uvex_transients.models.arnett.ArnettMagnetarSpindownSED.flux_bolometric_cgs#
- classmethod ArnettMagnetarSpindownSED.flux_bolometric_cgs(t: NumericalInput, redshift: NumericalInput, luminosity_distance: NumericalInput, **parameters: CGSParameterValue) FloatResult#
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. See
flux_log_cgs().
- Returns:
The observed bolometric flux, in erg/s/cm^2. A scalar is returned if the result is 0-dimensional.
- Return type: