GCN Circular 7764
Subject
GRB080521(?): detection of possible burst from BAT slew data and XRT ToO
Date
2008-05-22T23:51:40Z (17 years ago)
From
Antonio Copete at Harvard U <acopete@head.cfa.harvard.edu>
A. Copete, J. Grindlay (Harvard), J. Racusin (PSU)
S.Barthelmy, N. Gehrels (GSFC)
We report on the detection by the BAT Slew Survey (BATSS) of a
possible burst in the slew that began on 05/21/08 at 03:58:02 UT, at
the position:
RA (J2000): 12h 08m 44s
Dec(J2000): +30d 34' 57"
with an uncertainty of 6.4 arcmin (90% confidence). This detection is
an image trigger from 6.4 sigma and 4.8 sigma detections in the
15-150keV and 50-150keV energy bands, respectively. The lightcurve
features a downward sloping profile which suggest a main peak may have
occurred before the slew.
The detection was followed by an XRT ToO observation beginning on
05/22/08 at 15:30 UT. The 4ks observations yielded an uncatalogued X-
ray source within the BATSS error circle at
RA(J2000) = 12h 08m 49.54s
Dec(J2000) = +30d 33' 32.68"
with an uncertainty of 5.4 arcsec (90% confidence), and a count rate
of 0.022+/-0.004 counts/s. No indication of fading was found, however,
which could be due the relatively short exposure time compared to the
delay of more than a day from the initial BAT observation. A follow-up
XRT observation will be scheduled in order to determine fading.