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Table 1.

Discarded and quality-flagged data.

Frequency Outlier rings (a) Discarded rings (b) Discarded data (c) Relative Relative
[GHz] [%] [%] [%] total samples (d) masked samples (e)
30....... 0.71 1.88 2.62 1.119 1.095
44....... 0.57 1.76 2.19 1.120 1.098
70....... 0.71 1.89 2.84 1.114 1.091
100....... 0.97 2.17 20.00 1.167 1.163
143....... 1.16 2.36 21.53 1.167 1.160
217....... 0.95 2.16 20.98 1.221 1.209
353....... 0.90 2.08 21.78 1.179 1.174
545....... 0.89 2.06 15.93 1.068 1.066
857....... 0.93 2.11 17.76 1.019 1.015

(a)Rings with anomalous glitch rate, noise level, gain, or numerous jumps. A percentage of rings is not necessarily the same as a percentage of integration time, the ring length varies seasonally by almost a factor of 2.

(b)Total fraction of rings discarded because of outlier statistics and spacecraft events such as the sorption-cooler switchover, elevated spin-rate campaign and LFI reboot on day 1085 since launch.

(c)Total fraction of samples flagged because of pointing, jumps, cosmic-ray glitches, outlier pointing periods and spacecraft events.

(d)Ratio of total integration time in the full-frequency maps, in the sense (NPIPE / 2018).

(e)Ratio of total integration time in the full-frequency maps, in the sense (NPIPE / 2018), over the 50% of the sky with the least foregrounds. The distinction matters for LFI, because the ninth survey – included only in NPIPE – lies almost entirely in the Galactic plane.

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