Difference between revisions of "HFI/LFI joint data processing"
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| − | HFI/LFI common processing uses as basic input the maps at 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 provides a statistical characterisation of the CMB, in particular through a likelihood code (of a particular theoretical C(l) given Planck data). | The goal is to obtain various catalogues, identify the different astrophysical components whose superposition leads to the observed sky, and provides a statistical characterisation of the CMB, in particular through a likelihood code (of a particular theoretical C(l) given Planck data). | ||
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[[Category:Data processing|006]] | [[Category:Data processing|006]] | ||
Revision as of 14:17, 14 March 2013
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 provides a statistical characterisation of the CMB, in particular through a likelihood code (of a particular theoretical C(l) given Planck data).
(Planck) High Frequency Instrument
(Planck) Low Frequency Instrument
Cosmic Microwave background
