Simulations show that rapid tiling of large localization regions can increase TeV afterglow detections by up to a factor of two for ASTRI and LACT, and yield up to four detections per year with CTAO.
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astro-ph.HE 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
PIC-motivated acceleration models for GRB afterglows predict a GeV-band synchrotron cutoff in low-density short GRBs that current Fermi-LAT data cannot distinguish from the Bohm limit but future observations could.
citing papers explorer
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Detection of TeV emission during early afterglow from poorly localized GRBs with ground based IACTs
Simulations show that rapid tiling of large localization regions can increase TeV afterglow detections by up to a factor of two for ASTRI and LACT, and yield up to four detections per year with CTAO.
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Maximum Energy of Particles Accelerated in Gamma-Ray Burst Afterglow Shocks
PIC-motivated acceleration models for GRB afterglows predict a GeV-band synchrotron cutoff in low-density short GRBs that current Fermi-LAT data cannot distinguish from the Bohm limit but future observations could.