Planck 2015 results
Free Access

Fig. 43


Thermal dust polarization fraction for Galactic emission zero-level corrections of 0 μK (top) and 34 μK (bottom). A value of 34 μK corresponds to our current best estimate of the residual zodiacal light offset in the 353 GHz channel (Planck Collaboration VIII 2016). The statistical uncertainty on the Galactic emission zero-level from H i cross-correlation is 0.0067 MJy sr-1 or 23μKCMB.

This figure is made of several images, please see below:

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.