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[ascl:2206.014] SpinSpotter: Stellar rotation periods from high-cadence photometry calculator

SpinSpotter calculates stellar rotation periods from high-cadence photometry. The code uses the autocorrelation function (ACF) to identify stellar rotation periods up to one-third the observational baseline of the data. SpinSpotter includes diagnostic tools that describe features in the ACF and allows tuning of the tolerance with which to accept a period detection.

Code site:
https://github.com/rae-holcomb/SpinSpotter
Described in:
https://ui.adsabs.harvard.edu/abs/2022ApJ...936..138H
Bibcode:
2022ascl.soft06014H

Views: 1230

ascl:2206.014
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