Secondary CMB Anisotropy - Wayne Hu's Tutorials
Secondary CMB Anisotropy - Wayne Hu's Tutorials
Secondary CMB Anisotropy - Wayne Hu's Tutorials
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Lensing Observables<br />
• Lensing observables provide a simple way of accounting for<br />
non-Gaussianity and parameter degeneracies<br />
• Observables forecasts for Planck + 10% sky with noise ∆ P=1.4uK'<br />
w<br />
Smith, Hu, Kaplinghat (2006)<br />
-0.5<br />
-1<br />
-1.5<br />
observables<br />
-0.4<br />
Θ 1<br />
Θ 2<br />
unlensed<br />
-0.2 0 0.2 0.4 0.6<br />
Σ m ν (eV)
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