{
  "bibcode": "2013GCN.14601....1Y",
  "body": "T. Yasuda, M. Tashiro, Y. Terada, Y. Ishida, H. Ueno, S. Sugimoto\n(Saitama U.), M. Ohno, K. Takaki, T. Kawano, R. Nakamura, S. Furui,\nY. Fukazawa (Hiroshima U.), M. Yamauchi, N. Ohmori, M. Akiyama\n(Univ. of Miyazaki), K. Yamaoka (Nagoya U.),  S. Sugita (Ehime U.),\nY. E. Nakagawa, M. Kokubun, T. Takahashi (ISAS/JAXA), W. Iwakiri\n(RIKEN), Y. Hanabata (ICRR), Y. Urata (NCU), K. Nakazawa,\nK. Makishima (Univ. of Tokyo) on behalf of the Suzaku WAM team, report:\n\n\nThe bright, long GRB 130504C (GCN 14574; Fermi-LAT detection : Kocevski\net al.) triggered the Suzaku Wide-band  All-sky Monitor (WAM) which\ncovers an energy range of 50 keV - 5 MeV at 23:29:00.540 UT (=T0).\n\nThe observed light curve shows a multi-peaked structure starting at T0-9\ns, ending at T0+110 s with a duration (T90) of about 67 seconds.\nThe fluence in 100 - 1000 keV was 9.11 (+0.14/-0.51) x10^-5 erg/cm^2.\nThe 1-s peak flux measured from T0+ 27 s was\n15.9 (+0.3/-4.0) photons/cm^2/s in the same energy range.\n\nPreliminary result shows that the time-averaged spectrum from\nT0-9 s to T0+110 s is well fitted by a GRB Band model as follows.\nthe low-energy photon index alpha:  -1.59 (+0.17/-0.12),\nthe high-energy photon index beta: -2.43 (+0.17/-0.33),\nand the peak energy Epeak: 845 (+227/-159) keV (chi^2/d.o.f = 77.0/50).\n\nDue to the brightness of this burst, a 1% systematic error was added for\nlow energy channels.\nAll the quoted errors are at statistical 90% confidence level.\n\nThe light curves for this burst are available at:\nhttp://www.astro.isas.jaxa.jp/suzaku/HXD-WAM/WAM-GRB/grb/trig/grb_table.html",
  "circularId": 14601,
  "createdOn": 1367987461000,
  "email": "tashiro@phy.saitama-u.ac.jp",
  "subject": "GRB 130504C: Suzaku WAM observation of the prompt emission",
  "submitter": "Makoto Tashiro at Saitama U/Swift  <tashiro@phy.saitama-u.ac.jp>",
  "eventId": "GRB 130504C"
}