  We calculate the net extinction of galactic light as a function of
wavelength, inclination, central optical depth, and morphology for simple
galactic geometries using the Hyperion radiative transfer code. Compared to
previous, similar works we tabulate extinction over a much broader range of
galactic properties, and using a much finer grid in the model parameters. We
expect these results to be useful for constructing dust-extinguished spectra
and luminosities of model galaxies and, therefore, for synthetic survey
building. Results are made available as an HDF5 file at
https://doi.org/10.5281/zenodo.1442826
