  Charged, rotating Kerr-Newman black holes represent the most general class of
asymptotically flat black hole solutions to the Einstein-Maxwell equations of
general relativity. Here, we consider a simplified model for the Hawking
radiation produced by a Kerr-Newman black hole by utilising a (1+1)-dimensional
accelerated boundary correspondence (i.e. a flat spacetime mirror trajectory)
in Minkowski spacetime. We derive the particle spectrum and its late-time
thermal distribution which reduces to the Kerr, Reissner-Nordstr\"om and
Schwarzschild cases in the appropriate limits. We also compute the particle
spectrum of the extremal Kerr-Newman system and the total energy emitted.
