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Table 2
Summary of ratios of Planck 70, 100, and 143 GHz power spectra appearing in this paper.
| Spectrum Ratios | |||||
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| Location | Features | f sky | ℓ Range | 70/100 | 143/100 |
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| Sect. 3.4, Fig. 6, bottom centre ..... | No corrections | 59.6% | 70 ≤ ℓ ≤ 390 | 1.0089 | 1.0039 |
| 70 ≤ ℓ ≤ 830 | 1.0140 | 1.0020 | |||
| Sect. 3.4, Fig. 9 ........... | DSRa correction | 59.6% | 70 ≤ ℓ ≤ 390 | 1.0080 | 1.0045 |
| 70 ≤ ℓ ≤ 830 | 1.0094 | 1.0043 | |||
| Sect. 3.4, SMICA ........... | Paper VI, Fig. 35 | 40%d | 50 ≤ ℓ ≤ 300 | 1.0060 | 1.0020 |
| 300 ≤ ℓ ≤ 700 | 1.0075 | 1.0020 | |||
| Sect. 4.3, Fig. 12 ........... | NSc correction | 59.6% | 70 ≤ ℓ ≤ 390 | 1.0052 | 1.0040 |
| 70 ≤ ℓ ≤ 830 | 1.0077 | 1.0020 | |||
| Sect. 4.3, Fig. 13 ........... | DSRa+NSc corrections | 59.6% | 70 ≤ ℓ ≤ 390 | 1.0043 | 1.0046 |
| 70 ≤ ℓ ≤ 830 | 1.0032 | 1.0043 | |||
| Sect. 5, Fig. 14 ........... | CamSpecLikelihoodd | ... | ... | ... | 1.00058 |
Notes.
(b)
The mask used in Paper VI, Fig. 35 was similar but not identical to the 39.7% mask of Fig. 1. The differences do not affect the comparison.
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