Welcome to PPMAP’s documentation!¶
PPMAP is a Bayesian Point Process fitting routine for estimating the optical depth and dust properties of astrophysical objects from far-infrared and sub-millimetre observations.
PPMAP was developed by Ken Marsh.
PPMAP was first described in Marsh, et al. 2015, **MNRAS 454**.
PPMAP is currently maintained by Alexander Howard.
PPMAP is undergoing development. If you would like to run PPMAP, please contact Alexander Howard directly at alexander.howard@astro.cf.ac.uk for help in installing and running PPMAP.