analytic

This module contains semi-analytic functions for calculating X-ray scattering halo intensities from a power-law distribution of dust grain sizes (see Appendix of Corrales & Paerels, 2015).

When creating a Halo object, one must import from halo. The functions in this module are for Galactic sources only. (Note that galhalo contains functions for numerically integrated solutions).

Functions

Functions within this module modify the Halo object by updating the htype and intensity.