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.
This can be explained by the fact that we are sampling few GRBs compared to the all GRBs detected by GBM, and very bright GRBs are typically less frequent
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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.