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The XPOSE program computes the exposure of a single point in the sky for
a given time range and up to ten different energy levels. The time range
need not be restricted to a single viewing period. The program
requires user determination of certain parameters such as event class, spectral
index, zenith cutoff angle, and global scale factor. The resulting exposures
are recorded in the output file "xpose.log". The sensitive areas,
livetimes, and exposures for each exposure history file entry within the time
limits are stored to a binary output file.
CGRO SSC
1998-06-29