Skip to main content
New Announcement Feature, Code of Conduct, Circular Revisions. See news and announcements

GCN Circular 22757

Subject
GRB 180602A: MITSuME Akeno optical upper limits
Date
2018-06-03T09:29:22Z (6 years ago)
From
Katsuhiro L. Murata at Nagoya U <murata@u.phys.nagoya-u.ac.jp>
K. L. Murata, Y. Tachibana, R. Itoh, T. Yoshii, S. Harita, K. Morita, T.
Ozawa, H. Mamiya, K. Shiraishi, K. Iida, M. Oeda, R. Adachi, S. Niwano, Y.
Yatsu, and N. Kawai (Tokyo Tech)
report on behalf of the MITSuME collaboration:

We searched for the field of GRB 180602A (Cenko et al., GCN Circular
#22752) with the optical three color (g', Rc, and Ic) CCD cameras attached
to the MITSuME 50 cm telescope of Akeno Observatory, Yamanashi, Japan.

The observation started on 2018-06-02 11:12:09 UT (~3 hours after the
burst). We did not find any new point source within the enhanced XRT error
circle (Osborne et al., GCN Circular #22753) in all the three bands.


T0+[hour]    MID-UT      T-EXP[sec]    g'       Rc        Ic
------------------------------------------------------------
-------------------------------------------
~3.1        ~12:24       1200     >18.9     >18.3     >18.0
------------------------------------------------------------
-------------------------------------------

T0+ : Elapsed time after the burst
T-EXP: Total Exposure time
We used GSC2.3 catalog for flux calibration.
Looking for U.S. government information and services? Visit USA.gov