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--- foregroundstelecon20210429 [2021/04/29 09:31] – hanany
+++ foregroundstelecon20210429 [2021/05/19 21:33] (current) – hanany
@@ Line 8: / Line 8: @@
 === Agenda: ===
-  * New noise spectra from Reijo {{:pico_noise_v2.png?25|}}
+  * New noise spectra from Reijo {{:pico_noise_v2.png?15|}}
+  * Ragnhild+Clem
+  * Kris
-=== Notes (Mathieu) === \\
+  * Mathieu
+=== Notes (Shaul) === \\
+  * SH shows noise spectra from Reijo. ** SH: Needs to find noise parameters and provide to MR and Commander.** But this is not presently on the critical path.
+  * Ragnhild explains the variants of Commander:
+    * Commander 1: all frequencies have the same beam size
+    * Commander 2: each band can have its own beam size
+    * Commander 3: starts from TOD simulations and builds maps + accounts for foregrounds
+  * MR: NILC results are driven by foreground separation not noise. MR does not expect changes in the NILC results due to the 'real' noise. Currently resolution of results are at 1 deg. Don't expect results to depend on resolution.
+  * LB is working on extending the frequency coverage to higher frequencies
+  * Models to use: 90.91=d1s1, 90.92=d7s3 (this is expected to be a challenge for parametric models), MKD.