Metadata-Version: 2.1
Name: astro-eddy
Version: 2.1.3
Summary: Tools to recover expectionally precise rotation curves from spatially resolved spectra.
Home-page: https://github.com/richteague/eddy
Author: Richard Teague
Author-email: richard.d.teague@cfa.harvard.edu
License: MIT
Description: # eddy - Extracting Disk DYnamics
        
        [![status](http://joss.theoj.org/papers/2868c5ad4b6405eba1aaf1cd8ea53274/status.svg)](http://joss.theoj.org/papers/2868c5ad4b6405eba1aaf1cd8ea53274)
        [![DOI](https://zenodo.org/badge/DOI/10.5281/zenodo.1440051.svg)](https://doi.org/10.5281/zenodo.1440051)
        <a href="http://ascl.net/1901.010"><img src="https://img.shields.io/badge/ascl-1901.010-blue.svg?colorB=262255" alt="ascl:1901.010" /></a>
        [![Documentation Status](https://readthedocs.org/projects/eddy/badge/?version=latest)](https://eddy.readthedocs.io/en/latest/?badge=latest)
        
        `eddy` is a suite of Python tools to recover precise velocity profiles of protoplanetary disks from Doppler shifted line emission. `eddy` makes fitting of first moment maps and the inference of a rotation velocity from an annulus of spectra a breeze.
        
        ## Installation
        
        The most simple method is with `pip`,
        
        ```
        pip install astro-eddy
        ```
        
        The only real dependencies for this are `numpy`, `scipy`, `matplotlib`, and [`emcee`](https://github.com/dfm/emcee), If you want to run the Gaussian Process method you will also need [`celerite`](https://github.com/dfm/celerite) which can be easily installed if you follow their [installation guide](https://celerite.readthedocs.io/en/stable/python/install/).
        
        If things have installed correctly you should be able to run the [Jupyter Notebooks](https://github.com/richteague/eddy/tree/master/docs/tutorials) with no errors. If something goes wrong, please [open an issue](https://github.com/richteague/eddy/issues/new).
        
        ## Useage
        
        For guides on how to use `eddy` you will find extensive examples in the [documents](https://github.com/richteague/eddy/tree/master/docs). We shamelessly recommend [bettermoments](https://github.com/richteague/bettermoments) to make the moment maps required for the fitting.
        
        ## Citations
        
        If you use `eddy` as part of your research, please cite the [JOSS article](http://joss.theoj.org/papers/10.21105/joss.01220):
        
        ```latex
        @article{eddy,
            doi = {10.21105/joss.01220},
            url = {https://doi.org/10.21105/joss.01220},
            year = {2019},
            month = {feb},
            publisher = {The Open Journal},
            volume = {4},
            number = {34},
            pages = {1220},
            author = {Richard Teague},
            title = {eddy},
            journal = {The Journal of Open Source Software}
        }
        ```
        
        A full list of citations including dependencies can be found on the [citations](./docs/citations.md) page.
        
        ## Works using `eddy`
        
        A list of the works using (or at least citing) `eddy` can be found on [ADS](https://ui.adsabs.harvard.edu/abs/2019JOSS....4.1220T/citations).
        
Platform: UNKNOWN
Classifier: Programming Language :: Python :: 3.5
Classifier: License :: OSI Approved :: MIT License
Classifier: Operating System :: OS Independent
Description-Content-Type: text/markdown
