Planck early results
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Fig.13

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Examples of raw (unprocessed) TOI for one bolometer at each of six HFI frequencies and one dark bolometer. Slightly more than two scan circles are shown. The TOI is dominated by the CMB dipole, the Galactic dust emission, point sources, and glitches. The relative contribution of glitches is over represented on these plots due to the thickness of the lines that is larger than the real glitch duration.

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