  The free-free opacity in plasmas is fundamental to our understanding of
energy transport in stellar interiors and for inertial confinement fusion
research. However, theoretical predictions in the challenging dense plasma
regime are conflicting and there is a dearth of accurate experimental data to
allow for direct model validation. Here we present time-resolved transmission
measurements in solid-density Al heated by an XUV free-electron laser. We use a
novel functional optimization approach to extract the temperature-dependent
absorption coefficient directly from an oversampled pool of single-shot
measurements, and find a pronounced enhancement of the opacity as the plasma is
heated to temperatures of order the Fermi energy. Plasma heating and
opacity-enhancement is observed on ultrafast time scales, within the duration
of the femtosecond XUV pulse. We attribute further rises in the opacity on ps
timescales to melt and the formation of warm-dense matter.
