Difference between revisions of "HFI/LFI joint data processing"
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m (moved HL to HFI/LFI common processing) |
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Revision as of 18:54, 14 February 2013
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
Scientific analysis products[edit]
Are described here
(Planck) High Frequency Instrument
(Planck) Low Frequency Instrument
Cosmic Microwave background
