Data Handling¶
The classes defined here are used to find and store Kepler light curves.
The Lightcurve
class is in general the required data format for passing to the
Bayesian analysis functions.
Note
At the moment the Lightcurve
class is specifically designed for Kepler data (although
it could hold any time series if necessary by hardwiring some values). In the future versions
it will be made more generic.