  Tracking the thermal evolution of plasmas, characterized by an
n-distribution, using numerical simulations, requires the determination of the
emission spectra and of the radiative losses due to free-free emission from the
correspond- ing temperature averaged and total Gaunt factors. Detailed
calculations of the latter are presented, associated to n-distributed electrons
with the parameter n ranging from 1 (corresponding to the Maxwell-Boltzmann
distribu- tion) to 100. The temperature averaged and total Gaunt factors, with
decreasing n tend to those obtained with the Maxwell-Boltzmann distribution.
Radiative losses due to free-free emission in a plasma evolving under
collisional ionization equilibrium conditions and composed by H, He, C, N, O,
Ne, Mg, Si, S, and Fe ions, are presented. These losses decrease with the
decrease in the parameter n reaching a minimum when n = 1, and, thus converging
to the losses of a thermal plasma.
  Tables of the thermal averaged and total Gaunt factors calculated for n
distributions and a wide range electron and photon energies are presented.
