GCN Circular 10297
Subject
Swift Trigger 381434 is not a GRB
Date
2009-12-29T19:21:53Z (15 years ago)
From
Vanessa Mangano at INAF-IASFPA <vanessa@ifc.inaf.it>
S. D. Barthelmy (GSFC), C. B. Markwardt (GSFC/UMD),
V. Mangano, B. Sbarufatti (INAF-IASF PA), A. Breeveld (MSSL/UCL)
report on behalf the Swift team:
Using the full data set from telemetry downlinks, we report
that Swift Trigger 381434 is due to a cosmic ray shower event
in the BAT instrument. It is not due to a GRB nor any other
astrophysical source. There were two showers ~8 msec apart
which caused the 64msec trigger to fire.
The XRT observed the field of the target starting 68 s after
the trigger. In the initial 7 ks in PC mode no source is
detected within the 3 arcmin BAT error circle down to a limiting
flux of 8 x 10^-14 erg cm^-2 s^-1. Three X-ray sources are
detected with more than 3 sigma significance in the whole XRT
field of view, the brightest one likely associated to
1RXS J050001.1-550121, and the other two unidentified.
All of these sources are further than 4 arcmin from the target position.
The UVOT began settled observations of the field of the target
65 s after the BAT trigger. No new source is detected.
Preliminary 3-sigma upper limits using the UVOT photometric system
(Poole et al. 2008, MNRAS, 383, 627) for the first finding chart
(FC) exposure and subsequent exposures are:
Filter T_start(s) T_stop(s) Exp(s) Mag
white_FC 65 215 147 >21.1
u_FC 277 526 246 >20.4
white 65 1699 411 >21.6
v 606 1748 136 >19.4
b 532 1834 123 >20.3
u 277 1822 363 >20.6
w1 656 1798 136 >19.9
m2 631 1773 136 >19.8
w2 582 1551 117 >20.1
The values quoted above are not corrected for the Galactic extinction
due to the reddening of E(B-V) = 0.02 in the direction of the burst
(Schlegel et al. 1998).
The lack of a bright X-ray/optical counterpart of Trigger 381434 in
prompt observations strengthens the spurious trigger interpretation.