# Difference between revisions of "Iterative curved sky s06b nofg lensing templates"

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This pages describes the 100 iterative (maximum a posteriori, 'MAP') lensing map built from the s06b simulations without foreground, and the associated lensing template. | This pages describes the 100 iterative (maximum a posteriori, 'MAP') lensing map built from the s06b simulations without foreground, and the associated lensing template. | ||

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+ | The CMB likelihood model used to build the maps include: | ||

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+ | * Curved-sky geometry | ||

+ | * An inhomogeneous noise model built from the hit map <code>/project/projectdirs/cmbs4/expt_xx/06b/rhits/n2048.fits </code> together 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 |

## Revision as of 07:13, 10 April 2020

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.fits`

together 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