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Possible precursor to the SGR1900+14 giant burst
Hurley et al.
SOURCE: GCN
TITLE: GCN GRB OBSERVATION REPORT
NUMBER: 1045
SUBJECT: Possible precursor to the SGR1900+14 giant burst
DATE: 01/04/20 19:48:21 GMT
FROM: Kevin Hurley at UCBerkeley/SSL <khurley@sunspot.ssl.berkeley.edu>

K. Hurley, on behalf of the Ulysses GRB team; E. Montanari, C. Guidorzi, F. Frontera, and M. Feroci on behalf of the BeppoSAX GRBM team, report:

We have identified a likely precursor to the giant flare from SGR1900+14 (GCN 1041, GCN 1043) in the Ulysses data. This event occurred on April 17, 2001, ~42184 s at Ulysses, and if it was indeed from SGR1900+14, its Earth-crossing time would have been ~42332 s. This burst was ~50 s long, and its time history resembles that of the April 18 event, although it is considerably less intense. Its 25-100 keV fluence was ~2.3x10^-5 erg/cm^2, and its peak flux over 0.5 s was ~1.5x10^-6 erg/cm^2 s. Due to a high solar proton background, these numbers are subject to more than the usual uncertainties. As SGR1900+14 was Earth-blocked at BeppoSAX, it did not observe this event, and there is no localization data available.

The time history has been posted at ssl.berkeley.edu/ipn3/010417. Also, we note that the time history of the April 18 event, posted at ssl.berkeley.edu/ipn3/010418, was incorrectly labelled "Counts/ 0.5 s". The label should have read "Counts/Second". A corrected plot has been posted.

Searches are underway through the Ulysses data for more possible events from this source.

...
Cited by 1 message

GRB Observations

GRB_ID OBSDATE (UT) DURATION FLUENCE (erg cm-2) PEAK_FLUX (erg cm-2 s-1) EPEAK (keV) MIN_KEV MAX_KEV UPLIM
2001 Apr 17 11:45:32 50 s 2.3e-5 1.5e-6 25 100 no




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