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[ascl:1705.006] f3: Full Frame Fotometry for Kepler Full Frame Images

Light curves from the Kepler telescope rely on "postage stamp" cutouts of a few pixels near each of 200,000 target stars. These light curves are optimized for the detection of short-term signals like planet transits but induce systematics that overwhelm long-term variations in stellar flux. Longer-term effects can be recovered through analysis of the Full Frame Images, a set of calibration data obtained monthly during the Kepler mission. The Python package f3 analyzes the Full Frame Images to infer long-term astrophysical variations in the brightness of Kepler targets, such as magnetic activity or sunspots on slowly rotating stars.

Code site:
https://github.com/benmontet/f3
Appears in:
http://adsabs.harvard.edu/abs/2017arXiv170507928M
Bibcode:
2017ascl.soft05006M

ascl:1705.006
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