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Exoplanet population inference

This repository contains the code and text for the paper Exoplanet population inference and the abundance of Earth analogs from noisy, incomplete catalogs by Daniel Foreman-Mackey, David W. Hogg, and Timothy D. Morton and submitted to ApJ.

The code lives in the code directory and the LaTeX source code for the paper is in document.

Code

The meat of the probabilistic model is implemented in population.py. Then there are a set of scripts that you can use to generate the figures from the paper. You should look at the docstrings for details but the summary is:

  • simulate.py generates synthetic catalogs from known occurrence rate density functions,
  • main.py does the MCMC analysis on either real or simulated catalogs, and
  • results.py analyzes the results of the MCMC, makes some figures, and thins the chain to the published form.

Results

Our simulated catalogs and results are available online on figshare.

Attribution

This code is associated with and written specifically for our paper. If you make any use of it, please cite:

@article{exopop,
   author = {{Foreman-Mackey}, D. and {Hogg}, D.~W. and {Morton}, T.~D.},
    title = {Exoplanet population inference and the abundance of
             Earth analogs from noisy, incomplete catalogs},
  journal = {ArXiv --- submitted to ApJ},
     year = 2014,
   eprint = {1406.3020}
}

License

Copyright 2014 Daniel Foreman-Mackey

The code in this repository is made available under the terms of the MIT License. For details, see the LICENSE file.

exopop's People

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exopop's Issues

title, abstract, intro

I just refactored the abstract and it needs checking. I edited in the browser, so I may have broken LaTeX. I made huge changes to the ordering, to get it into context, aims, method, results order. I explicitly called out the differences with Petigura, which I now think is necessary.

I only tweaked the Intro. Let me know when you need more. Signed, @davidwhogg

compare posterior inferences about small planets

As per my reaction to Scott:

We should compare the posterior inferences about the small planets in Petigura to those that emerge (implicitly) in our hierarchical model. These might be significant for the most important planets.

return to multiplicity issues in the discussion

I like the intro discussion of this, but at least mention it at the end too. The discussion should contain all the reasons we might be wrong, and, where possible, the direction that wrongness would take us.

fig 10 missing

  • no comparisons.pdf is in the repo; please add; I get a failure on make
  • on that figure (and in the text) replace "negligible uncertainties" to "uncertainties ignored" or "uncertainties not used".

write note about optimal estimators

If you really have a result about 1/Vmax weighting, this should be published as a separate note, either arxiv-only or in an appropriate journal

thank Eric Ford

either in the list with Bovy, or else explicitly as the key organizer of SAMSI

plot adjustments

What about putting error bars on the points? too busy?

Should day T [days](as it does) but then ln(T / day).

Also, the b/w printer will suck -- you have vibrating red on grey. Make the Petigura points full black (they are the data!), and stretch the greyscale from 0.5 to 1.0, not 0. to 1.0. Then you can make the completeness contours thinner too.

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