Mathieu included a new figure in the draft to show spectra of foreground contamination at 22, 799 and 155 GHz for the various sky models, as compared to the level of B-modes (fig. 1)
Sebastian expanded the caption of Fig. 9. Suggestions for this figure: 1- move the QE stuff to an appendix; 2- try different color scale (from -0.25 to 0.25?) to emphasize differences betwee left and right; 3- do we need the mollviews?
Still waiting for including the lensing term in L1 and L2 —> Mathew?