| Frequency | Meana | Lowb | Highc | Deepd | Pol. Stat.e |
| (GHz) | (s/sq. deg.) | (%) | (%) | (%) | (%) |
| 30 | 953 | 4.5 | 1.7 | 0.42 | 0.8 |
| 44 | 953 | 3.3 | 1.5 | 0.28 | 3.7 |
| 100 | 953 | 4.3 | 1.5 | 0.41 | 0.61 |
| 353 | 953 | 4.3 | 1.2 | 0.37 | 0.10 |
Notes. (a) Integration time per square degree for typical channels. (b) Fraction of the sky with integration time lower than one-half the mean value.. (c) Fraction of the sky with integration time higher than four times the mean value.(d) Fraction of the sky with integration time higher than nine times the mean value. (e)
Fraction of the sky which has a high spread of scanning angles, for all
detectors at each frequency. The value is based on dividing the 2
range of angles into 16 bins; for a pixel on the sky, the spread
is considered high if there are samples in at least 5 bins. More
details are
available in Dupac & Tauber (2005).
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