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--- foregroundstelecon20210701 [2021/08/19 09:53] – hanany
+++ foregroundstelecon20210701 [2021/08/19 11:36] (current) – hanany
@@ Line 9: / Line 9: @@
 === Agenda: ===
-  - Ragnhild -
+  - Ragnhild
-  - Mathieu -
+  - Mathieu {{ ::nilc_pico_20210701.pdf | MR Update}}
-  - Kris -
+  - Kris
 === Notes (Shaul) === \\
+  * Ragnhild thinks that C2 estimation of CMB spectra is ok. Proceeding forward.
+  * {{ ::nilc_pico_20210701.pdf | MR shows an update with results for model 96}}. Kris suggests to integrate the likelihoods to get proper limits.
+    * Kris: you are doing r=0.003 and r = 0; but what if you have small r, but non-zero? Why are we using r =0.003?
+    * Some discussion about the level of delensing. Why are we using 60%? **SH to contact Julien Caron**.
+    * Kris: What are you assuming about the spectral index for synchrotron? We should not assume a uniform spectral index. What beta per pixel? **notes are not clear about the answer**
+  * Kris discusses his small scale synchrotron model: model is phenomenological, not physically motivated. It is tweaked to insert small scale 'mathematically', but not to violate what's know about the sky.
+    * He takes Planck 353 GHz dust and modifies it. So the small scale synchrotron would be highly correlated with Planck's dust in small patches of the sky.