Go to the U of M home page
School of Physics & Astronomy
Probe Mission Study Wiki

User Tools


foregroundstelecon20180301

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Next revision
Previous revision
foregroundstelecon20180301 [2018/03/01 10:38] – created hananyforegroundstelecon20180301 [2018/03/08 10:08] (current) pryke
Line 1: Line 1:
 ====== Telecon Notes, March 1, 2018 ====== ====== Telecon Notes, March 1, 2018 ======
  
-Attendance: Shaul, Julian, Davide, Belen, Ken, Lloyd, Brandon+Attendance: Shaul, Julian, Davide, Belen, Ken, Lloyd, Brandon, Charles, +..
  
 Agenda: Agenda:
Line 8: Line 8:
  
 === Notes === === Notes ===
- +(notes by Shaul) 
-  * Julian says currently running PICO noise. Should be available within few days. 1, 2, 4 years. Sky models are available.  +  * Julian is running PICO noise. Should be available within few days. Running 1, 2, 4 years. Sky models are available.  
-  * Shaul asks about which skies are available. Currently only one: PySM A2D7F1F3.  +  * Shaul asks about which skies are available. Currently only one: PySM A2D7F1S3.  
-  * Discussion about how many models to include. There are two axes to explore, to be completed... +  * Discussion about how many models to include. There are two axes to explore, that of multiple sky models with the same analysis, or that of the same sky model with different methods, and then combinations of the twoClem advocated in the past that we have common models as S4Decision: start with two models, the existing PySM and the MHD motivated model.  
- +  * __Action: Matthieu and Belen will run their analyses on these models. Estimate for initial results in 2-4 weeks, depending on technique. Julian will contact Josquin (SMICA?), Carlo and Raphael (NILC)__.  
-  * Matthieu wants Brandon's maps with nside = 16. Brandon will generate. +  * Question: which dust model to put into the MHD model? Decision: Modified BB (I think) 
 +  * Matthieu wants Brandon's maps with nside = 16. __Brandon will generate.__ 
   * Point source polarization: if we use high \ell we need to include point source polarization. Leave this for the future.    * Point source polarization: if we use high \ell we need to include point source polarization. Leave this for the future. 
   * Experts in dust and synchrotron should look at the new maps.    * Experts in dust and synchrotron should look at the new maps. 
-  * + 
foregroundstelecon20180301.1519922316.txt.gz · Last modified: 2018/03/01 10:38 by hanany