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[ascl:1602.014] k2photometry: Read, reduce and detrend K2 photometry

k2photometry reads, reduces and detrends K2 photometry and searches for transiting planets. MAST database pixel files are used as input; the output includes raw lightcurves, detrended lightcurves and a transit search can be performed as well. Stellar variability is not typically well-preserved but parameters can be tweaked to change that. The BLS algorithm used to detect periodic events is a Python implementation by Ruth Angus and Dan Foreman-Mackey (https://github.com/dfm/python-bls).

Code site:
https://github.com/vincentvaneylen/k2photometry
Appears in:
http://adsabs.harvard.edu/abs/2016arXiv160201851V
Bibcode:
2016ascl.soft02014V

ascl:1602.014
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