[docs]classNFWTruncatedMCRDuffySph(NFWTruncatedSph):""" This function only applies for the lens configuration as follows: Cosmology: FlatLamdaCDM H0 = 70.0 km/sec/Mpc Omega_Lambda = 0.7 Omega_m = 0.3 Redshfit of Main Lens: 0.6 Redshift of Source: 2.5 A truncated NFW halo at z = 0.6 with tau = 2.0 """def__init__(self,centre:Tuple[float,float]=(0.0,0.0),mass_at_200:float=1e9,redshift_object:float=0.5,redshift_source:float=1.0,):""" Input m200: The m200 of the NFW part of the corresponding tNFW part. Unit: M_sun. """self.mass_at_200=mass_at_200(kappa_s,scale_radius,radius_at_200,)=mcr_util.kappa_s_and_scale_radius_for_duffy(mass_at_200=mass_at_200,redshift_object=redshift_object,redshift_source=redshift_source,)super().__init__(centre=centre,kappa_s=kappa_s,scale_radius=scale_radius,truncation_radius=2.0*radius_at_200,)
[docs]classNFWTruncatedMCRLudlowSph(NFWTruncatedMCRScatterLudlowSph):def__init__(self,centre:Tuple[float,float]=(0.0,0.0),mass_at_200:float=1e9,redshift_object:float=0.5,redshift_source:float=1.0,):""" Input m200: The m200 of the NFW part of the corresponding tNFW part. Unit: M_sun. """super().__init__(centre=centre,mass_at_200=mass_at_200,scatter_sigma=0.0,redshift_object=redshift_object,redshift_source=redshift_source,)