Difference between revisions of "Summary LFI"

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The LFI performance are summarized in Table 1 below. All the details can be found in the LFI data processing paper <cite>#planck2013-p02</cite>.
 
The LFI performance are summarized in Table 1 below. All the details can be found in the LFI data processing paper <cite>#planck2013-p02</cite>.
  
[[File:LFIperformance.jpg|thumb|center|600px|Table 1. The LFI performance]]  
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<center>
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Table 1. Summary of the LFI performance parameters
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[[File:performance.jpg|thumb|center|655px|<math>^{ a \, }</math> White noise per pixel computed from half-ring difference maps. Those values are within the 1% with the withe noise sensitivity computed directly on the timelines, taking in account the actual mission time minus the manoeuvres and bad-science flagged data
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<math>^{ b \, }</math> FWHM and ellipticity from scanning beam are evaluated fitting Jupiter directly in the timelines.]]
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</center>
  
 
== References ==
 
== References ==

Revision as of 21:31, 14 March 2013

The LFI performance are summarized in Table 1 below. All the details can be found in the LFI data processing paper #planck2013-p02.

Table 1. Summary of the LFI performance parameters

[math]^{ a \, }[/math] White noise per pixel computed from half-ring difference maps. Those values are within the 1% with the withe noise sensitivity computed directly on the timelines, taking in account the actual mission time minus the manoeuvres and bad-science flagged data [math]^{ b \, }[/math] FWHM and ellipticity from scanning beam are evaluated fitting Jupiter directly in the timelines.

References[edit]

<biblio force=false>

  1. References

</biblio>

(Planck) Low Frequency Instrument

Full-Width-at-Half-Maximum