Campuses:
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| foregroundstelecon20210429 [2021/04/29 09:32] – hanany | foregroundstelecon20210429 [2021/05/19 21:33] (current) – hanany | ||
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| === Notes (Shaul) === \\ | === 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 ' | ||
| + | * 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. | ||