Difference between revisions of "HFI/LFI joint data processing"
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The HFI / LFI common processing uses as basic input the maps at the nine frequencies covered by the two instruments. | The HFI / LFI common processing uses as basic input the maps at the nine frequencies covered by the two instruments. | ||
| − | The goal is to obtain various catalogues, identify the different astrophysical components whose superposition leads to the observed sky, and provide a statistical | + | The goal is to obtain various catalogues, identify the different astrophysical components whose superposition leads to the observed sky, and provide a statistical characterization of the CMB, in particular through a likelihood code (of a particular theoretical <i>C</i><sub>ℓ</sub> given Planck data). |
[[Category:HFI/LFI joint data processing|000]] | [[Category:HFI/LFI joint data processing|000]] | ||
Revision as of 23:35, 11 January 2017
The HFI / LFI common processing uses as basic input the maps at the nine frequencies covered by the two instruments.
The goal is to obtain various catalogues, identify the different astrophysical components whose superposition leads to the observed sky, and provide a statistical characterization of the CMB, in particular through a likelihood code (of a particular theoretical Cℓ given Planck data).
(Planck) High Frequency Instrument
(Planck) Low Frequency Instrument
Cosmic Microwave background
