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 9 frequencies covered by the two instruments. | HFI/LFI common processing uses as basic input the maps at the 9 frequencies covered by the two instruments. | ||
| − | The goal is to obtain various | + | 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). |
| + | |||
| + | == Catalogues == | ||
| + | |||
| + | Are described [[here]] | ||
| + | |||
| + | == Component maps== | ||
| + | |||
| + | Are described [[here]] | ||
| + | |||
| + | == Power spectra and likelihood code== | ||
| + | |||
| + | Are described [[here]] | ||
| + | |||
| + | == Simulations == | ||
| + | |||
| + | Are described [[here]] | ||
| + | |||
| + | == Sceintific analysis products == | ||
| + | |||
| + | Are described [[here]] | ||
Revision as of 18:38, 20 October 2012
HFI/LFI common processing uses as basic input the maps at the 9 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).
Contents
Catalogues[edit]
Are described here
Component maps[edit]
Are described here
Power spectra and likelihood code[edit]
Are described here
Simulations[edit]
Are described here
Sceintific analysis products[edit]
Are described here
(Planck) High Frequency Instrument
(Planck) Low Frequency Instrument
Cosmic Microwave background
