mass_dependent_ia_model

adds mass dependence to IA, with a linear equation

File	intrinsic_alignments/mass_dependent_ia/mass_dependent_ia_model.py
Attribution	Marika Asgari
	Benjamin Joachimi
	Konrad Kuijken
URL

Takes input IA Cls, Cl^ij_II and Cl^ij_GI. Then creates new Cl^ij_II = [f_r^(i) * (<M_*>^(i) / M_{, pivot})^beta] * [f_r^(j) * (<M_>^(j) / M_{, pivot})^beta] * Cl^ij_II new Cl^ij_GI = [f_r^(j) * (<M_>^(j) / M_{, pivot})^beta] * Cl^ij_GI new Cl^ij_IG = [f_r^(i) * (<M_>^(i) / M_{*, pivot})^beta] * Cl^ij_IG

Assumptions

• Input model only produces E-modes.

• Currently only works for cosmic shear IA

Setup Parameters

Name	Type	Default	Description
suffix	str		suffix used to distinguish between different data vectors
new_suffix	str		If provided will save the resulting IA Cls using this suffix

Input values

Section	Name	Type	Default	Description
intrinsic_alignment_parameters_{suffix}	beta	real		Mass dependence power for early-type galaxies
	log10_M_pivot	real		log10 of pivot halo mass (M_sun/h), can be derive from mean halo mass of early-type galaxies
	log10_M_mean_{i}	real		log10 of mean halo mass (M_sun/h) of early-type galaxies per redshif bin from catalogues
	f_r_{i}	real		Fraction of early-type galaxies per redshift bin, can be calculated using T_B from catalogues
shear_cl_ii	nbin_a	int		Number of tomographic bins
	bin_{i}_{j}	real 1d		Intrinsic-intrinsic angular spectra for pairs of i,j values C_ell
shear_cl_gi	bin_{i}_{j}	real 1d		Shear-intrinsic angular spectra for pairs of i,j values C_ell
	bin_{j}_{i}	real 1d		Intrinsic-shear angular spectra for pairs of i,j values C_ell

Output values

Output values

Section	Name	Type	Description
shear_cl_ii	nbin_a	int	Number of tomographic bins
	bin_{i}_{j}	real 1d	Intrinsic-intrinsic angular spectra for pairs of i,j values C_ell
shear_cl_gi	bin_{i}_{j}	real 1d	Shear-intrinsic angular spectra for pairs of i,j values C_ell
	bin_{j}_{i}	real 1d	Intrinsic-shear angular spectra for pairs of i,j values C_ell