NASA NTRS ยท 20040031740
Burst Populations and Detector Sensitivity
Abstract
The F(sub T) (peak bolometric photon flux) vs. E(sub p) (peak energy) plane is a powerful tool to compare the burst populations detected by different detectors. Detector sensitivity curves in this plane demonstrate which burst populations the detectors will detect. For example, future CZT-based detectors will show the largest increase in sensitivity for soft bursts, and will be particularly well- suited to study X-ray rich bursts and X-ray Flashes. Identical bursts at different redshifts describe a track in the F(sub T)-E(sub p) plane.
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Band, David L.. 2003-01-01. Burst Populations and Detector Sensitivity. https://ntrs.nasa.gov/citations/20040031740
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