Home

Welcome to the MADHAT wiki!

MADHAT is a numerical tool that implements a Fermi-LAT data-driven and model-independent analysis of gamma-ray emission due to dark matter annihilation/decay or other nonstandard or unknown astrophysics in dwarf galaxies.

If you use MADHAT, please cite the following papers:
[1] K. Boddy, D. Kumar, D. Marfatia, and P. Sandick, Phys.Rev. D97 (2018) no.9, 095031, https://arxiv.org/abs/1802.03826
[2] K. Boddy, S. Hill, J. Kumar, P. Sandick, and B. Shams Es Haghi, in prep.

This wiki contains the following pages:
Required Libraries
Make Instructions
Running MADHAT
Output Options and Formatting
Input File Formatting
Testing Your Installation