@@ -370,7 +370,7 @@ def gather_model_parameters(pevent, model_fit):
370370 # Calculate the reduced chi2
371371 ndata = 0
372372 for i ,tel in enumerate (pevent .telescopes ):
373- ndata += len (tel .lightcurve_magnitude )
373+ ndata += len (tel .lightcurve )
374374 model_params ['red_chi2' ] = np .around (model_params ['chi2' ] / float (ndata - len (param_keys )),3 )
375375
376376 # Retrieve the flux parameters, converting from PyLIMA's key nomenclature to MOPs
@@ -526,10 +526,10 @@ def generate_model_lightcurve(pevent, model_params):
526526
527527 magnitude = toolbox .brightness_transformation .flux_to_magnitude (flux_model )
528528
529- model_telescope .lightcurve_magnitude ["mag" ] = magnitude * unit .mag
529+ model_telescope .lightcurve ["mag" ] = magnitude * unit .mag
530530
531531 mask = ~ np .isnan (magnitude )
532- model_telescope .lightcurve_magnitude = model_telescope .lightcurve_magnitude [mask ]
532+ model_telescope .lightcurve = model_telescope .lightcurve [mask ]
533533
534534 return model_telescope
535535
@@ -545,8 +545,8 @@ def store_model_lightcurve(mulens, model):
545545
546546 # Extract the model lightcurve timeseries from the PyLIMA fit object
547547 data = {
548- 'lc_model_time' : model .lightcurve_magnitude ['time' ].value .tolist (),
549- 'lc_model_magnitude' : model .lightcurve_magnitude ['mag' ].value .tolist ()
548+ 'lc_model_time' : model .lightcurve ['time' ].value .tolist (),
549+ 'lc_model_magnitude' : model .lightcurve ['mag' ].value .tolist ()
550550 }
551551
552552 # If there is no existing model for this target, create one
0 commit comments