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.
- Dan Foreman-Mackey (NYU)
- David W. Hogg (NYU) (MPIA)
- Bernhard Schölkopf (MPI-IS)
- Dun Wang (NYU)
Copyright 2013, 2014 the authors. Not ready for redistribution.