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We describe upgrades to a numerical code which computes synchrotron andinverse-Compton emission from relativistic plasma including full polarization.The introduced upgrades concern scattering kernel which is now capable ofscattering the polarized and unpolarized photons on non-thermal population ofelectrons. We describe the scheme to approach this problem and we test thenumerical code against known analytic solution. Finally, using the upgradedcode, we predict polarization of light that is scattered off sub-relativisticthermal or relativistic thermal and non-thermal free electrons. The upgradedcode enables more realistic simulations of emissions from plasma jetsassociated with accreting compact objects.

Polarization-sensitive Compton scattering by accelerated electrons