GCN Circular 14892

Y. Ishida, M. Tashiro, Y. Terada, T. Yasuda, H. Ueno, S. Sugimoto
(Saitama U.), M. Ohno, K. Takaki, T. Kawano, R. Nakamura, S. Furui,
Y. Fukazawa (Hiroshima U.), M. Yamauchi, N. Ohmori, M. Akiyama
(Univ. of Miyazaki), K. Yamaoka (Nagoya U.),  S. Sugita (Ehime U.),
Y. E. Nakagawa, M. Kokubun, T. Takahashi (ISAS/JAXA), W. Iwakiri
(RIKEN), Y. Hanabata (ICRR), Y. Urata (NCU), K. Nakazawa,
K. Makishima (Univ. of Tokyo) on behalf of the Suzaku WAM team,
report:

The bright, long GRB 130606B (Fermi-LAT detection: G. Vianello, et al .
14795) triggered the Suzaku Wide-band  All-sky Monitor (WAM) which
covers an energy range of 50 keV - 5 MeV at  UT 11:55:35.360(=T0).

The observed light curve shows a multi-peaked structure starting at
T0-3.5 s, ending at T0+63 s with a duration (T90) of about 43.7 seconds.
The fluence in 100 - 1000 keV was 1.33 (-0.73, +0.02) *10^-4 erg/cm^2.
The 1-s peak flux measured from T0+11.5 s was
20.64 (-4.72, +0.51) photons/cm^2/s in the same energy range.

Preliminary result shows that the time-averaged spectrum from T0-3 s to
T0+63 s is well fitted by a GRB Band model as follows.
the low-energy photon index alpha: -1.24 (-0.31, +0.79),
the high-energy photon index beta: -2.08 (-0.16, +0.11),
and the peak energy Epeak: 619 (-251, +396) keV,
(chi^2/d.o.f = 17.1/13).

Due to the brightness of this burst, a 3% systematic error was added for
low energy channels.
All the quoted errors are at statistical 90% confidence level.

The light curves for this burst are available at:
http://www.astro.isas.jaxa.jp/suzaku/HXD-WAM/WAM-GRB/grb/trig/grb_table.html