Imaging Large– and Small–Scale Structures of the Far Ultraviolet Background with the Faust Instrument
1990 ◽
Vol 139
◽
pp. 449-452
◽
Keyword(s):
The FAUST telescope is an ultraviolet survey instrument that features a wide 8° field of view, ~1′ angular resolution, and a photon counting detector. Operating in the 1400–1800 Å band, it will be sufficiently sensitive to detect blue mv =17 objects in a single 20 minute night. The instrument is part of the ATLAS-1 shuttle mission, presently scheduled for flight in May 1991. A substantial number of high galactic latitude fields will be investigated, with particular emphasis on studies of the origin of the diffuse far UV background.
1990 ◽
pp. 449-452
◽
2000 ◽
Vol 179
◽
pp. 403-406
2019 ◽
Keyword(s):
2007 ◽
Vol 3
(S247)
◽
pp. 152-157
◽
2009 ◽
Vol 399
(1)
◽
pp. 195-208
◽
Keyword(s):
2018 ◽
Vol 41
◽
pp. 88-96
◽
1980 ◽
Vol 2
(4)
◽
pp. 383-396
◽
Keyword(s):
Keyword(s):