![\begin{figure}
\par\includegraphics[width=8cm,clip]{0185fig1.ps} \end{figure}](/articles/aa/full/2004/20/aa0185/Timg41.gif) |
Figure 1:
The
dependence of the time domain constraint on relative offsets as a
function of the low frequency marginalization threshold (
). Three curved lines correspond to the fiducial LFI, HFI
and HFI-like white noise cases, respectively from top to bottom.
For comparison, the nearly horizontal lines show the noise per
beam-size ring pixel for LFI (top line) and HFI (bottom). The dotted
vertical line shows the spin frequency of the PLANCK satellite.
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