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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- References

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