TITLE: GCN CIRCULAR NUMBER: 43815 SUBJECT: GRB 260223A: SVOM/GRM observation DATE: 26/02/23 17:10:56 GMT FROM: Chenwei Wang at IHEP <cwwang@ihep.ac.cn> SVOM/GRM team: Yue Wang, Chen-Wei Wang, Shi-Jie Zheng, Yue Huang, Shao-Lin Xiong, Shuang-Nan Zhang (IHEP) SVOM/ECLAIRs team: Nicolas Dagoneau (CEA) Report on behalf of the SVOM team: SVOM/GRM was triggered in-flight by GRB 260223A (SVOM trigger reference: sb26022301) at 2026-02-23T04:11:28.000 (T0), which is also detected by Fermi/GBM (Fermi GBM team, GCN #43808). With the event-by-event data downloaded through the X-band ground station, the GRM light curve shows that this burst consists of multiple pulses with a T90 of 26 +8/-4 s in the 15-5000 keV band. The SVOM/GRM light curve can be found here: https://www.bursthub.cn//admin/static/svgrb260223A.png In addition, the position of this burst, as determined by Fermi/GBM (RA = 110.5, Dec = -29.4, Error = 1.7, GCN #43808), is located at about 96 degrees from the SVOM optical axis, which is outside the ECLAIRs field of view. ECLAIRs was not collecting data at the time of this burst. With this localization, the time-averaged spectrum from T0-23 to T0+15 s is best fitted by a power law function with an exponential high-energy cutoff. The power law index is -1.29 +0.10/-0.11 and the cutoff energy, parameterized as Epeak, is 194 +33/-25 keV. The event fluence (10-1000 keV) in this time interval is (2.27 +0.13/-0.13)E-05 erg/cm^2. The 1s peak spectrum, measured from T0-0 to T0+1 s, if fitted by a power law function with an exponential high-energy cutoff, the power law index is -1.39 +0.10/-0.11 and the cutoff energy, parameterized as Epeak, is 741 +456/-228 keV. The flux (10-1000 keV) in this time interval is (3.03 +0.18/-0.18)E-06 erg/cm^2/s. The localization of GRB 260223A in the 'Amati' relation diagram is shown at: https://www.bursthub.cn//admin/static/svgrb260223A_amati.png The localization of GRB 260223A in the 'Yonetoku' relation diagram is shown at: https://www.bursthub.cn//admin/static/svgrb260223A_yonetoku.png The SVOM/VT ToO has been performed. The Space Variable Objects Monitor (SVOM) is a China-France joint mission led by the Chinese National Space Administration (CNSA, China), National Center for Space Studies (CNES, France) and the Chinese Academy of Sciences (CAS, China), which is dedicated to observing gamma-ray bursts and other transient phenomena in the energetic universe. GRM is developed by the Institute of High Energy Physics (IHEP) of CAS. The SVOM/GRM point of contact for this burst is: Yue Wang (IHEP) (yuewang@ihep.ac.cn) View this GCN Circular online at https://gcn.nasa.gov/circulars/43815. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...