Overview of the Kepler Science Processing Pipeline
Jon M. Jenkins, Douglas A. Caldwell, Hema Chandrasekaran, Joseph D., Twicken, Stephen T. Bryson, Elisa V. Quintana, Bruce D. Clarke, Jie Li,, Christopher Allen, Peter Tenenbaum, Hayley Wu, Todd C. Klaus, Christopher K., Middour, Miles T. Cote, Sean McCauliff, Forrest R. Girouard

TL;DR
The paper describes the comprehensive data processing pipeline of the Kepler Mission, detailing how raw photometric data are calibrated, corrected, and analyzed to detect transiting exoplanets while minimizing false positives.
Contribution
It provides an overview of the entire Kepler data processing pipeline, highlighting novel techniques for systematic error removal and transit detection in space-based photometry.
Findings
Pipeline successfully detects planetary signatures
Effective false positive rejection methods implemented
Robust identification of transiting exoplanets
Abstract
The Kepler Mission Science Operations Center (SOC) performs several critical functions including managing the ~156,000 target stars, associated target tables, science data compression tables and parameters, as well as processing the raw photometric data downlinked from the spacecraft each month. The raw data are first calibrated at the pixel level to correct for bias, smear induced by a shutterless readout, and other detector and electronic effects. A background sky flux is estimated from ~4500 pixels on each of the 84 CCD readout channels, and simple aperture photometry is performed on an optimal aperture for each star. Ancillary engineering data and diagnostic information extracted from the science data are used to remove systematic errors in the flux time series that are correlated with these data prior to searching for signatures of transiting planets with a wavelet-based, adaptive…
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