GCN Circular 19533
Subject
GRB 160519A: 15 GHz upper limits from AMI
Date
2016-06-14T16:18:09Z (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), C. Rumsey, 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
160519A (D'Avanzo et al., GCN 19436) 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 19.35, May 20.50, May
22.61, May 26.50, and May 29.49 (UT) do not reveal any variable radio
source within the BAT error circle (Stamatikos et al., GCN 19441), with
3sigma upper limits of 202 uJy, 72 uJy, 84 uJy, 87 uJy, and 87 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/.