GCN Circular 17567
Subject
GRB 150222A: CrAO optical observation
Date
2015-03-11T21:13:05Z (9 years ago)
From
Alexei Pozanenko at IKI, Moscow <apozanen@iki.rssi.ru>
V. Rumyantsev (CrAO), E. Mazaeva (IKI), A. Volnova (IKI), A. Pozanenko
(IKI) report on behalf of larger GRB follow-up collaboration:
We observed the field of the Swift GRB GRB 150222A (Bernardini et al.,
GCN 17486) with ZTSh telescope of CrAO observatory starting on
Feb. 22 (UT) 23:19:54. We took several images in R-filter of 120 s
exposure under non-optimal weather conditions and mean seeing of 4".
Within enhanced XRT position (Beardmore et al., GCN 17494) we detect a
source in coordinates (J2000) 13 15 08.74 -12 09 07.2 with uncertainty
of 0.4 arcsec in both coordinates. The source position is coincident
with the optical afterglow candidate (Nicuesa Guelbenzu et al., GCNs
17495, GCN 17506). Photometry of the source in a combined image is
following
Date UT start, t-t0 Filter Exp. OT OT_err UL(3sigma)
(mid, days) (s)
2015-02-22 23:19:54 0.2913 R 34*120 23.0 0.3 23.3
The photometry is based on USNO-B1.0 star 0778-0337957 (J2000) 13 15
05.41 -12 08 17.5 assuming R2=15.31
Taking into account photometry of the source r' = 24.6+/-0.3 at ~0.42
days reported by Nicuesa Guelbenzu et al. (GCN 17495) one could suggest
the source is the optical afterglow of GRB 150222A.
The source reported in GCN 17489 (Mazaeva et al) is clearly visible in
coordinates (J2000) 13 15 08.30 -12 08 57.5 with uncertainty of 0.4
arcsec in both coordinates. A photometry of the source is R=22.12+/-0.12.