[vsnet-grb-info 21917] GRB 190326A: MITSuME Okayama optical upper limits
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Wed Mar 27 15:53:27 JST 2019
TITLE: GCN CIRCULAR
NUMBER: 24016
SUBJECT: GRB 190326A: MITSuME Okayama optical upper limits
DATE: 19/03/27 06:52:18 GMT
FROM: Masafumi Niwano at Tokyo Institute of Tech <niwano at hp.phys.titech.ac.jp>
M. Niwano, K. L. Murata, R. Itoh, Y. Tachibana,
K. Morita, K. Iida, K. Shiraishi, R. Adachi, M. Oeda, Y. Yatsu,
and N. Kawai (Tokyo Tech) report on behalf of the MITSuME collaboration
We searched for the optical counterpart of
GRB 190326A (M. H. Siegel et al., GCN #24009)
with optical three color (g', Rc, and Ic) cameras attached to the
MITSuME 50 cm
reflector in the Okayama Astrophysical Observatory, Japan.
The observation started at 19:01:19 UT which corresponds to 41151
sec since the trigger.
We did not find any new point source within the Swift BAT error circle
(M. H. Siegel et al., GCN #24009) in all three bands.
The obtained 5 sigma upper limits of the optical counterpart are
summarize below:
T0+[sec] MID-UT T-EXP[sec] g' Rc Ic
-------------------------------------------------------------------------------------------------------
41151 19:33:27 600 >16.8 >16.8 >16.2
-------------------------------------------------------------------------------------------------------
T0+ : Elapsed time after the burst
T-EXP: Total Exposure time
We used UCAC-4 catalog for flux calibration.
More information about the vsnet-grb-info
mailing list