GCN Circular 43111
Subject
GRB 251213A: SVOM/GRM observation
Event
Date
2025-12-15T09:24:16Z (a day ago)
From
Chenwei Wang at IHEP <cwwang@ihep.ac.cn>
Via
Web form
SVOM/GRM team: Chen-Wei Wang, Wen-Jun Tan, Yue Huang, Shi-Jie Zheng, Shao-Lin Xiong, Shuang-Nan Zhang (IHEP)
SVOM/ECLAIRs team: Ulysse Jacob (LUPM)
Report on behalf of the SVOM team:
SVOM/GRM was triggered in-flight by a burst GRB 251213A (SVOM trigger reference: sb25121302) at 2025-12-13T12:30:05.000 UTC (T0), which is also detected by GRID, GECAM-B (Wang et al., GCN#43106) and AstroSat (Harsha K. H. et al., GCN#43108).
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 36.5 +1.0/-1.0 s in the 15-5000 keV band.
The SVOM/GRM light curve can be found here:
https://www.bursthub.cn//admin/static/svgrb251213A.png
In addition, the position of this burst, as determined by GECAM-B (RA= 296.5, DEC= -11.9, ERR=5.6), is located at about 102 degrees from the SVOM optical axis, which is outside the ECLAIRs field of view.
With this localization, the time-averaged spectrum from T0-5 to T0+45 s is best fitted by a power law function with an exponential high-energy cutoff. The power law index is -0.95 +0.10/-0.09 and the cutoff energy, parameterized as Epeak, is 453 +63/-50 keV. The event fluence (10-1000 keV) in this time interval is (5.58 +0.18/-0.19)E-05 erg/cm^2.
The 1s peak spectrum, measured from T0+5.0 to T0+6.0 s, is also best fitted by a power law function with an exponential high-energy cutoff. The power law index is -1.09 +0.14/-0.12 and the cutoff energy, parameterized as Epeak, is 800 +286/-182 keV. The flux (10-1000 keV) in this time interval is (3.31 +0.13/-0.14)E-06 erg/cm^2/s.
The localization of GRB 251213A in the 'Amati' relation diagram is shown at:
https://www.bursthub.cn//admin/static/svgrb251213A_amati.png
And the localization in the 'Yonetoku' relation diagram is shown at:
https://www.bursthub.cn//admin/static/svgrb251213A_yonetoku.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 point of contact for this burst is: Chen-Wei Wang (IHEP)(cwwang@ihep.ac.cn)