TITLE: GCN CIRCULAR NUMBER: 42219 SUBJECT: GRB 251013B: SVOM/GRM observation DATE: 25/10/13 15:20:56 GMT FROM: Yue Wang m18509381757@163.com
SVOM/GRM team: Yue Wang, Chen-Wei Wang, Wen-Jun Tan, Shi-Jie Zheng, Yue Huang, Shao-Lin Xiong, Shuang-Nan Zhang (IHEP)
SVOM/ECLAIRs team: Stéphane Schanne (CEA), Hui Yang (IRAP)
Report on behalf of the SVOM team:
SVOM/GRM was triggered on-ground by GRB 251013B at 2025-10-13T08:24:36.250 (T0), which is also detected by Fermi/GBM (Fermi GBM Team, GCN #42215).
With the event-by-event data downloaded through the X-band ground station, the GRM light curve shows that this burst consists of mutli-peaks with a T90 of 55 +16/-7 s in the 15-5000 keV band.
The SVOM/GRM light curve can be found here: https://www.bursthub.cn//admin/static/svgrb251013B.png
In addition, the position of this burst, as determined by Fermi/GBM (RA=356.5, DEC=7.5, GCN #42215), is located at about 68.2 degrees from the SVOM optical axis, which is outside the ECLAIRs field of view.
With this localization, the time-averaged spectrum from T0-30 to T0+50 s is best fitted by a power law function with an exponential high-energy cutoff. The power law index is -1.63 +0.10/-0.13 and the cutoff energy, parameterized as Epeak, is 324 +567/-129 keV. The event fluence (10-1000 keV) in this time interval is (1.08 +0.09/-0.11)E-05 erg/cm^2.
The localization of GRB 251013B in the 'Amati' relation diagram is shown at: https://www.bursthub.cn//admin/static/svgrb251013B_amati.png
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)
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