uvex_transients.transients.supernovae.TypeIIbSNe.rate_shape

TypeIIbSNe.rate_shape(z: float | NDArray[float64]) → float | NDArray[float64]

Return the shared core-collapse SNe redshift shape (Madau & Dickinson 2014) at redshift(s) z.

Parameters:

z (float or numpy.ndarray) – Redshift(s) at which to evaluate the rate shape.

Returns:

The dimensionless rate shape, common to every core-collapse SNe subtype.

Return type:

float or numpy.ndarray