GCN Circular 26019
Subject
GRB191016A: MITSuME Okayama optical observation
Date
2019-10-17T11:15:15Z (5 years ago)
From
Sayaka Toma at Tokyo Institute of Technology <toma@hp.phys.titech.ac.jp>
S. Toma, M. Niwano, R. Adachi, K. L. Murata, M. Oeda, K.Shiraishi, K. Iida,
F. Ogawa, R. Hosokawa, Y. Yatsu, and N. Kawai (TokyoTech)
report on behalf of the MITSuME collaboration:
We searched for the optical counterpart of GRB 191016A (J.D. Gropp et
al., GCN Circular #26008) with the optical three color (g', Rc, and
Ic) CCD cameras
attached to the MITSuME 50 cm telescope of Okayama
Astrophysical Observatory, Okayama, Japan.
The observation started on 09:37:49.50 UT which corresponds to
5.5 hours after the trigger.
We detected the point source at the position consistent with the
afterglow detected previously (Alan M. Watson et al. GCN #26010).
The measured magnitudes and 3-sigma limit are listed as follows.
T0+[sec] MID-UT T-EXP[sec] g' Rc Ic
���������������������������������������������������������������������������������������������������������������������������������������������������������
20794 13:31:46 20040 19.5+/-0.4
> 19.0 18.6+/-0.2
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T0+ : Elapsed time after the burst
T-EXP: Total Exposure time
We used GSC2.3 and UCAC4 catalog for flux calibration.
The magnitudes are expressed in the Vega system.