Explicit analytical formulas convert synchrotron Stokes parameters from the local disk frame to the observer frame around a Schwarzschild black hole, including disk thickness and radial accretion motion.
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Analytical ray-tracing of synchrotron emission around accreting black holes
Explicit analytical formulas convert synchrotron Stokes parameters from the local disk frame to the observer frame around a Schwarzschild black hole, including disk thickness and radial accretion motion.