Fig. 16
Power spectrum of the TOI of the 143-5 bolometer, before (in black) and after (in red) the 100 mK fluctuations traced by the dark bolometers (smoothed by a 2-min box kernel) have been removed. The removal of 100 mK fluctuations affects only the very low frequencies below the first sky harmonic at fspin ≃ 0.017 Hz.
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