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A great contribution was given by the GRBM to the IPN, as soon as the
automatic on-line GRB quest became operative, i.e. since April 2000.
A detailed analysis of the GRBM contribution to the IPN before this date
is given in [Hurley, 2000b]: therein, a set of 16 bursts, which had been
previously localized with high accuracy by other experiments,
has been used to test the
agreement of the Ulysses-BeppoSAX annuli with the known positions
and the possibility of constraining error regions derived from
experiments like the WFCs and/or the NFIs aboard BeppoSAX.
The GRBM in the 3rd IPN
Example of a 31.25 ms GRBM light curve used for the IPN: