A balloon-borne instrumentation for cosmic gamma-ray burst detection and measurement

Details A balloon-borne instrumentation for cosmic gamma-ray burst detection and measurement A balloon-borne instrumentation for cosmic gamma-ray burst detection and measurement

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nimpa.226..524v&link_type=abstract

Nuclear Instruments and Methods in Physics Research Section A, Volume 226, Issue 2-3, p. 524-533.

Physics

3

Scientific paper

A wide-field X-ray detector for observations of cosmic gamma-ray bursts has been prepared and launched on a balloon platform from the base of Trapani-Milo (Sicily) in July of 1983. The detector is an imaging type, 40 cm diameter gamma camera, paired with a 1.8 m diameter pseudorandom, 50% open mask, to make up the telescope. The detector works in the energy range between 30 and 600 keV with imaging capabilities up to 300 keV. A description is given of the detector characteristics, main payload electronics and also the supporting packages and subsystems.

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