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: | ||
| + | |||
| + | * 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 08:13, 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.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
