GCN Circular 19950
Subject
GRB 160912A: 15 GHz upper limits from AMI
Date
2016-09-27T16:29:37Z (8 years ago)
From
Kunal Mooley at Oxford U <kunal.mooley@physics.ox.ac.uk>
K. P. Mooley, 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
160912A (Cannizzo et al., GCN 19912) 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 Sep 12.72, Sep 13.81, and
Sep 18.87 (UT) do not reveal any radio source at the XRT location
(Beardmore et al., GCN 19915), with 3sigma upper limits of 147 uJy, 258
uJy, and 102 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/.