# Summary of LFI data characteristics

$^{ \rm a \, }$ and ellipticity from scanning beam evaluated fitting Jupiter directly in the timelines. $\hspace{480mm}$ $^{ \rm b \, }$ from effective beam estimated from the main beam solid angle of the effective beam. Those are the values used in the source extraction pipeline Planck-2013-XXVIII[2]. $\hspace{70mm}$ $^{ \rm c \, }$ White noise per pixel computed from half-ring difference maps. Those values are within the 1% with the white noise sensitivity computed directly on the timelines, taking in account the actual mission time minus the manoeuvres and bad-science flagged data.