################# Dust Grain Fitter ################# ``DGFit`` is a python package to derive dust grain size and composition distributions based on fitting observations of interstellar dust. User Documentation ================== .. toctree:: :maxdepth: 2 Running DGFit Observed Data Plotting results Size Distributions Installation ============ .. toctree:: :maxdepth: 2 How to install Repository ========== GitHub: `DGFit `_ Quick Start =========== Material needed. Reporting Issues ================ If you have found a bug in ``DGFit`` please report it by creating a new issue on the ``DGFit`` `GitHub issue tracker `_. Please include an example that demonstrates the issue sufficiently so that the developers can reproduce and fix the problem. You may also be asked to provide information about your operating system and a full Python stack trace. The developers will walk you through obtaining a stack trace if it is necessary. Contributing ============ Like the `Astropy`_ project, ``DGFit`` is made both by and for its users. We accept contributions at all levels, spanning the gamut from fixing a typo in the documentation to developing a major new feature. We welcome contributors who will abide by the `Python Software Foundation Code of Conduct `_. ``DGFit`` follows the same workflow and coding guidelines as `Astropy`_. The following pages will help you get started with contributing fixes, code, or documentation (no git or GitHub experience necessary): * `How to make a code contribution `_ * `Coding Guidelines `_ * `Developer Documentation `_ For the complete list of contributors please see the `DGFit contributors page on Github `_. Reference API ============= .. automodapi:: dgfit.obsdata .. automodapi:: dgfit.dustgrains .. automodapi:: dgfit.dustmodel :inherited-members: