|
Full sky map of the temperature anistropies of the Cosmic Microwave Background obtained from the 9 Planck channels
Credit: ESA - Planck Collaboration |
|
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 |
|
Visualization of the low galactic latitude 353GHz polarization which traces the magnetic field of our galaxy
Credit: ESA - Planck Collaboration |
|
Details of the 353GHz polarization superimposed on a map of the dust temperature
Credit: ESA - Planck Collaboration - Marc-Antoine Miville-Deschênes |
|
Details of the 353GHz polarization superimposed on a map of the dust temperature
Credit: ESA - Planck Collaboration - Marc-Antoine Miville-Deschênes |
|
Contribution of the dust induced B mode polarization at high galactic latitude, normalized to the amplitude of the BICEP2 measurement
Credit: ESA - Planck Collaboration |
|
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 |
|
Map of the clusters and superclusters of galaxies as seen by Planck through the Sunyaev-Zeldovich effect (preliminary result 2014)
Credit: ESA - Planck Collaboration |