Metadata-Version: 2.1
Name: pdspy
Version: 1.5.5
Summary: Radiative transfer modeling of protoplanetary disks
Home-page: https://github.com/psheehan/pdspy
Author: Patrick Sheehan
Author-email: psheehan@northwestern.edu
License: UNKNOWN
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        # pdspy: A MCMC Tool for Continuum and Spectral Line Radiative Transfer Modeling
        
        Welcome to the GitHub page for pdspy! This code is meant to fit Monte Carlo Radiative Transfer models for protostellar/protoplanetary disks to ALMA continuum and spectral line datasets using Markov Chain Monte Carlo fitting.
        
        Further capabilities (e.g. fitting spectral line data with a radiative equilibrium calculation) are being developed. If you are interested in new features, do let me know and I would be happy to either add them myself, or to work with you to add them. The documentation is currently included below, but will be ported to a more extensive, better laid out format soon. 
        
        If you are interested in making use of the code, please check out the [documentation](http://pdspy.readthedocs.io).
        
        For more extensive details on what the code does, please see these papers:
        
           + [Disk Masses for Embedded Class I Protostars in the Taurus Molecular Cloud](https://ui.adsabs.harvard.edu/abs/2017ApJ...851...45S/abstract)
           + [High-precision Dynamical Masses of Pre-main-sequence Stars with ALMA and Gaia](https://ui.adsabs.harvard.edu/abs/2019ApJ...874..136S/abstract)
           
        If you have any questions about using the code (or this documentation), requests for features, or suggestions for improvement, please don't hesitate to send me an e-mail.
        
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Description-Content-Type: text/markdown
