Difference between revisions of "UCSD-2019: Analysis/Pipeline Working Group: Low-ell BB"

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(Created page with "[https://cmb-s4.org/wiki/index.php/UCSD-2019:_Cosmology_with_CMB-S4#Agenda Link back to agenda] == Charge == == Agenda == == Notes ==")
 
(Charge)
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== Charge ==
 
== Charge ==
  
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# Identify key decisions that must be made (and justified) prior to CD-1,
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# Make progress on (or actually make) those decisions,
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# Lay out a timeline and process for making each decision, consistent with the post-decision work and internal reviews that will be needed to complete preparations for CD-1,
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# Ensure that those timelines and processes are understood and supported by the collaboration, and that we (together) believe we can follow them.
  
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=== Key Issues ===
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* How do we optimize detector allocation across frequency in the face of uncertainty about foreground properties, for both the SATs and the delensing LAT?
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* What are the advantages of split bands? How does performance compare to non-split bands?
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* Do we need a 20 GHz channel on delensing LAT (for SAT science)
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* How well will de-lensing work in practice?
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* What are the necessary analysis tools to answer these questions?
  
 
== Agenda ==
 
== Agenda ==

Revision as of 10:57, 8 October 2019

Link back to agenda

Charge

  1. Identify key decisions that must be made (and justified) prior to CD-1,
  2. Make progress on (or actually make) those decisions,
  3. Lay out a timeline and process for making each decision, consistent with the post-decision work and internal reviews that will be needed to complete preparations for CD-1,
  4. Ensure that those timelines and processes are understood and supported by the collaboration, and that we (together) believe we can follow them.

Key Issues

  • How do we optimize detector allocation across frequency in the face of uncertainty about foreground properties, for both the SATs and the delensing LAT?
  • What are the advantages of split bands? How does performance compare to non-split bands?
  • Do we need a 20 GHz channel on delensing LAT (for SAT science)
  • How well will de-lensing work in practice?
  • What are the necessary analysis tools to answer these questions?

Agenda

Notes