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[ascl:1411.016] Flicker: Mean stellar densities from flicker

Flicker calculates the mean stellar density of a star by inputting the flicker observed in a photometric time series. Written in Fortran90, its output may be used as an informative prior on stellar density when fitting transit light curves.

Code site:
https://github.com/davidkipping/flicker https://github.com/RuthAngus/flicker
Described in:
https://ui.adsabs.harvard.edu/abs/2014ApJ...785L..32K
Bibcode:
2014ascl.soft11016K

Views: 3793

ascl:1411.016
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