py21cmsense.conversions.dL_df

py21cmsense.conversions.dL_df(z: float | np.array, cosmo: FLRW = FlatLambdaCDM(name='Planck15', H0=<Quantity 67.74 km / (Mpc s)>, Om0=0.3075, Tcmb0=<Quantity 2.7255 K>, Neff=3.046, m_nu=<Quantity [0., 0., 0.06] eV>, Ob0=0.0486), approximate=False) un.Quantity[un.Mpc / un.MHz / littleh][source]

Get the factor to convert bandwidth to line-of-sight distance in Mpc/h.

Parameters:

z (float) – The redshift