uvex_transients.models.arnett.ArnettDecaySED.flux_bolometric#
- classmethod ArnettDecaySED.flux_bolometric(t: Quantity, *, redshift: PhysicalInput | None = None, luminosity_distance: Quantity | None = None, angular_diameter_distance: Quantity | None = None, proper_distance: Quantity | None = None, cosmology: FLRW | None = None, **parameters: ParameterValue) Quantity#
Evaluate the observed bolometric flux at the given time.
- Parameters:
t (
Quantity) – Observed time since explosion.redshift (
array-likeorQuantity, optional) – Seeflux_log().luminosity_distance (
Quantity, optional) – Seeflux_log().angular_diameter_distance (
Quantity, optional) – Seeflux_log().proper_distance (
Quantity, optional) – Seeflux_log().cosmology (
FLRW, optional) – Seeflux_log().**parameters – This model’s parameter values. See
eval_log_cgs().
- Returns:
\(F_\mathrm{bol}(t)\), in erg/s/cm^2.
- Return type: