Difference between revisions of "LowellBB Project List"

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(Threads that can use more attention)
(updates to low-ell BB projects)
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Summary of low-ell BB work so far and sketch of plans forward (Oct 2019 UCSD meeting): [[https://docs.google.com/presentation/d/164NM-vBg0DvYUgGAtbZ1XgIgBNFFloOTWmcewPEsIGQ/edit?usp=sharing slides]]
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== Active projects ==
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* Bayesian r-analysis: Millea, Knox, others
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* MAP phi estimate extension to curved-sky
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* Foreground clean map for phi reconstruction: Umiltà
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* Cross-spectra parametric r-pipeline: Buza, Racine, Bischoff, Pryke, Willmert
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* ILC pipeline: Flauger
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* SO pipeline: Errard
  
Summary of low-ell BB work so far and sketch of plans forward (Oct 2019 UCSD meeting): [[https://docs.google.com/presentation/d/164NM-vBg0DvYUgGAtbZ1XgIgBNFFloOTWmcewPEsIGQ/edit?usp=sharing slides]]
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== Inputs to pre-CD1 decisions ==
  
= On-going projects =
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[https://docs.google.com/spreadsheets/d/1h7lshu3siUubJa-EAoUD1ewEtwkDivaiVhaD-vqxKCE/edit#gid=454361358 Pre-CD1 decision spreadsheet]
  
  - Bayesian r-analysis
+
* Justification for 20 GHz channel on LAT: Bischoff
  - MAP phi estimate extension to curved-sky
+
* Justification for 85/95 and 145/155 split bands: Bischoff
  - Foreground clean map for phi reconstruction
+
* Requirement for angular resolution and sensitivity of delensing LAT: Wu
  - Cross-spectra parametric r-pipeline
 
  
= Threads that can use more attention =
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== Threads that can use more attention ==
  - Impacts of Galactic foregrounds on delensing  
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  - Instrumental systematics impacts on delensing
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* Impacts of Galactic foregrounds on delensing  
  - Instrumental systematics impacts on degree-scale measurements
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* Instrumental systematics impacts on delensing
  - Field selection for the deep survey
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* Instrumental systematics impacts on degree-scale measurements
  - Forecast comparison between S4 and SO sims
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* Field selection for the deep survey
  - Development of additional foreground models/sims, and development of an approach to managing our uncertainty about foreground properties and how this impacts flowdown to design.
+
* Forecast comparison between S4 and SO sims
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* Development of additional foreground models/sims, and development of an approach to managing our uncertainty about foreground properties and how this impacts flowdown to design.
  
 
Join by working on [[Data_Challenges]]!
 
Join by working on [[Data_Challenges]]!

Revision as of 18:05, 25 February 2020

Summary of low-ell BB work so far and sketch of plans forward (Oct 2019 UCSD meeting): [slides]

Active projects

  • Bayesian r-analysis: Millea, Knox, others
  • MAP phi estimate extension to curved-sky
  • Foreground clean map for phi reconstruction: Umiltà
  • Cross-spectra parametric r-pipeline: Buza, Racine, Bischoff, Pryke, Willmert
  • ILC pipeline: Flauger
  • SO pipeline: Errard

Inputs to pre-CD1 decisions

Pre-CD1 decision spreadsheet

  • Justification for 20 GHz channel on LAT: Bischoff
  • Justification for 85/95 and 145/155 split bands: Bischoff
  • Requirement for angular resolution and sensitivity of delensing LAT: Wu

Threads that can use more attention

  • Impacts of Galactic foregrounds on delensing
  • Instrumental systematics impacts on delensing
  • Instrumental systematics impacts on degree-scale measurements
  • Field selection for the deep survey
  • Forecast comparison between S4 and SO sims
  • Development of additional foreground models/sims, and development of an approach to managing our uncertainty about foreground properties and how this impacts flowdown to design.

Join by working on Data_Challenges!