Differences
This shows you the differences between two versions of the page.
| Next revision Both sides next revision | |||
|
planck_lmc_polarization [2022/11/29 15:28] Déborah Paradis created |
planck_lmc_polarization [2022/11/29 15:29] Déborah Paradis |
||
|---|---|---|---|
| Line 2: | Line 2: | ||
| Large Magellanic Cloud’s maps of intensity and linear polarization parameters as derived in Alina et al. 2022. | 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. | + | 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. | 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. | The units for I, Q, and U are MJy/sr. | ||