Fig. 4
HFI flight results: glitch energy distribution for the three families of glitches with respect to the peak amplitude, in signal-to-noise units, for three different PSB and SWB in-flight bolometers (Planck Collaboration X 2014). The blue line is for the short glitch population, black is for long, red is for slow, and green is for total. Power laws are shown for comparison as dashed lines.
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