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private:teleconsnotes20170412 [2017/04/14 16:27] – hananyprivate:teleconsnotes20170412 [2017/04/15 10:41] (current) – hanany
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     * Alex Van Engelen and Blake Sherwin were mentioned as some who can contribute analysis.       * Alex Van Engelen and Blake Sherwin were mentioned as some who can contribute analysis.  
     * __Lloyd will organize study of delensing.__  Question: "what is the level of r that can be achieved as a function of resolution and depth?"     * __Lloyd will organize study of delensing.__  Question: "what is the level of r that can be achieved as a function of resolution and depth?"
-    * Foregrounds: we will need to assess foreground cleaning and contamination. Clem, Julian, Raphael, point out that a pipeline exists for S4 and can be used for the Probe. It will be adapted to handle full sky. +  * Foregrounds: we will need to assess foreground cleaning. Clem, Julian, Raphael, point out that a pipeline exists for S4 and can be used for the Probe. It will be adapted to handle full sky. 
-    * A discussion ensues about the need for various different groups to analyze the data without assuming the input models. We will announce the availability of maps (when available) and invite anyone interested in contributing. Lloyd will coordinate this 'data challenge'. Julian will allocate space at NERSC.  +  * A discussion ensues about the need for various different groups to analyze the data without assuming the input models. We will announce the availability of maps (when available) and invite anyone interested in contributing. __Lloyd will coordinate this 'data challenge'__. Julian will allocate space at NERSC.  
-    * The challenge will need frequency bands and noise levels. __Shaul is responsible to provide.__  +  * The challenge will need frequency bands and noise levels. __Shaul is responsible to provide.__  
-    * Spectrometer:  +  * Al suggests a kick-off workshop to discuss foreground approaches and to help coordinate the community. __Shaul will communicate the suggestion to Jamie/Graca__ (coordinators of the KISS workshop).  
-      * what is the motivation for a stand alone super-pixie?  +  * Spectrometer:  
-      * what is the motivation for compspec (=complementary spectrometer)? Al: excellent foreground removal, and T information that can extend the science by cross-correlating with optical survey.  +    * what is the motivation for a stand alone super-pixie?  
-    * __Al will organize a group that will assess the motivation for a super-pixie and/or develop the case for compspec__. How will such a complementary spectrometer look like? Is it a mini-pixie?  +    * what is the motivation for compspec (=complementary spectrometer)? Al: excellent foreground removal, and T information that can extend the science by cross-correlating with optical survey.  
-    * Other science: 'What is the dream data set that the galactic magnetic field and dust afficionados would like to see'? __Shaul will write to Darren Dowell, and Giles Novack__ to check who from these communities is interested in participating. __Bill Jones will talk with Aureliene__+  * __Al will organize a group that will assess the motivation for a super-pixie and/or develop the case for compspec__. How will such a complementary spectrometer look like? Is it a mini-pixie?  
 +  * Other science: 'What is the dream data set that the galactic magnetic field and dust afficionados would like to see'? __Shaul will write to Darren Dowell, and Giles Novack__ to check who from these communities is interested in participating. __Bill Jones will talk with Aureliene__
private/teleconsnotes20170412.1492205241.txt.gz · Last modified: 2017/04/14 16:27 by hanany

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