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Pearl Sandick edited this page Oct 8, 2019
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4 revisions
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, [https://arxiv.org/abs/1910.02890]