Marshall

Marshall is a tool for detecting artefacts masquerading as transits of small, long period planets in *Kepler* data. It is described in detail in Mullally et al. (2015, submitted to ApJ)

This code is published primarily as a record of how the results in that paper were produced, and running this package depends on code not yet made available. However, the core of the algorithm is self contained, even if the details of how I ran it on Kepler data are incomplete.

See the readme file for more details.