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

User Tools


foregroundstelecon20211013

Differences

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

Link to this comparison view

Both sides previous revisionPrevious revision
foregroundstelecon20211013 [2021/10/20 22:24] hananyforegroundstelecon20211013 [2021/10/20 22:37] (current) hanany
Line 37: Line 37:
       * same as above       * same as above
  
-  * Charles gives outline for gap list paper. +  * Charles gives outline for gap list paper (see below)SH: there is a specific form that needs to be filled. We need to highlight urgency, such as 'critical', or 'mission enhancing'. Perhaps 10-20 GHz would be 'mission enhancing'; do we know we can call it critical?  
 + 
 + 
 +Hi Shaul & Co.: 
 + 
 +As promised, here's a draft outline of the case for broadening the frequency range of the tech gap list on CMB detectors. 
 + 
 +1. Intro 
 +    statement of what we're writing about.  Overview or argument.  Context of space CMB mission science requirements. 
 + 
 +2. high frequency (now 600, we'll argue to raise to 800) 
 +    results of simulations, showing the improvement in CMB extraction with the addition of frequencies between 600 and 800 GHz 
 +    at least one figure.  What's the best one to use? 
 + 
 +3. low frequency (now 30, we'll argue to lower to 10) 
 +    "practical" argument from Oslo about SNR and real estate 
 +    if we have any simulation results that seem relevant, we'll use them, otherwise say that we don't yet. 
 + 
 +4. summary 
 + 
 + 
 +Charles 
 + 
  
foregroundstelecon20211013.1634786680.txt.gz · Last modified: 2021/10/20 22:24 by hanany