UMICH-2015: Inflation break-out session 1

From CMB-S4 wiki
Revision as of 10:24, 16 September 2015 by Dunkley (talk | contribs)
Jump to navigationJump to search

Wiki navigation

Return to main workshop page

Return to Inflation sessions page


Foregrounds

  • What are our latest estimates of foreground levels post-Planck?
  • Do we need frequencies <40 GHz and >230 GHz?
  • What tools do we have for forecasting?
  • How much sky?

Delensing

  • 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?

Foregrounds

  • What are our latest estimates of foreground levels post-Planck?(Steve Choi, Joaquin Errard)
  • Do we need frequencies <40 GHz and >230 GHz? (Jo)
  • What tools do we have for forecasting?

Delensing

  • What is the impact of delensing on r, and on nt? (Blake Sherwin)
  • How does internal CMB delensing compare to external (e.g. CIB)?
  • What sensitivity and resolution do we need for the lensing map?
Retrieved from "https://cmb-s4.uchicago.edu/wiki/index.php?title=UMICH-2015:_Inflation_break-out_session_1&oldid=208"