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Table 3
Summary of ratios of Planck 70 and 100 GHz and WMAP V- and W-band power spectra appearing in this paper.
| Spectrum ratios | ||||||
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| Location | Features | f sky | ℓ Range | 70/V | 100/W | 100/(V + W) |
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| Sect. 6.1, Fig. 20 ..... | No corrections | 56.7% | 70 ≤ ℓ ≤ 390 | 0.983 | 0.979 | ... |
| 110 ≤ ℓ ≤ 310 | 0.981 | 0.977 | ... | |||
| Sect. 6.1, Fig. 21 ..... | Near-sidelobe (NS) correction, 100 GHz | 56.7% | 70 ≤ ℓ ≤ 390 | 0.983 | 0.983 | ... |
| 110 ≤ ℓ ≤ 310 | 0.981 | 0.981 | ... | |||
| Sect. 6.1, Fig. 22 ..... | Discrete-source residual+NS corrections | 56.7% | 70 ≤ ℓ ≤ 390 | 0.983 | 0.983 | ... |
| 110 ≤ ℓ ≤ 310 | 0.981 | 0.981 | ... | |||
| Sect. 6.2 ......... | Likelihood “calibration factor”; WMAP full-mission maps at Nside = 512 rather than yearly maps at Nside = 1024; Planck detector sets (see Sect. 5) rather than full-frequency half-ring data. | 56.7% | 50 ≤ ℓ ≤ 400 | 0.978 | 0.976 | 0.974 |
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