CTAO simulations show it can constrain IGMF strengths up to 10^{-15} G for GRB-like sources, with LST-1 observations of GRB 221009A favoring 3×10^{-17} G.
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Intergalactic Magnetic Field constraints from detected very high-energy Gamma-Ray Bursts using the Cherenkov Telescope Array Observatory
CTAO simulations show it can constrain IGMF strengths up to 10^{-15} G for GRB-like sources, with LST-1 observations of GRB 221009A favoring 3×10^{-17} G.