About the ability of GRASP to measure diffuse gamma-ray line sources

Details About the ability of GRASP to measure diffuse gamma-ray line sources About the ability of GRASP to measure diffuse gamma-ray line sources

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aipc..170..427d&link_type=abstract

AIP Conference Proceedings, Volume 170, pp. 427-431 (1988).

Astronomy and Astrophysics

Astronomy

1

X- And Gamma-Ray Telescopes And Instrumentation

Scientific paper

The GRASP mission (Gamma-ray Astronomy with Spectroscopy and Positioning) is currently under study as an ESA space astronomy mission to be launched in the mid 90's GRASP is designed as a high quality spectral imager (E/ΔE~=1000 at 1 MeV) with positioning to the arc minute level within a large field of view (~=7°) which operates over a wide spectral range (30 keV-100 Mev) with a 3σ sensitivity of typically 10 mcrab or better over the entire operational range within an observational period of ~=105 seconds. In this paper, we will mainly discuss the capability of the instrument with respect to the study of both point source and diffuse source measurements.

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