uvex_transients.models.supernovae.villar.VillarCoolingBlackbodySED.mag_bandpass

classmethod VillarCoolingBlackbodySED.mag_bandpass(bandpass: SpectralElement, 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, log_attenuation: NumericalInput | None = None, **parameters: ParameterValue) → Quantity

Evaluate the apparent AB magnitude of the flux averaged over bandpass.

Convenience wrapper around mag_band() that reads its nu and throughput straight off bandpass instead of requiring them as separate arguments – see mag_bandpass_cgs().

Parameters:

• bandpass (SpectralElement) – The bandpass to average over, e.g. one of an ~m4opt.synphot.Detector’s own ~m4opt.synphot.Detector.bandpasses.

• t (Quantity) – Observed time since explosion.

• redshift (array-like or Quantity, optional) – See flux_log().

• luminosity_distance (Quantity, optional) – See flux_log().

• angular_diameter_distance (Quantity, optional) – See flux_log().

• proper_distance (Quantity, optional) – See flux_log().

• cosmology (FLRW, optional) – See flux_log().

• log_attenuation (array-like, optional) – See flux_band_log_cgs().

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

Returns:

The apparent AB magnitude, as an ABmag Quantity.

Return type:

Quantity