Go to the U of M home page
School of Physics & Astronomy
Probe Mission Study Wiki

User Tools


foregroundstelecon20210826

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revisionPrevious revision
Next revision
Previous revision
foregroundstelecon20210826 [2021/09/08 20:40] hananyforegroundstelecon20210826 [2021/09/08 20:47] (current) hanany
Line 15: Line 15:
 DELENSING PLAN  DELENSING PLAN 
  
-  1) get simulated maps at proper nside (2048), with PICO optical beam and noise. No point sources: Two options: PySM or PSM. To be discussed with Clem. +  get simulated maps at proper nside (2048), with PICO optical beam and noise. No point sources: Two options: PySM or PSM. To be discussed with Clem. 
-  2) Do delensing without FG, but with a mask and noise +  beams (Julien). +  Do delensing without FG, but with a mask and noise +  beams (Julien). 
-  3) Do delensing on component-separated maps (Julien). +  Do delensing on component-separated maps (Julien). 
-  4) Julien will provide a B-modes from lensing alone (+ characterization)+  Julien will provide a B-modes from lensing alone (+ characterization) 
 + 
 +WORK ON COMPSEP 
 + 
 +Commander: Ragnhild working on debugging. 
 + 
 +NILC: Mathieu gave an update of the GNILC pipeline on 5 models: (91, 92 93, 96, 98); Draft on overleaf filled with figures from Mathieu (figures for model 98 still to be added). Satisfactory component separation for all models except 98. Low and high frequency channels are useful. 
 + 
 +Q. Does the delensing go in the paper currently being drafted? A separate section at nside=2048 could be included.
  
foregroundstelecon20210826.1631151655.txt.gz · Last modified: 2021/09/08 20:40 by hanany