The Meraxes semi-analytic galaxy formation model.

If you use this code or its results in any publications, please cite Mutch et al. 2016b (MNRAS, 462, 250):

@ARTICLE{2016MNRAS.462..250M,
   author = {{Mutch}, S.~J. and {Geil}, P.~M. and {Poole}, G.~B. and {Angel}, P.~W. and 
	{Duffy}, A.~R. and {Mesinger}, A. and {Wyithe}, J.~S.~B.},
    title = "{Dark-ages reionization and galaxy formation simulation - III. Modelling galaxy formation and the epoch of reionization}",
  journal = {\mnras},
archivePrefix = "arXiv",
   eprint = {1512.00562},
 keywords = {galaxies: formation, galaxies: high redshift, dark ages, reionization, first stars},
     year = 2016,
    month = oct,
   volume = 462,
    pages = {250-276},
      doi = {10.1093/mnras/stw1506},
   adsurl = {http://adsabs.harvard.edu/abs/2016MNRAS.462..250M},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

If you use any of the following features, please also cite the relevant papers:

AGN model : Qin et al. 2017 (arXiv:1703.04895)

Minihalo model : Ventura et al. Subm. (arXiv:2401.07396)

• Simon Mutch (Lead author; The University of Melbourne)
• Paul Geil (The University of Melbourne)
• Yuxiang Qin (The University of Melbourne)
• Hansik Kim (The University of Melbourne)
• Greg Poole (Astronomy Data and Compute Services)
• Yisheng Qiu (The University of Melbourne)
• Brad Greig (The University of Melbourne)
• Emanuele Maria Ventura (The University of Melbourne)

1. Fork the official repository.
2. Make your changes in a new, appropriately named branch (e.g. mutch_starformation or fix_progenitor_order).
   • All git commit messages should loosely follow the standard format outlined here.
   • Ensure your new code is commented enough so that others can understand what it's doing.
3. Issue a pull request to the official repository.