pypi i galpy


Galactic Dynamics in python

by Jo Bovy

1.8.1 (see all)License:New BSD
pypi i galpy

Galactic Dynamics in python

galpy is a Python package for galactic dynamics. It supports orbit integration in a variety of potentials, evaluating and sampling various distribution functions, and the calculation of action-angle coordinates for all static potentials. galpy is an astropy affiliated package and provides full support for astropy’s Quantity framework for variables with units.


Jo Bovy - bovy at astro dot utoronto dot ca

See AUTHORS.txt for a full list of contributors.

If you find this code useful in your research, please let me know. If you use galpy in a publication, please cite Bovy (2015) and link to See the acknowledgement documentation section for a more detailed guide to citing parts of the code. Thanks!


The latest documentation can be found here. You can also join the galpy slack community for any questions related to galpy; join here.

If you find any bug in the code, please report these using the Issue Tracker or by joining the galpy slack community.

If you are having issues with the installation of galpy, please first consult the Installation FAQ.


galpy supports Python 3. Specifically, galpy supports Python 3.7, 3.8, 3.9, 3.10, and 3.11. GitHub Actions CI builds regularly check support for Python 3.10 (and of 3.7, 3.8, and 3.9 using a more limited, core set of tests) on Linux and Windows (and 3.10 on Mac OS); Appveyor builds regularly check support for Python 3.10 on Windows. Python 2.7 is no longer supported.

This package requires Numpy, Scipy, and Matplotlib. Certain advanced features require the GNU Scientific Library (GSL), with action calculations requiring version 1.14 or higher. Other optional dependencies include:

  • Support for providing inputs and getting outputs as Quantities with units is provided through astropy.
  • Querying SIMBAD for the coordinates of an object in the Orbit.from_name initialization method requires astroquery.
  • Displaying a progress bar for certain operations (e.g., orbit integration of multiple objects at once) requires tqdm.
  • Plotting arbitrary functions of Orbit attributes requires numexpr.
  • Speeding up the evaluation of certain functions in the C code requires numba.
  • Constant-anisotropy DFs in galpy.df.constantbetadf require JAX.
  • Use of SnapshotRZPotential and InterpSnapshotRZPotential requires pynbody.

Other parts of the code may require additional packages and you will be alerted by the code if they are not installed.


If you are interested in contributing to galpy\'s development, take a look at this brief guide on the wiki. This will hopefully help you get started!

Some further development notes can be found on the wiki. This includes a list of small and larger extensions of galpy that would be useful here as well as a longer-term roadmap here. Please let the main developer know if you need any help contributing!


The dehnendf and shudf disk distribution functions can be corrected to follow the desired surface-mass density and radial-velocity-dispersion profiles more closely (see 1999AJ....118.1201D). Calculating these corrections is expensive, and a large set of precalculated corrections can be found here [tar.gz archive]. Install these by downloading them and unpacking them into the galpy/df/data directory before running the installation. E.g.:

curl -O
tar xvzf galpy-dfcorrections.tar.gz -C ./galpy/df/data/
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