  We construct the gravitational dual of a one-parameter class of states of
strongly coupled $SU(N)$ $\mathcal{N}=4$ SYM at infinite $N$ and asymptotic
temperature $T_{\infty}$, on a fixed Schwarzschild black hole background with
temperature $T_{\mathrm{BH}}$. The resulting bulk geometry is of the flowing
type and allow us to measure Hawking radiation at strong coupling. The outgoing
Hawking flux is a function of the dimensionless ratio $\tau\equiv
T_{\infty}/T_{\mathrm{BH}}$ and appears to be non-monotonic in $\tau$. At
present, we have no field theory understanding for this behaviour.
