Table 6
Sky coverage (as a percentage) of full-mission, single-year, and single-survey frequency maps.
30 GHz | 44 GHz | 70 GHz | ||||||||
Survey | Pid rangea | Map | Scan | Destriping | Map | Scan | Destriping | Map | Scan | Destriping |
|
||||||||||
Full .............. | 3–44072 | 100.0 | 100.0 | 78.74 | 100.0 | 100.0 | 89.37 | 100.0 | 100.0 | 89.67 |
Year 1 .......... | 3–10957 | 99.999 | 100.0 | 78.74 | 99.998 | 100.0 | 89.37 | 100.0 | 100.0 | 89.67 |
Year 2 .......... | 10 958–21482 | 99.98 | 100.0 | 78.74 | 99.998 | 100.0 | 89.37 | 100.0 | 100.0 | 89.67 |
Year 3 .......... | 21 483–32761 | 99.72 | 99.74 | 78.66 | 99.91 | 100.0 | 89.37 | 99.65 | 99.65 | 89.38 |
Year 4 .......... | 32 762–44072 | 95.68 | 95.76 | 76.61 | 96.87 | 98.68 | 88.35 | 97.38 | 97.43 | 87.63 |
Survey 1 ....... | 3– 5483 | 97.20 | 98.11 | 76.88 | 93.93 | 98.03 | 87.41 | 97.94 | 97.95 | 87.62 |
Survey 2 ....... | 5484–10957 | 97.48 | 97.58 | 77.40 | 93.31 | 98.13 | 87.89 | 97.47 | 97.49 | 87.62 |
Survey 3 ....... | 10 958–16454 | 97.62 | 97.71 | 76.49 | 93.65 | 98.23 | 87.61 | 97.61 | 97.63 | 87.30 |
Survey 4 ....... | 16 455–21482 | 91.88 | 91.98 | 72.37 | 89.53 | 94.92 | 84.85 | 92.40 | 92.43 | 82.89 |
Survey 5 ....... | 21 483–27404 | 90.89 | 91.02 | 70.27 | 88.43 | 96.70 | 86.08 | 92.44 | 92.50 | 82.33 |
Survey 6 ....... | 27 405–32761 | 87.79 | 88.06 | 72.35 | 86.10 | 94.56 | 85.29 | 89.95 | 90.18 | 82.04 |
Survey 7 ....... | 32 762–38574 | 85.40 | 85.60 | 68.29 | 83.70 | 92.49 | 82.80 | 88.43 | 88.52 | 79.65 |
Survey 8 ....... | 38 575–44072 | 80.01 | 80.26 | 67.54 | 78.92 | 89.61 | 81.15 | 83.83 | 84.09 | 77.05 |
Notes. We give the pointing period (Pid) range for each survey combination, the sky coverage of the final map (“map”), the area that was scanned by at least one horn (“scan”) and is available for destriping, and the area that remains after applying a Galactic mask and that was used for destriping (“destriping”). Since the full-mission data set covers the full sky, the coverage of the destriping mask can be read from the intersection of the “full” (mission) row and the “destriping” column.
Pid is a counter for pointings of the spin axis, which had an average duration of about 45 minutes (see Planck Collaboration I 2014, for the explicit definition).
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