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astro-ph.HE2026
GRB 241113B: the first SVOM and EP gamma-ray burst A soft GRB likely seen on-axis, from soft X-rays to gamma-rays
D. Adrien, D. Turpin, T. Maiolino +50
In 2024, two new missions were launched to detect high-energy transients. EP and SVOM aim to observe soft transients from X-ray rich gamma-ray bursts (XRR), X-ray flashes (XRF), to…
astro-ph.HE2026
First Gamma-Ray Burst Observations with SVOM
F. Daigne, D. Turpin, J. -L. Atteia +34
Following its launch on 22 June 2024, the Space-based multi-band astronomical Variable Objects Monitor (SVOM) successfully completed its flight acceptance, commissioning, and scien…
astro-ph.HE2026
XRF 241001A/SN 2024aiiq: A faint soft X-ray transient detected by SVOM with a broad-line type Ic supernova revealed by JWST
B. Schneider, M. Brunet, B. P. Gompertz +61
X-ray flashes (XRFs) are a type of gamma-ray burst (GRB) with prompt emission predominantly below 30 keV and have been poorly detected by previous missions. The advent of the SVOM…