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 catlogues, 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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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).

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