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

User Tools


foregroundstelecon20220217

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
foregroundstelecon20220217 [2022/02/21 16:18] hananyforegroundstelecon20220217 [2022/02/21 16:27] (current) hanany
Line 8: Line 8:
 Regrets:  Regrets: 
  
-=== Agenda: ===+=== Agenda + Notes: ===
  
   * Commander - Low \ell likelihood   * Commander - Low \ell likelihood
     * {{::galloway_20220217_r_curv_0.0.png?25|}}      * {{::galloway_20220217_r_curv_0.0.png?25|}} 
     * {{::galloway_20220217_r_curv_0.0030.png?25|}}     * {{::galloway_20220217_r_curv_0.0030.png?25|}}
 +    * Matthew show two simulations (above) one for r=0 and another for r=0.003, comparing the Gaussian likelihood to the correct low-ell approximation. The likelihood is only calculated for \ell 2-12; full sky, no masking or sky fraction. Not delensed. For next week: extend \ell range to \ell=200, and masked sky.  
   * NILC - small patch analysis   * NILC - small patch analysis
 +    * {{::jd_20220217_patchy-sky.png?25|}}
 +    * Jacques produced patches for MR. Code sent. MR will compute r in each patch. 
   * Delensing - include material in paper   * Delensing - include material in paper
 +    * {{ ::nilc_pico_20220217.pdf |r likelihood with real delensing noise }}
 +    * MR took the real delensing noise and injected it into his r-estimate for r=0 and finds an essentially identical result. Julien suggest doing the same with r=0.003, but MR argues we should again be reproducing his calculations. 
 +
  
-=== Notes: === 
  
foregroundstelecon20220217.1645481925.txt.gz · Last modified: 2022/02/21 16:18 by hanany