Planck LMC Polarization

Large Magellanic Cloud’s maps of intensity and linear polarization parameters as derived in Alina et al. 2022. The maps were derived using Planck PR3 release, at 353 GHz, nside = 1024, at the resolution of 16’ from which the foreground contribution has been subtracted using the method proposed in Alina et al. 2022. CADE distributes foreground-subtracted Stokes I, Q, and U maps and the map of the signal-to-noise ratio of the polarization fraction, after foreground subtraction.

The units for I, Q, and U are MJy/sr.