Extensive simulations calibrate the bright-ring to shadow-size relation and quantify uncertainty reduction via 345 GHz observations, geometric constraints, spin-jet alignment, and magnetically arrested accretion flows.
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Prospects for Improving the Theoretical Uncertainty for Tests of General Relativity with the EHT
Extensive simulations calibrate the bright-ring to shadow-size relation and quantify uncertainty reduction via 345 GHz observations, geometric constraints, spin-jet alignment, and magnetically arrested accretion flows.