GCN Circular 12486
Subject
GRB 111016A: optical upper limit
Date
2011-10-23T19:32:31Z (13 years ago)
From
Alexei Pozanenko at IKI, Moscow <apozanen@iki.rssi.ru>
A. Volnova (SAI MSU), E. Litvinenko (UBAI), I. Molotov (KIAM), A. Pozanenko
(IKI) on behalf of larger GRB follow up collaboration report:
We observed the field of the Swift GRB 111016A (Mangano et al., GCN 12439)
with 40-cm telescope ORI-40 of Kitab ISON observatory on Oct. 16 starting on
(UT) 22:07:26. On the stacked image we do not detect any source within the
enhanced XRT error box (Evans et al., GCN 12441). The photometry is based
on the reference star SDSS 101516.54+272642.0 assuming (after recalibration
gri->R) R=17.77:
Tstart UT, T0+, Filter, Exposure, OT, UL (3 sigma)
(mid, d) (s)
22:07:26 0.15905 none 36*60 n/d 19.2