Detailed documentation: https://rpoleski.github.io/MulensModel/
Latest release: 2.23.0 and we're working on further developing the code.
MulensModel can generate a microlensing light curve for a given set of microlensing parameters, fit that light curve to some data, and return a chi2 value. That chi2 (and its gradient in some cases) can then be input into an arbitrary likelihood function to find the best-fit parameters.
If you want to learn more about microlensing, please visit Microlensing Source website.
Currently, MulensModel supports:
Need more? Open an issue, start a discussion, or send us an e-mail.
Are you using MulensModel for scientific research? Please give us credit by citing the paper published in "Astronomy and Computing" and ASCL reference. For arXiv version please see link. You should also cite relevant papers for algorithms used. In a typical run that uses binary lenses these will be Bozza (2010) and Skowron & Gould (2012). HERE is a list of papers to cite for various algorithms used in MulensModel. We also thank other people who helped in MulensModel development - please see list in AUTHORS.md file.
We have more than a dozen of examples - starting from very simple ones (like plotting a model) to very advanced (like fitting a binary lens model with finite source effect). Please see:
The full documentation of API is at https://rpoleski.github.io/MulensModel/.
The easiest way is to run:
pip install MulensModel
which will download all files and also install all dependencies (using the PyPI website).
If the above method doesn't work or you would like to see other possibilities, then please see the install file.
If you want to contribute to MulensModel, then please see this file.
file revised May 2024