[vsnet-grb-info 6087] GRB 080515: Swift detection of a burst
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Thu May 15 15:21:09 JST 2008
TITLE: GCN CIRCULAR
NUMBER: 7721
SUBJECT: GRB 080515: Swift detection of a burst
DATE: 08/05/15 06:19:28 GMT
FROM: David Palmer at LANL <palmer at lanl.gov>
S. T. Holland (CRESST/USRA/GSFC), A. P. Beardmore (U Leicester),
P. A. Evans (U Leicester), E. A. Hoversten (PSU),
H. A. Krimm (CRESST/GSFC/USRA), C. B. Markwardt (CRESST/GSFC/UMD),
P. T. O'Brien (U Leicester), K. L. Page (U Leicester),
D. M. Palmer (LANL) and R. L. C. Starling (U Leicester) report on
behalf of the Swift Team:
At 06:01:13 UT, the Swift Burst Alert Telescope (BAT) triggered and
located GRB 080515 (trigger=311658). Swift could not slew to the burst
due to Sun constraint. The BAT on-board calculated location is
RA, Dec 3.150, +32.599 which is
RA(J2000) = 00h 12m 36s
Dec(J2000) = +32d 35' 57"
with an uncertainty of 3 arcmin (radius, 90% containment, including
systematic uncertainty). The BAT light curve from TDRSS was
truncated by the beginning of a Malindi downlink and
is further complicated as we were coming out of the SAA at the time, but
shows activity from the trigger time to the end of available data
at T+8s, with a peak count rate of ~500 counts/s (15-350 keV).
This burst is only 45.9 degrees from the Sun, so there will be no prompt
XRT or UVOT data. The field will be outside the Swift Sun observing
constraint tomorrow.
Burst Advocate for this burst is S. T. Holland (sholland AT milkyway.gsfc.nasa.gov).
Please contact the BA by email if you require additional information
regarding Swift followup of this burst. In extremely urgent cases, after
trying the Burst Advocate, you can contact the Swift PI by phone (see
Swift TOO web site for information: http://www.swift.psu.edu/too.html.)
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