marg-iso - A program to estimate p(s,A,R|data) for stars
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Author - Stuart Sale
Intro
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This is python based module to estimate the posterior p(s,A,R|data)
for stars by fitting a Gaussian mixture model, where s is the
distance, A the (monochromatic) extinction and R parametrises the
extinction law.
This software accompanies Sale & Magorrian (2015)
http://adsabs.harvard.edu/abs/2015MNRAS.448.1738S .
The posteriors p(s,A,R|data) can be used in the Gaussian Process
based 3d extinction method of Sale & Magorrian (2014)
http://adsabs.harvard.edu/abs/2014MNRAS.445..256S .
Comments
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More documentation to follow in due course.
