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A data-driven causal model for modeling systematics in Kepler light curves

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The CPM for Kepler Data
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A data-driven model to calibrate out instrument-induced systematics in
*Kepler* light curves.
The model exploits causal structure to remove telescope and stellar
variability without distorting exoplanet signals.

authors
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- Dan Foreman-Mackey (NYU)
- David W. Hogg (NYU) (MPIA)
- Bernhard Schölkopf (MPI-IS)
- Dun Wang (NYU)

license
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Copyright 2013, 2014 the authors.  **Not ready for redistribution.**

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forked from https://github.com/dfm/cpm

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