kappa_ell_cut¶
Apply minimum and maximum ell to cross-power spectra with CMB kappa.
File |
cmb_lensing/kappa_ell_cut/kappa_beam.py |
URL |
It is often useful to apply a maximum or minimum ell cut to a CMB lensing map before measuring correlation functions with galaxies and shears. If such an ell-cut is applied, we must account for it on the modeling side. This module applies the lmin/lmax cut to the relevant cross-power spectra.
Assumptions¶
None
Setup Parameters¶
Name |
Type |
Default |
Description |
|---|---|---|---|
shearkappa_section |
str |
Section name where harmonic-space cross-spectrum between galaxy shear and CMB kappa is stored. Leave blank if none. |
|
galkappa_section |
str |
Section name where harmonic-space cross-spectrum between galaxy density and CMB kappa is stored. Leave blank if none. |
|
lmin |
0 |
Minimum ell to impose for CMB kappa cross-spectra. |
|
lmax |
int |
999999 |
Maximum ell to impose for CMB kappa cross-spectra. |
Input values¶
Section |
Name |
Type |
Default |
Description |
|---|---|---|---|---|
shear_cmbkappa_cl |
ell |
int 1d |
Angular frequency values at which Shear-kappa c_ell is evaluated |
|
bin_{i}_{j} |
real 1d |
Shear-kappa C_ell calculated at corresponding ell for relevant i and j combinations |
||
galaxy_cmbkappa_cl |
ell |
int 1d |
Angular frequency values at which Galaxy-kappa c_ell is evaluated |
|
bin_{i}_{j} |
real 1d |
Galaxy-kappa C_ell calculated at corresponding ell for relevant i and j combinations |
Output values¶
Section |
Name |
Type |
Description |
|---|---|---|---|
shear_cmbkappa_cl |
ell |
int 1d |
Angular frequency values at which Shear-kappa c_ell is evaluated |
bin_{i}_{j} |
real 1d |
Shear-kappa C_ell, set to zero outside cuts |
|
galaxy_cmbkappa_cl |
ell |
int 1d |
Values at which c_ell is evaluated |
bin_{i}_{j} |
real 1d |
Galaxy-kappa C_ell, set to zero outside cuts |