  We present our software to compute gamma-ray emission from inverse-Compton
scattering by cosmic-ray leptons in the heliosphere, as well as in the
photospheres of stars. It includes a formulation of modulation in the
heliosphere, but it can be used for any user-defined modulation model. Profiles
and spectra are output to FITS files in a variety of forms for convenient use.
Also included are general-purpose inverse-Compton routines with other features
like energy loss rates and emissivity for any user-defined target photon and
lepton spectra. The software is publicly available and it is under continuing
development.
