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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Radiative cooling cools the dense inner disk of MAD M87* models, yielding a dimmer ring, brighter extended jets, lower total flux, and reduced high-frequency SED emission.
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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.
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Impacts of radiative cooling on the images of a black hole shadow and extended jets in two-temperature GRMHD simulations
Radiative cooling cools the dense inner disk of MAD M87* models, yielding a dimmer ring, brighter extended jets, lower total flux, and reduced high-frequency SED emission.