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[ascl:1512.012] DiffuseModel: Modeling the diffuse ultraviolet background

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.

Code site:
https://docs.google.com/document/d/1_CWFC0ed0yhSNsE61q3cI6tGd625R7vdrAfOsg3JdFs/edit https://www.dropbox.com/s/78ium7k3rzh1vag/diffuse_light.zip?dl=0
Used in:
http://adsabs.harvard.edu/abs/2016MNRAS.459.1710M
Bibcode:
2015ascl.soft12012M

Views: 1636

ascl:1512.012
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