Difference between revisions of "UMICH-2015: Inflation break-out session 1"
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*What is the impact of delensing on r, and on nt? | *What is the impact of delensing on r, and on nt? | ||
*How does internal CMB delensing compare to external (e.g. CIB)? | *How does internal CMB delensing compare to external (e.g. CIB)? | ||
| + | *How important is it to have lensing map from the same instrument? | ||
*What sensitivity and resolution do we need for the lensing map? | *What sensitivity and resolution do we need for the lensing map? | ||
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Revision as of 15:48, 17 September 2015
B-modes challenges: foregrounds and de-lensing
Return to Inflation sessions page
Foregrounds
- What are our latest estimates of foreground levels post-Planck?
- What simulations and tools do we have for forecasting impact on r?
- What are still physical unknowns?
- Do we need new data at <40 GHz and >230 GHz?
- How important is large sky area?
Delensing
- What is the impact of delensing on r, and on nt?
- How does internal CMB delensing compare to external (e.g. CIB)?
- How important is it to have lensing map from the same instrument?
- What sensitivity and resolution do we need for the lensing map?
(This is the space to add your name and upload figures)
Foregrounds
- What are our latest estimates of foreground levels post-Planck? (Steve, Raphael...)
Can we make a new version of this figure: Attach:oldFG.png
- What simulations and tools do we have for forecasting impact on r? (Jacques, Raphael, Stephen F, Aurelien, Jo)
- What are still physical unknowns?
- Do we need new data at <40 GHz and >230 GHz? (Jo)
- How important is large sky area?
Delensing (Blake Sherwin, Olivier Dore, Chris Sheehy, Josquin Errard, Stephen Feeney)
- What is the impact of delensing on r, and on nt?
- How does internal CMB delensing compare to external (e.g. CIB)?
- What sensitivity and resolution do we need for the lensing map?
