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We present digital tables for the radiative terms that appear in the energyand momentum equations used to simulate the accretion onto supermassive blackholes (SMBHs) in the center of galaxies. Cooling and heating rates andradiative accelerations are calculated with two different Spectral EnergyDistributions (SEDs). One SED is composed of an accretion disk +[X-ray]-powerlaw, while the other is made of an accretion disk +[Corona]-bremsstrahlung with $T_X=1.16 \times 10^8$ K, where precomputedconditions of adiabatic expansion are included. Quantification of differentphysical mechanisms at operation are presented, showing discrepancies andsimilarities between both SEDs in different ranges of fundamental physicalparameters (i.e., ionization parameter, density, and temperature). With therecent discovery of outflows originating at sub-parsec scales, these tables mayprovide a useful tool to model gas accretion processes onto a SMBH.

IMPETUS: New Cloudy's radiative tables for accretion onto a galaxy black hole