CosmicFish
Reference documentation for version 1.0
Looking into future Cosmology
|
This module contains the code to compute the noise for CMB lensing. More...
Functions/Subroutines | |
subroutine, public | calc_nldd (incls, inlcls, clnoise, nldd, jjmaxTmax, lmaxM) |
This subroutine computes the noise for the Okamoto & Hu's estimator of the CMB lensing. More... | |
This module contains the code to compute the noise for CMB lensing.
subroutine, public lensnoise::calc_nldd | ( | real(dl), dimension (:,:), intent(in) | incls, |
real(dl), dimension (:,:), intent(in) | inlcls, | ||
real(dl), dimension (:,:), intent(in) | clnoise, | ||
real(dl), dimension (:), intent(out) | nldd, | ||
integer, intent(inout) | jjmaxTmax, | ||
integer, intent(in) | lmaxM | ||
) |
This subroutine computes the noise for the Okamoto & Hu's estimator of the CMB lensing.
[in] | incls | Input scalar Cls vector: 1 = Temperature 2 = E mode polarization 3 = TE cross correlation 4 = dd lensing deflection angle 5 = Td temperature lensing deflection cross correlation |
[in] | inlcls | Input lensed Cls vector: 1 = Temperature 2 = E mode polarization 3 = TE cross correlation 4 = B mode polarization |
[in] | clnoise | Input noise Cls vector: 1 = Temperature noise 2 = Polarization noise |
[out] | nldd | Output CMB lensing noise vector |
[in,out] | jjmaxtmax | FuturCMB internal parameter. Needs to be a suitable value. If the value is too small the code will enforce compatibility with lmaxM. |
[in] | lmaxm | Maximum l at which to compute lensing noise. |
Definition at line 53 of file 007_FUTURCMB_lensnoise.f90.