Cluster Population Pipeline

This site contains the data and source code required for the Bayesian forward-modelling method to derive the demographics of star cluster populations described in Krumholz, Adamo, Fumagalli, & Calzetti (2018). It consists of two parts:

The source code for the pipeline is available from bitbucket
The libraries required to for the analysis are available at http://www.mso.anu.edu.au/~krumholz/data/kafc18.tgz (warning: 23 GB download)

To run this code you will also need to Download SLUG, and to have a copy of Daniel Foreman-Mackey's emcee package.

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