uvex_transients.models.supernovae.Ibc.TypeIbSED.eval#

classmethod TypeIbSED.eval(nu: Quantity, t: Quantity, **parameters: ParameterValue) → Quantity#

Evaluate the spectral luminosity at the given frequency and time.

Parameters:
  • nu (Quantity) – Frequency at which to evaluate the model.

  • t (Quantity) – Time since explosion.

  • **parameters – This model’s parameter values. See eval_log_cgs().

Returns:

\(L_\nu(\nu, t)\), in erg/s/Hz.

Return type:

Quantity