NASA NTRS ยท 20060023328
Burst Detector Sensitivity: Past, Present and Future
Abstract
I compare the burst detection sensitivity of CGRO's BATSE, Swift's BAT, the GLAST Burst Monitor (GBM) and EXIST as a function of a burst s spectrum and duration. A detector's overall burst sensitivity depends on its energy sensitivity and set of accumulations times (Delta)t; these two factors shape the detected burst population. For example, relative to BATSE, the BAT s softer energy band decreases the detection rate of short, hard bursts, while the BAT s longer accumulation times increase the detection rate of long, soft bursts. Consequently, Swift is detecting long, low fluence bursts (2-3 x fainter than BATSE).
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Band, David L.. 2005-01-01. Burst Detector Sensitivity: Past, Present and Future. https://ntrs.nasa.gov/citations/20060023328
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