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Astronomical observations with the FAUST telescopeThe far-ultraviolet space telescope (FAUST) was flown on Spacelab 1 to provide wide-field imaging in the wavelength range 1300 to 1800 angstroms.Most of the developed film showed high levels of background exposure. Frames with a lower background included exposures of the Cygnus Loop supernova remnant and an exposure in the direction of the galaxy cluster Abell 2634. Several exposures will be used in a search for hot white dwarf stars.
Document ID
19840057500
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Bixler, J.
(California Univ. Berkeley, CA, United States)
Bowyer, S.
(California Univ. Berkeley, CA, United States)
Malina, R.
(California Univ. Berkeley, CA, United States)
Martin, C.
(California Univ. Berkeley, CA, United States)
Lampton, M.
(California, University Berkeley, CA, United States)
Deharveng, J. M.
(California Univ. Berkeley, CA, United States)
Courtes, G.
(CNRS Laboratoire d'Astronomie Spatiale, Marseille, France)
Date Acquired
August 12, 2013
Publication Date
July 13, 1984
Publication Information
Publication: Science
Volume: 225
ISSN: 0036-8075
Subject Category
Astronomy
Accession Number
84A40287
Funding Number(s)
CONTRACT_GRANT: NAS8-32577
Distribution Limits
Public
Copyright
Other

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