Resummed energy loss in extreme-mass-ratio scattering using critical orbits

Ancillary files for the paper "Resummed energy loss in extreme-mass-ratio scattering using critical orbits." ancillary.m is a Mathematica script containing all of the models of the energy radiated to infinity and down the black hole horizon. UnstableCircularOrbitFluxes.dat contains all of the unstable circular-orbit numerical data used to produce the circular-orbit energy flux models [Eq. (31)] and generate Figure 2. RadiatedEnergyScattering.dat contains all of the 1SF energy radiated to infinity numerical data used to generate Figures 3-7.AbsorbedEnergyScattering.dat contains all of the 1SF energy absorbed by the black hole numerical data used to generate Figure 8.