GCN Circular 22684
Subject
GRB 180504A: NOT afterglow candidate
Date
2018-05-05T07:05:30Z (7 years ago)
From
Daniele Malesani at Dark Cosmology Centre, Niels Bohr Inst <malesani@dark-cosmology.dk>
D. Malesani (DAWN/NBI and DARK/NBI) and Illa R. Losada (NOT, Nordita,
Stockholm Univ.) report on behalf of a larger collaboration:
We observed the field of GRB 180504A (Lien et al., GCN 22682) with the
Nordic Optical Telescope equipped with the AlFOSC camera. The field has
a bad visibility from La Palma, and observations were carried out at
large airmass (~2) and straddling twilight. The average seeing was 1.5".
Coincident with the UVOT-enhanced position reported by Evans (GCN
22683), we note the presence of a faint source, at a position (J2000;
0.5" error):
RA = 22:04:34.61
Dec = -14:39:30.0
We note that the automatically reported un-enhanced XRT position
(available from http://www.swift.ac.uk/xrt_positions/) is at the time of
writing significantly different from the one quoted in the GCN, and
would not include our afterglow candidate.
Photometry of the candidate against nearby stars from the Pan-STARRS
survey yields r = 22.5 +/- 0.3 (AB) at a mean time 2018 May 5.222 UT
(9.57 hr after the trigger)
Further observations are planned.