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- W2035127794 abstract "The hard X-ray/soft gamma-ray telescope SIGMA has been successfully operating for more than two years aboard the soviet spacecraft GRANAT. This paper is intended to give a report of the most important technical as well as astrophysical inferences which have been obtained from this mission. From these, the mandatory capabilities of a future mission with their relative priorities can be drawn. The most important ones are (1) simultaneous spectral and imaging capabilities, (2) a wide field of view, and (3) a better sensitivity at 0.5 MeV. A sketch of a possible future satellite experiment fulfilling these requirements is given. It is a spectral imager in the sense that priority is given to the angular resolution in comparison with the spectral resolution. Its field of view (360 degree(s) X 10 degree(s)) enables continuous monitoring of the galactic plane emission, involving no cooling, no mechanics, and a coarse stabilization, it should be very reliable, thus allowing a long duration mission. A highly eccentric orbit of the same type as that of GRANAT would be the most efficient." @default.
- W2035127794 created "2016-06-24" @default.
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- W2035127794 date "1992-10-08" @default.
- W2035127794 modified "2023-10-16" @default.
- W2035127794 title "<title>Main lessons from the SIGMA mission for the future of hard x-ray and soft gamma-ray astronomy</title>" @default.
- W2035127794 doi "https://doi.org/10.1117/12.130677" @default.
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