Difference between revisions of "LowellBB Project List"
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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]] | ||
| + | |||
| + | == 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 == | |
| − | = | + | [https://docs.google.com/spreadsheets/d/1h7lshu3siUubJa-EAoUD1ewEtwkDivaiVhaD-vqxKCE/edit#gid=454361358 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 = | + | == 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]]! | 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
- 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!
