Difference between revisions of "Summary LFI"

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{{DISPLAYTITLE:Summary of LFI data characteristics}}
 
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> {{P2013|2}}.
 
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> {{P2013|2}}.
  
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[[Category:LFI data processing|009]]

Revision as of 21:11, 17 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 Planck-2013-II .


Table 1. Summary of the LFI performance parameters

[math]^{ \rm a \, }[/math] FWHM and ellipticity from scanning beam evaluated fitting Jupiter directly in the timelines. [math]\hspace{480mm} [/math] [math]^{ \rm b \, }[/math] FWHM from effective beam estimated from the main beam solid angle of the effective beam. Those are the values used in the source extraction pipeline #planck2013-p05 Planck-2013-XXVIII . [math]\hspace{70mm} [/math] [math]^{ \rm c \, }[/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.


References[edit]

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  1. References

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(Planck) Low Frequency Instrument

Full-Width-at-Half-Maximum