Iterative curved sky s06b nofg lensing templates
Julien Carron, April 10 2020
This pages describes the 100 iterative (maximum a posteriori, 'MAP') lensing map built from the s06b simulations without foreground, and the associated lensing template.
The CMB likelihood model used to build the maps include:
- Curved-sky geometry
- An inhomogeneous noise model built from the hit map
/project/projectdirs/cmbs4/expt_xx/06b/rhits/n2048.fitstogether with the empirically estimated central noise value
- Exact deprojection of all B-modes from 2 to 200, to ensure these modes are not used to build the lensing template
- Used are E-modes from 2 to 3000 and B-modes from 200 to 3000
- The same mean-field is used for each iteration
The approximation to the mean-field leaves a residual sometimes visible near the edges of the patch. This is however restricted to low lensing multipoles, and does not affect the B-template quality.
A typical cross-correlation to the input lensing looks like this (calculated in the central region of the patch)
The B-templates are built remapping the estimated unlensed E-mode
Across the central region, I estimate the residual B-power after template substraction to be about 0.1 (for something close to 0.3 for the QE, the starting point)