PyMF is a pure-Python implementation of several matched filtering image processing techniques. These methods are designed for applications in astronomy and use the flat-sky approximation.

Online documentation is available at pymf.readthedocs.io.

Please cite Erler, Ramos-Ceja, Basu & Bertoldi (2018) if you find this code useful in your research. The BibTeX entry for the paper is:

@ARTICLE{2018arXiv180906446E,
    author = {{Erler}, J. and {Ramos-Ceja}, M.~E. and {Basu}, K. and {Bertoldi}, F.},
     title = "{Introducing constrained matched filters for improved separation of point sources from galaxy clusters}",
   journal = {ArXiv e-prints},
      year = 2018,
    eprint = {1809.06446}
}

Copyright 2020 Jens Erler and contributors.

PyMF is free software made available under the MIT License. For details see the LICENSE file.