Differences

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--- foregroundstelecon20200820 [2020/08/20 13:42] – hanany
+++ foregroundstelecon20200820 [2020/11/01 20:50] (current) – hanany
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 ====== Telecon Notes Aug 20 2020 ======
-[[https://zzz.physics.umn.edu/ipsig/foregrounds|Link to main foregrounds telecons page]] \\
+[[https://spa-zzz-01.spa.umn.edu/!ipsig/foregrounds|Link to main foregrounds telecons page]] \\
 [[https://zzz.physics.umn.edu/ipsig/logbook|Link to logbook]]
@@ Line 9: / Line 9: @@
 Notes: Shaul \\
-  * Ragnhild shows {{::20200820_commander_pico.pdf|recent work}} on model 90.91. Reminder: Ragnhild reported that when she used 90.92 she identified excess power at low \ell; so she is attempting to use a simpler model. 90.92 has two dust spectra; 90.91 has a single dust spectrum.
+  * Ragnhild shows {{::20200820_commander_pico.pdf|recent work on model 90.91}}. Reminder: Ragnhild reported that when she used 90.92 she identified excess power at low \ell; so she is attempting to use a simpler model. 90.92 has two dust spectra; 90.91 has a single dust spectrum.
   * Slide 3 (bottom panel) shows the difference between input CMB and reconstructed CMB. Large scale synchrotron is clearly visible.
   * Slide 4 shows maps of chi^2. There are areas of high excess, which implies that Ragnhild may need to adjust the area of the mask, and/or futz some more with the fitting.