|
|
Line 30: |
Line 30: |
| </biblio> | | </biblio> |
| | | |
− | [[Category:LFI data processing|009]] | + | [[Category:LFI data processing|008]] |
Revision as of 12:25, 21 May 2014
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 white noise sensitivity computed directly on the timelines, taking in account the actual mission time minus the manoeuvres and bad-science flagged data.
References[edit]
<biblio force=false>
- References
</biblio>