TITLE: GCN CIRCULAR NUMBER: 16040 SUBJECT: GRB 140320D: Suzaku WAM observation of the prompt emission DATE: 14/03/29 03:42:36 GMT FROM: Tetsuya Yasuda at Saitama U T. Yasuda, M. Tashiro, Y. Terada, Y. Ishida, H. Ueno, S. Sugimoto S. Koyama, S. Takeda, T. Nagayoshi (Saitama U.), M. Yamauchi, N. Ohmori, M. Akiyama, R. Kinoshita (Univ. of Miyazaki), M. Ohno, K. Takaki, T. Kawano, R. Nakamura, S. Furui, Y. Fukazawa (Hiroshima U.), K. Yamaoka (Nagoya U.), S. Sugita (Ehime U.), W. Iwakiri(RIKEN), Y. Hanabata (ICRR), Y. E. Nakagawa, M. Kokubun, T. Takahashi (ISAS/JAXA), Y. Urata (NCU), K. Nakazawa, K. Makishima (Univ. of Tokyo) on behalf of the Suzaku WAM team, report: The bright, long, and IPN localized GRB 140320D (Hurley et al., GCN 16023; Golenetskii et al., GCN 16025) triggered the Suzaku Wide-band All-sky Monitor (WAM) which covers an energy range of 50 keV - 5 MeV at 20:21:38.309 UT (=T0). The observed light curve shows a multi-peaked structure lasting from T0-5 s to T0+50 s with a duration (T90) of about 22 seconds. The fluence in 100 - 1000 keV was 1.14 (+0.03, -0.04) x10^-4 erg/cm^2. The 1-s peak flux measured from T0+17 s was 35.4 (+0.8, -0.9) photons/cm^2/s in the same energy range. Preliminary result shows that the time-averaged spectrum from T0-10.5 s to T0+49.5 s is well fitted in 200 keV to 5 MeV by a power-law with exponential cutoff model: dN/dE ~ E^{-alpha} * exp(-(2-alpha)*E/Epeak) with alpha 0.99 (+0.12, -0.13), and Epeak 746 (+33, -31) keV (chi^2/d.o.f. = 72.1/48). Fitting by a GRB Band model yields the following parameters: the low-energy photon index alpha: -0.97 (+0.14, -0.13), the high-energy photon index beta: <-3.62, and the peak energy Epeak: 742 (+34, -22) keV (chi^2/d.o.f = 71.4/47). 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 will be available at: http://www.astro.isas.jaxa.jp/suzaku/HXD-WAM/WAM-GRB/grb/trig/grb_table.html