uvex_transients.models.supernovae.Ia.TypeIaSED.eval_cgs#

classmethod TypeIaSED.eval_cgs(nu: NumericalInput, t: NumericalInput, **parameters: CGSParameterValue) → FloatResult#

Spectral luminosity, taking and returning plain cgs numbers.

Parameters:
  • nu (array-like) – Frequency, in Hz.

  • t (array-like) – Time since explosion, in seconds.

  • **parameters – This model’s parameter values, in cgs units. See eval_log_cgs().

Returns:

\(L_\nu(\nu, t)\), in erg/s/Hz. A scalar is returned if the result is 0-dimensional.

Return type:

numpy.ndarray or float