Difference between revisions of "UMICH-2015: Inflation break-out session 1"
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==[[UMICH-2015:ChallengeForegrounds|Foregrounds log-book]]== | ==[[UMICH-2015:ChallengeForegrounds|Foregrounds log-book]]== | ||
*What are our latest estimates of foreground levels post-Planck? | *What are our latest estimates of foreground levels post-Planck? | ||
| − | *What simulations and tools do we have for forecasting impact on r? (details for Tuesday) | + | *What simulations and tools do we have for forecasting impact on r? (details for Tuesday, also incl delensing) |
*What are still physical unknowns? | *What are still physical unknowns? | ||
*Do we need new data at <40 GHz and >230 GHz? (and 60 GHz?) | *Do we need new data at <40 GHz and >230 GHz? (and 60 GHz?) | ||
Revision as of 09:04, 20 September 2015
Contents
Return to Inflation sessions page
B-modes challenges: foregrounds and de-lensing
Foregrounds log-book
- What are our latest estimates of foreground levels post-Planck?
- What simulations and tools do we have for forecasting impact on r? (details for Tuesday, also incl delensing)
- What are still physical unknowns?
- Do we need new data at <40 GHz and >230 GHz? (and 60 GHz?)
- How important is large sky area?
- What is the path to a convincing claim that a B-mode signal is not foregrounds?
Delensing logbook
- What is the impact of delensing on r, and on nt or BB wiggles?
- What sensitivity and resolution do we need for the lensing map?
