![](CMB-2K_ic.jpg) |
Full sky map of the temperature anistropies of the Cosmic Microwave Background obtained from the 9 Planck channels
Credit: ESA - Planck Collaboration |
![](Planck_all_sky_dark_matter_ic.jpg) |
Full sky map of the matter distribution in the Universe at large scale, as measured using the weak gravitational lensing effect
Credit: ESA - Planck Collaboration |
![](Champ-magnetique-voie-lactee_ic.jpg) |
Visualization of the low galactic latitude 353GHz polarization which traces the magnetic field of our galaxy
Credit: ESA - Planck Collaboration |
![](LIC_3-7_ic.jpg) |
Details of the 353GHz polarization superimposed on a map of the dust temperature
Credit: ESA - Planck Collaboration - Marc-Antoine Miville-Deschênes |
![](LIC_3-8_ic.jpg) |
Details of the 353GHz polarization superimposed on a map of the dust temperature
Credit: ESA - Planck Collaboration - Marc-Antoine Miville-Deschênes |
![](Carte-estimation-signal-galactique_ic.jpg) |
Contribution of the dust induced B mode polarization at high galactic latitude, normalized to the amplitude of the BICEP2 measurement
Credit: ESA - Planck Collaboration |
![](ClTT-ClTE-ClEE_ic.jpg) |
Temperature angular anisotropies and polarisation power spectra of the Planck Cosmic Microwave Background data, and their excellent agreement with the best fitting comological model (preliminary result 2014)
Credit: ESA - Planck Collaboration |
![](Carte-SZ_ic.jpg) |
Map of the clusters and superclusters of galaxies as seen by Planck through the Sunyaev-Zeldovich effect (preliminary result 2014)
Credit: ESA - Planck Collaboration |