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- W2002079050 abstract "The scientific interest in observing the 900–1200 Å spectral range is based on the fact that this spectral region contains the bulk of the accessible emission of hot objects (T ∼ 10 5 –10 6 K) and the majority of the resonance lines of many astrophysically important atoms and ions. To pursue the pioneering work with Copernicus on bright objects in that spectral range, a high spectral resolution of 3 10 4 should be attained. In addition, to have access to extragalactic targets (i.e. increase the cosmological return of this observatory) a large collecting area is needed. A design based on the use of 1m class grazing incidence telescope is now under study. Instrumentation at its focal plane may include a 3 10 4 resolution spectrograph in the 900–1200 Å spectral range, a 10 3 resolution spectrograph in the 100–300 Å spectral region and a 10 4 resolution spectrograph in the 1200–2000 Å region." @default.
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- W2002079050 date "1986-01-01" @default.
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- W2002079050 title "The Fuse/Lyman observatory" @default.
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- W2002079050 doi "https://doi.org/10.1016/0273-1177(86)90399-6" @default.
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