Secondary eclipse modelling

Secondary eclipses are modelled using muscat2ta.M2EclipseLPF. The eclipse modelling LPF uses the reduced fits-format light curves, so you need to first carry out a per-night light curve reduction using the standard muscat2ta.TransitAnalysis class. The class can be used in its simplest form as

from muscat2ta import M2EclipseLPF

lpf = M2EclipseLPF(name)

where name is the analysis name that will be used also when saving the modelling results, and it also takes a number of arguments that can be used to tell where to look for data and tune the analysis. The full signature is

M2EclipseLPF(name,
             datadir: Union[str, Path] = 'results',
             pattern: str = '*.fits',
             downsample: Optional[float] = None,
             model_baseline: bool = True)

where datadir is the directory where the light curves are stored, pattern is a glob pattern used to identify the light curves, downsample sets binning in time (in seconds), and model_baseline sets whether to use a linear baseline model or not.