When generating a light curve, ASTERIA only returns a time series bound by the times set by a given supernova model. In principle, for returning noisy data, we could have the option to pad the data with background-only counts for times outside the range set by the model.
When generating a light curve, ASTERIA only returns a time series bound by the times set by a given supernova model. In principle, for returning noisy data, we could have the option to pad the data with background-only counts for times outside the range set by the model.