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.
Right panel: normalized fluence distributions ofP 2 andP 5, illustrating that the mock sample repro- duces the prompt-emission properties of GBM-detected GRBs
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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.