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imagerteleconnotes20180516 [2018/05/16 15:42] wenxx181imagerteleconnotes20180516 [2018/05/16 15:49] (current) wenxx181
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     * Kris argues that either option is good at some locations; we need to specify science goals before we really answer this question. Also, since we are using action-wheels, we can fairly easily adjust precession in space. This is different from Planck. Planck did have some big gaps.     * Kris argues that either option is good at some locations; we need to specify science goals before we really answer this question. Also, since we are using action-wheels, we can fairly easily adjust precession in space. This is different from Planck. Planck did have some big gaps.
     * Jacque argues that we need to compare gap size with beam size. 48 hours comes from CORE study, which has 2-min spin rate and 96-hour precession.     * Jacque argues that we need to compare gap size with beam size. 48 hours comes from CORE study, which has 2-min spin rate and 96-hour precession.
-    * +    * conclusion: the report should probably say “there are a range of considerations, for either 10 or 48 hours” 
 +    * Shaul: the fly-wheel will be able to do the change of precession; slow-motion can also be done. 
 + 
 +  * Noise Requirements vs Best Case Estimate (BCE) 
 +    * Best case estimate: not everything is most optimistic, just reasonable. 
 +    * Shaul proposed BEC/sqrt(2)*0.9 
 +      * root 2 is coming from Planck, which had achieved within 20% BCE. 
 +      * 0.9 is 90% yield of pixels; BCE is optimistic on 100%-yield assumption 
 +      * This number is for feedback loop to science teams. 
 +      * Jacques: CORE did something similar, no major impacts on science 
 + 
 +  * Noise/Bands Figure 
 +    * goal: a standard visual 
 +    * needs to clarify things, needs suggestions 
 + 
 + 
imagerteleconnotes20180516.1526503366.txt.gz · Last modified: 2018/05/16 15:42 (external edit)