GRB 221009A exhibits a TeV spectral downturn explained by neutron-induced synchrotron photons as a prompt emission echo, while intergalactic cascades are suppressed for typical filament magnetic fields above 1 nG.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
years
2026 2verdicts
UNVERDICTED 2roles
background 1polarities
background 1representative citing papers
SVOM-GRM uses three detectors for on-board and MCMC-based ground localization of GRBs in 15-5000 keV, with preliminary results consistent with Fermi/GBM for GRB 240629A.
citing papers explorer
-
Multi-TeV $\gamma$-ray candidates from GRB 221009A: a downturn in the intrinsic $\gamma$-ray spectrum, an echo of the prompt emission phase, and intergalactic electromagnetic cascades
GRB 221009A exhibits a TeV spectral downturn explained by neutron-induced synchrotron photons as a prompt emission echo, while intergalactic cascades are suppressed for typical filament magnetic fields above 1 nG.
-
The trigger and localization system of SVOM-GRM
SVOM-GRM uses three detectors for on-board and MCMC-based ground localization of GRBs in 15-5000 keV, with preliminary results consistent with Fermi/GBM for GRB 240629A.