Event Screening and Selection on Data from the GLAST Balloon Prototype

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

The triggering and data analysis for the GLAST balloon prototype, like that of the GLAST gamma-ray telescope planned for launch in 2006, is much more flexible than was the case for the CGRO/EGRET instrument. Furthermore, the much larger data volume expected from GLAST/LAT precludes the type of manual event review that was done for EGRET data. Thus a great deal of attention must be given to the software ``cuts'' that are used to eliminate the huge background of events produced by charged cosmic rays without reducing significantly the efficiency for gamma-ray detection. Event screening on data from the July 2001 GLAST balloon flight has reduced the background so that a good measurement of the atmospheric gamma rays is possible, and we are starting on the much more difficult problem of pushing the background down to a level that (in the absence of atmospheric secondaries) would allow measurements of cosmic gamma-ray fluxes. We will describe the types of cuts being used, as well as their effects on both the background and the gamma-ray efficiency. The performance of the prototype as an imaging gamma-ray telescope will be demonstrated using Monte Carlo simulations in addition to the balloon data.

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