CosmicFish  Reference documentation for version 1.0
Looking into future Cosmology
Functions/Subroutines
lensnoise Module Reference

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...
 

Detailed Description

This module contains the code to compute the noise for CMB lensing.

Function/Subroutine Documentation

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.

Parameters
[in]inclsInput 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]inlclsInput lensed Cls vector: 1 = Temperature 2 = E mode polarization 3 = TE cross correlation 4 = B mode polarization
[in]clnoiseInput noise Cls vector: 1 = Temperature noise 2 = Polarization noise
[out]nlddOutput CMB lensing noise vector
[in,out]jjmaxtmaxFuturCMB internal parameter. Needs to be a suitable value. If the value is too small the code will enforce compatibility with lmaxM.
[in]lmaxmMaximum l at which to compute lensing noise.

Definition at line 53 of file 007_FUTURCMB_lensnoise.f90.