Difference between revisions of "UCSD-2019: Analysis/Pipeline Working Group: Low-ell BB"
From CMB-S4 wiki
Jump to navigationJump to search (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) |
||
Line 3: | Line 3: | ||
== Charge == | == Charge == | ||
+ | # Identify key decisions that must be made (and justified) prior to CD-1, | ||
+ | # Make progress on (or actually make) those decisions, | ||
+ | # 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, | ||
+ | # 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 == | == Agenda == |
Revision as of 11:57, 8 October 2019
Contents
Charge
- Identify key decisions that must be made (and justified) prior to CD-1,
- Make progress on (or actually make) those decisions,
- 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,
- 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?