GCN Circular 21213
Subject
GRB 170526A: 15 GHz upper limits from AMI
Date
2017-06-07T22:39:09Z (7 years ago)
From
Kunal Mooley at Oxford U <kunal.mooley@physics.ox.ac.uk>
K. P. Mooley (Hintze Fellow, Oxford), T. D. Staley, R. P. Fender
(Oxford), G. E. Anderson (Curtin), T. Cantwell (Manchester), D.
Titterington, S. H. Carey, J. Hickish, Y. C. Perrott, N. Razavi-Ghods,
P. Scott (Cambridge), K. Grainge, A. Scaife (Manchester)
The AMI Large Array robotically triggered on the Swift alert for GRB
170526A (Sbarufatti et al., GCN 21149) as part of the 4pisky program,
and subsequent follow up observations were obtained up to 10 days
post-burst. Our observations at 15 GHz on 2016 May 27.16, May 30.29, May
31.33 and Jun 03.28 (UT) do not reveal any radio source at the XRT
location (Goad et al., GCN 21151), with 3sigma upper limits of 312 uJy,
117 uJy, 96 uJy and 105 uJy respectively.
We thank the AMI staff for scheduling these observations. The AMI-GRB
database is a log of all GRB follow up observations with the AMI, and is
available at http://4pisky.org/ami-grb/.