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

A compendium of extinction curves for simple galactic geometries