[vsnet-grb-info 21119] GRB 180715A: 15 GHz upper limits from the AMI Short GRB Program
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Mon Sep 10 15:56:18 JST 2018
TITLE: GCN CIRCULAR
NUMBER: 23217
SUBJECT: GRB 180715A: 15 GHz upper limits from the AMI Short GRB Program
DATE: 18/09/10 06:54:19 GMT
FROM: Kunal Mooley at NRAO,Caltech <kmooley at caltech.edu>
J. Bright (Oxford), K. P. Mooley (NRAO, Caltech; Jansky Fellow), R. P.
Fender (Oxford)
We observed the field of short GRB 180718A (Ukwatta et al., GCN 22947)
with the AMI Large Array at 15 GHz. Our observations on 2018 Jul 16.80,
Jul 17.73, Jul 19.80 and Jul 23.80 (UT) (1.05 d, 1.98 d, 4.05 d and 7.05
d post-burst) does not reveal any potential afterglow candidate
consistent with the BAT location (Ukwatta et al., GCN 22947), and our
3sigma upper limit to the flux density are 137 uJy, 186 uJy, 106 uJy and
146 uJy respectively.
We thank the MRAO staff for scheduling these observations. Results from
the AMI Short GRB program are posted on the AMI-GRB database available
at http://4pisky.org/ami-grb/.
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