TITLE: GCN CIRCULAR NUMBER: 22342 SUBJECT: GRB 180113B: Insight-HXMT/HE observation DATE: 18/01/15 14:30:16 GMT FROM: Shaolin Xiong at IHEP C. K. Li, S. L. Xiong, X. B. Li, C. Z. Liu, X. F. Li, Z. W. Li, Z. Chang, J. L. Zhao, A. M. Zhang, Y. F. Zhang, X. F. Lu, C. L. Zou (IHEP), Y. J. Jin, Z. Zhang (THU), T. P. Li (IHEP/THU),F. J. Lu, L. M. Song, H. Y. Wang, M. Wu, Y. P. Xu, S. N. Zhang (IHEP),report on behalf of the Insight-HXMT team: At 2018-01-13T00:16:00.00 UT (T0), the Insight-HXMT/HE detected GRB 180113B(trigger ID: HEB180113011) in a routine search of the data, which was also triggered by Fermi/GBM (Veres et al. GCN 22329) and INTEGRAL/SPI-ACS. The Insight-HXMT light curve consists of multiple pulses with a duration (T90) of 11.7 s measured from T0+1.06 s. The 1-s peak rate, measured from T0+1.30 s, is 13236.7 cnts/sec. The total counts from this burst is 31306.5 counts. URL_LC: http://www.hxmt.org/images/GRB/HEB180113011_lc.jpg All measurements above are made with the CsI detectors operating in the regular mode with the energy range of about 80-800 keV (record energy). Only gamma-rays with energy greater than about 200 keV can penetrate the spacecraft and leave signals in the CsI detectors installed inside of the telescope. The analysis results presented above are preliminary; final results will be published elsewhere. Insight-HXMT is the first Chinese space X-ray telescope, which was funded jointly by the China National Space Administration (CNSA) and the Chinese Academy of Sciences (CAS). More information about it could be found at: http://www.hxmt.org/index.php/enhome .