Summary LFI

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

$^{ \rm a \, }$ 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 $^{ \rm b \, }$ FWHM and ellipticity from scanning beam evaluated fitting Jupiter directly in the timelines. $\hspace{50mm}$ $^{ \rm c \, }$ FWHM and ellipticity from effective beam evaluated as mean from different position on the sky. $\hspace{42mm}$ $^{ \rm d \, }$ FWHM from effective beam evaluated as FWHM$_{eff} = \sqrt{\frac{Ω}{2π}} · 2 · \sqrt{2 \log 2}$, where Ω is the mean beam solid angle of the effective beam. Those are the values used in the source extraction pipeline #planck2013-p05 Planck-2013-XXVIII

References

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1. References

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