[vsnet-grb-info 18259] Swift-BAT trigger 704327 was due to noise
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Fri Jul 15 01:21:00 JST 2016
TITLE: GCN CIRCULAR
NUMBER: 19707
SUBJECT: Swift-BAT trigger 704327 was due to noise
DATE: 16/07/14 16:20:15 GMT
FROM: Scott Barthelmy at NASA/GSFC <scott at lheamail.gsfc.nasa.gov>
T. Sakamoto (AGU), S. D. Barthelmy (GSFC), A, Breeveld (UCL-MSSL),
J. R. Cummings (GSFC/UMBC), N. Gehrels (GSFC), H. A. Krimm (GSFC/USRA),
A. Y. Lien (GSFC/UMBC), C. B. Markwardt (GSFC), D. M. Palmer (LANL),
B. Sbarufatti (INAF-OAB/PSU), M. Stamatikos (OSU), B. Sbarufatti ((INAF-OAB/PSU)),
T. N. Ukwatta (LANL) (i.e. the Swift-BAT team):
Using the full BAT data set from T-240 to T+962 sec from recent telemetry downlinks,
we report that trigger #704327 was due to a noise fluctuation in the image domain.
The BAT ground analysis shows the image significance has dropped to 3.2 sigma.
No obvious emission is seen in the mask-weighted light curve.
We have analyzed 607 s of XRT data, from T+116 s to T+723 s. No source is detected
inside the BAT error circle, down to a 3-sigma upper limit of 2.7E-2 counts/s.
The Swift/UVOT began settled observations of the field 113 s after the BAT
trigger. No optical afterglow consistent with the BAT position
is detected in the initial UVOT exposures.
Therefore, we believe this trigger is due to a noise fluctuation.
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