model_halo

This module is for modeling scattering halos for Galactic sources (see galhalo) from a dust grain size distribution (astrodust.distlib) and apparent flux spectrum of a point source. It uses HaloDict objects from the halodict module.

Functions

The following two functions are helpers for integrating up the total intensity from a HaloDict object.

The following functions take inputs that will allow us to simulate a scattering halo intensity profile from a set of basic starting parameters.