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foregroundstelecon20180315 [2018/03/16 16:46] – created hananyforegroundstelecon20180315 [2018/03/16 17:03] (current) – hanany
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 === Notes === === Notes ===
 + 
 +  * Shaul gives an update from Julian: maps for pico have not been made yet. Julian contacted Josquin (SMICA) and Carlo (NILC) and waiting to hear back. **Action for Julian: to get the maps made.** 
 +  * Belen asks whether the high resolution maps will be available, not only nside=16. Agreement that they should be available. Also agreeing that it is useful to run the SEVEM analysis on both the nside=16 maps and higher resolution nside=128, to compare with Matthieu, and to check the results for higher resolution, respectively. 
 +  * Some discussion around Matthieu's results from last week that the 21, 25 GHz bands turned out to not provide extra constraining power on r. The highest two PICO frequencies did.
 +    * Agreement all around that this is not yet an indication that we should remove the low frequency bands.
 +    * Agreement that this result may depend on the input model
 +    * Enrique points out that Mattieu's analysis goes to \ell=50. Perhaps if we include information up to \ell=200, the value of the higher frequency bands would degrade. 
 +    * Shaul reports on Clem's suggestion from last week that Matthieu will re-run with fixed dust temperature, not varying across the sky. 
 +  * Shaul suggests that since Belen is set to run on PSM, she would repeat Matthieu's analysis to get a cross check of the results with a different code and the ability to go to higher \ells. **Belen says she can do that. She will get in touch with Matthieu.** 
  
    
foregroundstelecon20180315.1521236775.txt.gz · Last modified: 2018/03/16 16:46 by hanany

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