Planck 2018 results
Free Access

Fig. 33.


EE (top panel) and BB (bottom panel) power spectra for synchrotron and thermal dust as computed from the Commander, SMICA, and 353 GHz frequency maps; see Planck Collaboration XI (2020) for algorithmic details. All spectra are evaluated outside the common polarization mask, over 78% of the sky. Dashed lines indicate the best-fit power-law fits for the Commander case, as reported in Table 6. Error bars indicate 3σ uncertainties. All spectra have been colour corrected to monochromatic reference frequencies of 30 GHz for synchrotron and 353 GHz for thermal dust emission, respectively.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.