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private:teleconsnotes20170712 [2017/07/12 16:53] flaugerprivate:teleconsnotes20170712 [2017/07/19 13:02] (current) hanany
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 ====== Telecon Notes 20170712 ====== ====== Telecon Notes 20170712 ======
  
-Attendance: \\+Attendance: Brendan, Raphael, Amy, Al, Shaul, Julian\\
 Notes by: Raphael\\ Notes by: Raphael\\
  
 +=== Actions ===
 +  * Finalize dates + time for Foregrounds workshop (Raphael)
 +  * Communicate with Nobu, Mark/Bill re science workshop (Shaul)
  
 +=== Workshops === 
 +  * Foregrounds 
 +    * Currently aiming for last week of October or first week of November 
 +    * Some rooms cost money. Shaul says to not worry about cost of rooms. 
 +    * Raphael says he would have time to finalize dates and rooms during the week of July 17, when he is back at San Diego
 +  *  Science + Complementarity
 +    * Shaul talked with Mark. Some preference for May 2018
 +    * JB: Possibly coordinate with series of workshops for LiteBIRD? Previous workshops in 12/15 (Japan) and 1/17 (Montreal) Third workshop proposed around 1/18. Shaul suggested that they focus on technology or systematics, to complement our 'science and complementarity' later in the year. 
 +    * SH: Should workshops be endorsed by both teams? May not be good at this point? 
 +    * Shaul to communicate with Mark/Bill, and Nobu (LiteBIRD)
  
-  * Update on Workshops +=== WG ===     
-    - Foregrounds - Raphael +  * Update from Fundamental Physics WG - Raphael 
-      - Currently aiming for last week of October or first week of November  +    * Slides posted 
-    - Science + Complementarity - Mark and/or Bill or Shaul+    * At this point need more input regarding target sensitivities
  
-      - Current target date is May 2018 
-        - JB: Possibly coordinate with series of workshops for LiteBIRD? Previous workshops in 12/15 (Japan) and 1/17 (Montreal) Third workshop proposed around 1/18  
-        - SH: Should workshops be endorsed by both teams? May not be good at this point? 
-         
-  * Update from Fundamental Physics WG - Raphael 
   * Update from Extragalactic WG - Nick Battaglia   * Update from Extragalactic WG - Nick Battaglia
 +    * Recently formed extragalactic science working group, currently 15 members (+pending)
 +    * current approach: extragalactic science cases given CORE design
 +    *  Galaxy clusters: - finding clusters, cosmology, CIB and radio contamination, y-maps, individual tSZ, kSZ, and rSZ for cluster science
 +    * Galaxy formation at z > 2 - properties of star-formation (SF) during the peak of SF via the CIB
 +    * Velocity fields - cosmology, contamination, systematics
 +    * Thermodynamic of galaxy formation - feedback, non-thermal pressure, ionized baryon content
 +    * Reionization - Optical depth constraints, kSZ power spectrum, mid-point and duration of reionization
 +    * Gravitational lensing? Need to involve experts in lensing/delensing, currently involved in extragalactic science working group
 +    * SH: what resolution is needed? at 150 GHz CMBP will not have 1' resolution.  NB: OK to have 1' at the higher frequencies to complement ground-based telescopes. JM: Why are Planck beams not diffraction limited at high frequencies? BC: Not enough signal band width. JM: Can we handle signal band width for diffraction limited beams at ~800 GHz? Amy: we can accommodate 150 Mbits/s for approximately 2 hours a day
 +    * SH: What frequencies are important for cluster science? NB: up to 500-600 GHz
  
-    - Recently formed extragalactic science working group, currently 15 members (+pending) +=== More on NASA slides (continuation from 2 weeks ago) === 
-    - current approach: extragalactic science cases given CORE design +  moved to next telecon
-      - Galaxy clusters: - finding clusters, cosmology, CIB and radio contamination, y-maps, individual tSZ, kSZ, and rSZ for cluster science +
-      - Galaxy formation at z > 2 - properties of star-formation (SF) during the peak of SF via the CIB +
-      - Velocity fields - cosmology, contamination, systematics +
-      - Thermodynamic of galaxy formation - feedback, non-thermal pressure, ionized baryon content +
-      - Reionization - Optical depth constraints, kSZ power spectrum, mid-point and duration of reionization +
-      - Gravitational lensing? Need to involve experts in lensing/delensing, currently involved in extragalactic science working group +
- +
-        JM: Why are Planck beams not diffraction limited at high frequencies? +
-        BC: Not enough signal band width +
-        JM: Can we handle signal band width for diffraction limited beams at ~800 GHz? +
-        SH, NB: What is needed for cluster science? 500-600 GHz? +
- +
-  * More on NASA slides (continuation from 2 weeks ago) - Shaul +
-      moved to next telecon+
private/teleconsnotes20170712.1499896381.txt.gz · Last modified: 2017/07/12 16:53 by flauger