{
  "bibcode": "2015GCN.18525....1M",
  "body": "T. Masumitsu, H. Negoro, (Nihon U.), N. Kawai (Tokyo Tech), T. Sakamoto (AGU),\nS. Ueno, H. Tomida, S. Nakahira, M. Kimura, M. Ishikawa, Y. E. Nakagawa (JAXA),\nT. Mihara, M. Sugizaki, M. Serino, M. Shidatsu, J. Sugimoto, \nT. Takagi, M. Matsuoka (RIKEN), T. Yoshii, Y. Tachibana (Tokyo Tech), \nA. Yoshida, Y. Kawakubo, H. Ohtsuki (AGU), H. Tsunemi, R. Imatani (Osaka U.), \nM. Nakajima, K. Tanaka (Nihon U.), Y. Ueda, T. Kawamuro, T. Hori (Kyoto U.), \nY. Tsuboi, S. Kanetou (Chuo U.), M. Yamauchi, D. Itoh (Miyazaki U.), \nK. Yamaoka (Nagoya U.), M. Morii (ISM)\nreport on behalf of the MAXI team:\n\nMAXI/GSC performed scanning observations at the region of \nGRB 151027A (Maselli et al. GCN 18478) for 48 sec each \nat the centroid time 03:38:56, 1168 s before the Swift trigger, and \n05:11:32, 4388 s after the Swift trigger.\nNo positive 4-10 keV flux was obtained at the former scan transit\nwith the 3 sigma upper limit of 0.037 photons/cm2/s (~ 31 mCrab).\nAt the latter scan transit, the 4-10 keV flux was 0.0166 +/- 0.0175 \nphotons/cm2/s (~ 14 +/- 15 mCrab). \nThe detection is not significant, but the flux is consistent with \nthe interpolation from the Swift/XRT light curve (V. D'Elica et al. #18509).",
  "circularId": 18525,
  "createdOn": 1446116472000,
  "email": "negoro@phys.cst.nihon-u.ac.jp",
  "subject": "GRB 151027A: MAXI/GSC detection",
  "submitter": "H. Negoro at Nihon U.  <negoro@phys.cst.nihon-u.ac.jp>",
  "eventId": "GRB 151027A"
}