A review of horizon-scale polarized imaging concludes that current EHT data pin down magnetic-field geometry and accretion state more reliably than black-hole spin magnitude or direction.
Efficient generation of jets from magnetically arrested accretion on a rapidly spinning black hole.Monthly Notices of the Royal Astronomical Society2011,418, L79–L83
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Signatures of Black Hole Spin in Horizon-Scale Polarimetry
A review of horizon-scale polarized imaging concludes that current EHT data pin down magnetic-field geometry and accretion state more reliably than black-hole spin magnitude or direction.