Difference between revisions of "UMICH-2015: CMB-Lensing break-out session 2"

Revision as of 01:14, 22 September 2015

Questions for discussion

Experiment design
- Can we combine different experiments, and is it worth having two different noise levels on two experiments (high-res + low-res)
Algorithms - Quadratic Estimator / Iterative / Sampling
- What is the best algorithm to use?
- How low ell do we use/need for reconstruction?
Systematics and Delensing
- Dust foregrounds and sources - how do they propagate through the delensing procedure? How much do they matter?
- Instrumental systematics, higher order biases, LSS non-Gaussianity - any concerns for delensing?
Analysis of Delensed Maps
- What are the statistical and noise properties of the delensed maps? How to construct likelihoods?

Questions for discussion:

weak lensing calibration: cross-correlations with LSST / Euclid / ... weak lensing
- how precise are the correlations?
- is this level of multiplicative bias calibration interesting?
- are intrinsic alignments a limiting factor?
clustering from correlations with DESI/Euclid/LSST galaxies / quasars / ...
- how well can biases be modeled and constrained?
- can these observables be used cleanly and powerful enough to detect neutrino mass?
- what are the key science drivers in extragalactic astrophysics?
other surveys
- would overlap with external datasets gain from a northern site?
- is there a way to make use of cross-correlations with Ly-alpha or intensity mapping, or are the modes they probe too different?

@@ Line 16: / Line 16: @@
 ==CMB Lensing Cross-correlations==
-Blake, ~10 min, [[File:crosses.pdf]]
+[[File:crosses.pdf]]
 Questions for discussion: