Enumeration
NumCosmoXcorKernelCMBLensingSource
Description [src]
Where the CMB photons are placed along the line of sight. The thin screen is the usual single source plane at $z_$. The visibility source integrates the lensing efficiency over the last-scattering shell, whose width in comoving distance is about one percent of $\chi_$. With reionization, the tenth of the photons that last scatter at $z \sim 10$ are lensed only by the structure in front of them: between the reionization bump and the shell the kernel is lowered by that fraction, while at low redshift, where every source is far away, the two visibility sources agree.
Members
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NC_XCOR_KERNEL_CMB_LENSING_SOURCE_THIN_SCREEN -
Every CMB photon last scatters at the decoupling redshift of the
NcDistance.- Value:
0 - Available since: 1.0
- Value:
-
NC_XCOR_KERNEL_CMB_LENSING_SOURCE_VISIBILITY -
The sources follow the visibility function of the
NcXcorKernelCMBLensing:recombobject over the last-scattering shell, normalized to unit integral there.- Value:
1 - Available since: 1.0
- Value:
-
NC_XCOR_KERNEL_CMB_LENSING_SOURCE_VISIBILITY_REIONIZATION -
The sources follow the full visibility function, the reionization bump included.
- Value:
2 - Available since: 1.0
- Value: