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Ultraviolet Sky Surveys
Published online by Cambridge University Press: 25 May 2016
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Among all spectral bands, the ultraviolet has long been neglected, despite the advantage of small space experiments: the sky is very dark, thus detection of faint objects does not compete against an enhanced background (O'Connell 1987) and the telescope construction techniques are very similar (at least longward of ∼50 nm) to those of optical astronomy.
- Type
- Part 1. General Sky Survey Reviews
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- Copyright
- Copyright © Kluwer 1998
References
Bowyer, S.
1990 in “The Galactic and Extragalactic Background Radiation” (Bowyer, S. and Leinert, Ch., eds.), Dordrecht: Reidel, p. 171.Google Scholar
Bowyer, S. and Malina, R.F.
1991
“Extreme Ultraviolet Astronomy” (Malina, R.F. and Bowyer, S., eds.), New York: Pergamon Press, p. 397.Google Scholar
Lipovetsky, V.A.
1992 in “Astronomy from Wide-Field Imaging” (MacGillivray, H. T. et al. eds.), Dordrecht: Reidel, p. 3.Google Scholar
Pye, J.P.
1995 in “Astrophysics in the Extreme Ultraviolet”
proceedings of IAU Colloquium no. 152.Google Scholar
Tovmassian, H.M. et al. 1988
Pis'ma v Astron. Zh.
14, 291
(Sov. Astron. Lett. 14, 123).Google Scholar
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