CONAN._classes.load_lightcurves.contamination_factors#

CONAN._classes.load_lightcurves.contamination_factors(cont_ratio=0, verbose=True)#

add contamination factor for each unique filter defined in load_lightcurves(). This is the sum of contaminating flux divided by the target star flux within the aperture.

Parameters:

cont_ratio (tuple, float;) – ratio of contamination flux to target flux in aperture for each filter. The order of list follows lc_obj._filnames. Very unlikely but if a single float/tuple is given for several filters, same cont_ratio is used for all.

_contfact_dict#

dictionary of contamination factors for each filter

Type:

dict;

Examples

>>> lc_obj.contamination_factors(cont_ratio=0.1)  # fixed contamination ratio for all filters
>>> lc_obj.contamination_factors(cont_ratio=[0.1,0.08])  # different contamination ratio for each filter
>>> lc_obj.contamination_factors(cont_ratio=(0.1,0.01))  # normal prior for all filters