Frontiers of Space And Ground-Based Astronomy pp 475-486 | Cite as
Integral — Fine Spectroscopy and Fine Imaging of Celestial Gamma-Rays
Abstract
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A wide operational bandwidth (15 keV to 10 MeV, main instruments).
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High resolution spectroscopy from 15 keV to 10 MeV (E/ΔE = 500 at 1 MeV).
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Imaging with 17′ FWHM angular resolution and accurate source positioning (~ 1′) within a field of view of ~ 50 square degrees.
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High sensitivity. Line: 1.5 × 10-6 ph cm-2 s-1; Continuum: 3×l0-8 ph cm-2 s-1 keV-1, at E = 1 MeV, 3σ in 106 s.
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Polarization sensitivity: 10 mCrab, φ ~ degrees, 3σ in 106 s.
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Concurrent monitoring in X-ray (4 keV — 100 keV) and optical (550 nm — 850 nm) bands. This brief article concentrates on an outline description of the instrumental complement of the mission as presented in the INTEGRAL Phase-A report.
Keywords
Angular Resolution Integral Science Bismuth Germanate Continuum Sensitivity Mask ElementPreview
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References
- International Science Working Team. 1993, INTEGRAL: Report on the Phase ‘A’ Study, ESA Document SCI(93)1.Google Scholar