Planck early results
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Fig.14

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Typical power spectrum amplitude of bolometers 143-5 and 545-2. For the upper panels, this is the power spectrum density of valid samples, after an average ring (the sky signal) has been subtracted from the TOI. Stacking of the result for 200 rings is shown in the lower panel. Here, the instrument time response is not deconvolved from the data.

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