GRB 250930A

The Fermi GBM team reports the detection of a likely LONG GRB

"At 20:59:58.57 UT on 30 September 2025, the Fermi Gamma-ray Burst Monitor (GBM)
triggered and located GRB 250930A (trigger 780958803/250930875).

The on-ground calculated location, using the Fermi GBM trigger data,
is RA = 336.97, Dec = -44.97 (J2000 degrees, equivalent to J2000 22h 27m, -44d 58'),
with a statistical uncertainty of 3.27 degrees.

The angle from the Fermi LAT boresight is 109 degrees.

The skymap can be found here:
https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2025/bn250930875/quicklook/glg_skymap_all_bn250930875.png

The HEALPix FITS file, including the estimated localization systematic, can be found here:
https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2025/bn250930875/quicklook/glg_healpix_all_bn250930875.fit

The GBM light curve can be found here:
https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2025/bn250930875/quicklook/glg_lc_medres34_bn250930875.gif"

SVOM/GRM team: Chen-Wei Wang. Wen-Jun Tan, Yue Huang, Shi-Jie Zheng, Shao-Lin Xiong, Shuang-Nan Zhang (IHEP)

SVOM/ECLAIRs team: Frédéric Daigne (IAP), Frédéric Piron (LUPM), Jean-Luc Atteia (IRAP)

Report on behalf of the SVOM team:

SVOM/GRM was triggered in-flight by a burst GRB 250930A (SVOM trigger reference: sb25093008) at 2025-09-30T21:00:23.000 UTC (T0), which is also detected by Fermi/GBM (TrigNum#780960200). 

With the event-by-event data downloaded through the X-band ground station, the GRM light curve shows that this burst consists of multi-pulses with a T90 of 49 +8/-6 s in the 15-5000 keV band.

The SVOM/GRM light curve can be found here:
https://www.bursthub.cn//admin/static/svgrb250930A.png

In addition, the position of this burst, as determined by Fermi/GBM (RA= 341.57, DEC= -47.95, TrigNum#780958803), is located at about 58 degrees from the SVOM optical axis, which is outside the ECLAIRs field of view, but this burst is still marginally detected by ECLAIRs above 50 keV. 

With this localization, the time-averaged spectrum from T0-37 to T0+24 s is best fitted by a power law function with an exponential high-energy cutoff. The power law index is -1.13 +/-0.14 and the cutoff energy, parameterized as Epeak, is 107 +17/-12 keV. The event fluence (10-1000 keV) in this time interval is (8.58 +0.69/-0.57)E-06 erg/cm^2. 

The localization of GRB 250930A in the 'Amati' relation diagram is shown at: 
https://www.bursthub.cn//admin/static/svgrb250930A_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 point of contact for this burst is: Chen-Wei Wang (IHEP)(cwwang@ihep.ac.cn)