def radio_lumfn(L, params, z=0.):
"""
Calculate radio luminosity function for a given set of model parameters.
"""
# Number density as a function of sfr, dn/dlog(sfr)
sfr = L * 5.52e-29 # erg/s/Hz, Bell (2003), Eq. 6
dndlogsfr_sfms, dndlogsfr_pass = g.sfr_fn(hm, sfr, z=z, params=params)
phi = dndlogsfr_sfms #+ dndlogsfr_pass # FIXME: Remove passive galaxies
return phi
def radio_lumfn(L, _params):
"""
Calculate radio luminosity function for a given set of model parameters.
"""
# Number density as a function of sfr, dn/dlog(sfr)
sfr = L * 5.52e-29 # erg/s/Hz, Bell (2003), Eq. 6
dndlogsfr_sfms, dndlogsfr_pass = g.sfr_fn(hm, sfr, z=0., params=_params)
#phi = dndlogsfr_sfms #+ dndlogsfr_pass
return dndlogsfr_sfms, dndlogsfr_pass
def radio_lumfn(L, params, z=0.):
"""
Calculate radio luminosity function for a given set of model parameters.
"""
# Number density as a function of sfr, dn/dlog(sfr)
sfr = L * 5.52e-29 # erg/s/Hz, Bell (2003), Eq. 6
dndlogsfr_sfms, dndlogsfr_pass = g.sfr_fn(hm, sfr, z=z, params=params)
phi = dndlogsfr_sfms #+ dndlogsfr_pass # FIXME: Remove passive galaxies
return phi
def radio_lumfn(L, _params):
"""
Calculate radio luminosity function for a given set of model parameters.
"""
# Number density as a function of sfr, dn/dlog(sfr)
sfr = L * 5.52e-29 # erg/s/Hz, Bell (2003), Eq. 6
dndlogsfr_sfms, dndlogsfr_pass = g.sfr_fn(hm, sfr, z=0., params=_params)
#phi = dndlogsfr_sfms #+ dndlogsfr_pass
return dndlogsfr_sfms, dndlogsfr_pass