Difference between revisions of "CMB halo lensing sensitivity as a function of map sensitivity and resolution"
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Latest revision as of 10:32, 15 March 2017
The following figures (shown at the 2016 Chicago CMB-S4 meeting) give our estimate of CMB halo lensing mass uncertainty for different estimators of as a function CMB map sensitivity and angular resolution.
Figure: Pure polarization estimators are flat with angular resolution, implying that gains on sigma8(z) from angular resolution in this case will be due to better Poisson statistics of the cluster catalog.