GCN Circular 20116
Subject
GRB 161015A: 15 GHz upper limits from AMI
Date
2016-10-27T21:38:30Z (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)
We observed the Fermi/LAT GRB 161015A (Ohno et al., GCN 20054) with the
AMI Large Array at 15 GHz on 2016 Oct 17.75, Oct 18.73, Oct 20.70, and
Oct 24.65 (UT) as part of the 4pisky program. We do not detect any radio
source at the XRT location (D'Avanzo et al., GCN 20057), with 3sigma
upper limits of 105 uJy, 96 uJy, 147 uJy, and 78 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/.