instrument are described. The prime objective is to observe faint astronomical sources with sensitivities higher than previously available. Scientific programs will include: (1) a search for ultraviolet stars which are predicted to exist at the stage of evolution prior to the final death of a star; (2) observations of galaxies and quasars; and (3) joint programs with other Spacelab 1 experiments. The secondary objective is to verify the suitability of the Spacelab as a platform for far ultraviolet astronomy: data will be provided on the ultraviolet background levels due to astronomical, terrestrial, and spacecraft generated sources; the levels of contaminants which affect ultraviolet instruments; and the capability of the Orbiter for stable pointing at celestial sources for useful periods of time.

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