GCN Circular 22399
Subject
GRB 180204A: MITSuME Okayama optical upper limits
Date
2018-02-07T08:04:10Z (7 years ago)
From
Kotaro Morita at Tokyo Tech <morita@hp.phys.titech.ac.jp>
K. Morita, R. Itoh, K. L. Murata, T. Yoshii, Y. Tachibana, S. Harita, T.
Ozawa, H. Mamiya, K. Shiraishi, Y. Yatsu, and N. Kawai (Tokyo Tech)
report on behalf of the MITSuME collaboration:
We searched for the optical counterpart of GRB 180204A (K. L. Page et al.,
GCN Circular #22375) with the optical three color (g', Rc, and Ic) CCD
cameras attached to the MITSuME 50 cm telescope of Okayama Astrophysical
Observatory, Japan.
The observation started on 2018-02-04 9:37:11.83 UT. We did not find any
new point source within the XRT circle (J. P. Osborne et al., GCN Circular
#22377) in all three bands.
We obtained following limits for the magnitudes.
T0+[h] MID-UT T-EXP[sec] g' Rc Ic
------------------------------------------------------------
-------------------------------------------
~7.0 9:48:54 1140 >17.5 >17.4 >17.0
------------------------------------------------------------
-------------------------------------------
T0+ : Elapsed time after the burst
T-EXP: Total Exposure time
We used GSC2.3 catalog for flux calibration