POSYDON is a next-generation single and binary-star population synthesis code incorporating full stellar structure and evolution modeling with the use of MESA.
@ZepeiX showed that lambda values for grid slices in the CO_HeMS(_RLO) grid have lambda values ( ie S1_lambda_CE_pure_He_star_1cent) that are all NaN. PR #338 still has NaN slices in training.
Current behaviour:
As such, these parameters are not included in the BaseIFInterpolator.evaluate() output. This function returns interpolator values from out_keys and out_nan_keys stored in the BaseIFInterpolator.
Because we set out_keys as an input based on the presence of at least 1 non-nan value in the grid, the key is excluded andout_nan_keys is not calculated, since it's not part of BaseIFInterpolator.__init__.
Expected behaviour
We want the interpolator to return these grid values to allow for CE evolution.
As such, I've added the out_nan_keys as an input to the BaseIFInterpolator.__init__ in PR #342
@ZepeiX showed that lambda values for grid slices in the CO_HeMS(_RLO) grid have lambda values ( ie
S1_lambda_CE_pure_He_star_1cent) that are all NaN. PR #338 still has NaN slices in training.Current behaviour: As such, these parameters are not included in the
BaseIFInterpolator.evaluate()output. This function returns interpolator values fromout_keysandout_nan_keysstored in the BaseIFInterpolator. Because we setout_keysas an input based on the presence of at least 1 non-nan value in the grid, the key is excluded andout_nan_keysis not calculated, since it's not part ofBaseIFInterpolator.__init__.Expected behaviour We want the interpolator to return these grid values to allow for CE evolution. As such, I've added the
out_nan_keysas an input to theBaseIFInterpolator.__init__in PR #342