GCN Circular 19937
Subject
GRB 160910A: 15 GHz detection from AMI
Date
2016-09-21T22:42:24Z (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)
We observed the Fermi/LAT GRB 160910A (Racusin et al., GCN 19902) with
the AMI Large Array at 15 GHz on 2016 Sep 12.65, Sep 13.68, Sep 15.67,
and Sep 20.68 (UT) as part of the 4pisky program. We detect the radio
afterglow at the NOT location (Malesani et al., GCN 19908) at flux
densities of 791+/-55 uJy, 1151+/-82 uJy, 840+/-146 uJy, and 462+/-39
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/.