uvex_transients.models.arnett.ArnettDecaySED.flux_bolometric_log_cgs#

classmethod ArnettDecaySED.flux_bolometric_log_cgs(t: NumericalInput, redshift: NumericalInput, luminosity_distance: NumericalInput, **parameters: CGSParameterValue) → FloatResult#

Natural log of the observed bolometric flux, taking and returning plain cgs numbers.

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

  • redshift (array-like) – Cosmological redshift, dimensionless.

  • luminosity_distance (array-like) – Luminosity distance, in cm.

  • **parameters – This model’s parameter values, in cgs units; must already broadcast against t.

Returns:

The natural log of the observed bolometric flux, in erg/s/cm^2. A scalar is returned if the result is 0-dimensional.

Return type:

numpy.ndarray or float