Difference between revisions of "Summary LFI"
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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>. | 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>. | ||
| − | [[File: | + | <center> |
| + | Table 1. Summary of the LFI performance parameters | ||
| + | [[File:performance.jpg|thumb|center|655px|<math>^{ a \, }</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 | ||
| + | <math>^{ b \, }</math> FWHM and ellipticity from scanning beam are evaluated fitting Jupiter directly in the timelines.]] | ||
| + | </center> | ||
== References == | == References == | ||
Revision as of 21:31, 14 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.
Table 1. Summary of the LFI performance parameters
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 FWHM and ellipticity from scanning beam are evaluated fitting Jupiter directly in the timelines.
References[edit]
<biblio force=false>
</biblio>
(Planck) Low Frequency Instrument
Full-Width-at-Half-Maximum
