Next: Background Fit
Up: The GRB Catalog
Previous: GRBM Efficiency with Direction
The automatic estimates of the main features of each single
burst found with the off-line search,
have been checked and refined one by one, after visual
inspection of the light curves and of the background fits
established by the automatic off-line quest.
Once the background fit around each burst has been refined,
the total counts and the peak counts estimates are
re-calculated in each GRBM unit, in both energy bands.
Then, the and durations are computed from
the refined background substracted light curves.
As for the localization technique described
in section , the way the arrival direction
is estimated, when feasible, has been treated extensively
in section .