GCN Circular 20083
Subject
GRB 161007A: 15 GHz upper limits from AMI
Date
2016-10-20T10:33:59Z (8 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
161007A (D'Elia et al., GCN 20008) 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 Oct 08.05, Oct 09.25, Oct
11.25 and Oct 15.25 (UT) do not reveal any radio source at the XRT
location (Goad et al., GCN 20013), with 3sigma upper limits of 372 uJy,
273 uJy, 333 uJy and 222 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/.