UCSD-2019: Cross-Cut: Delensing

Charge

General charge to all parallels:

We need to use the October collaboration meeting to advance our preparations for CD-1. Right away, we need to:

Identify key decisions that must be made (and justified) prior to CD-1,
Make progress on (or actually make) those decisions,
Lay out a timeline and process for making each decision, consistent with the post-decision work and internal reviews that will be needed to complete preparations for CD-1,
Ensure that those timelines and processes are understood and supported by the collaboration, and that we (together) believe we can follow them.

Specific charge to this delensing cross-cut session:

For the de-lensing LAT, what are the benefits and costs of variation in angular resolution (dish size) for legacy survey science goals?
What is minimum dish size / throughput needed for delensing? Would multiple smaller telescopes be better than one bigger one? (both r + Neff)
What are the effects of foregrounds on delensing (both for r and Neff)

1) On-going work related to delensing (50 min - 1hr):

f_NL
- Will Coulton on delensing for f_NL
Foregrounds
- Anton Baleato Lizancos on biases to delensing from CIB and EB estimator File:AntonBL S4meeting.pdf
- Marius Millea on incorporating foregrounds in Bayesian delensing
N_eff
- Selim Hotinli on delensing for N_eff

2) What are some of the questions that need answering for moving CMB-S4 to CD-1 readiness in delensing (1hr):

How map non-idealities impact delensing efficiency File:File.pdf (Toshiya Namikawa)
Discussion on instrumental systematics: need inputs from all! (Kimmy Wu)
What inputs are needed in order to address session charges discussion