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Fig. C.4.

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Full sky angular power spectra of the moment maps of d12. All the auto-spectra of the expansion up to second order are represented on the left panel while the dominant terms of the (absolute values of the) cross-spectra on the right panel. The full lines represent the BB spectra while the dashed lines represent the EE spectra. The spectra are expressed in units of ( μ K CMB ) 2 · K 2 α T $ (\mu {\mathrm {K}}_{CMB})^2\cdot {\mathrm {K}}^{-2\alpha _{{\cal {{T}}}}} $ where α T $ \alpha _{{\cal {{T}}}} $ is the order of the moment with respect to T $ {\cal {{T}}} $.

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