Flicker: Mean stellar densities from flicker
Abstract
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.
- Publication:
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Astrophysics Source Code Library
- Pub Date:
- November 2014
- Bibcode:
- 2014ascl.soft11016K
- Keywords:
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- Software