DiffuseModel: Modeling the diffuse ultraviolet background
Abstract: DiffuseModel calculates the scattered radiation from dust scattering in the Milky Way based on stars from the Hipparcos catalog. It uses Monte Carlo to implement multiple scattering and assumes a user-supplied grid for the dust distribution. The output is a FITS file with the diffuse light over the Galaxy. It is intended for use in the UV (900 - 3000 A) but may be modified for use in other wavelengths and galaxies.
Credit: Murthy, Jayant
Site: https://www.dropbox.com/s/78ium7k3rzh1v ... t.zip?dl=0
https://ui.adsabs.harvard.edu/abs/2016MNRAS.459.1710M
Bibcode: 2015ascl.soft12012M
ID: ascl:1512.012