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

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(Created page with "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 asso...")
 
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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
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* 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
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* Exact deprojection of all B-modes from 2 to 200, to ensure these modes are not used to build the lensing template
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* 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.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