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Planck 2015 results
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Table 8

Goodness-of-fit statistics for the temperature analysis evaluated at 1deg FWHM.

Rms outside LM93 Frac. res.
inside
Map [μK] LM93 [%]
Planck 30 1.56 0.55 0.08
44 .................................... 2.51 0.83 0.42
70-ds1 .................................. 3.67 0.96 0.78
70-ds2 .................................. 3.88 0.97 0.82
70-ds3 .................................. 3.98 0.97 0.80
100-ds1 ............................... 1.00 1.11 0.18
100-ds2 ............................... 0.61 0.76 0.08
143-ds1 ............................... 0.72 1.02 0.08
143-ds2 ................................ 0.68 0.97 0.08
143-5 .................................... 1.03 1.14 0.15
143-6 .................................... 1.17 1.06 0.12
143-7 .................................... 1.04 1.04 0.10
217-1 .................................... 1.70 0.94 0.06
217-2 .................................... 1.90 1.00 0.09
217-3 .................................... 1.68 0.98 0.08
217-4 .................................... 1.64 0.91 0.05
353-ds2 ................................ 4.28 0.95 0.03
353-1 .................................... 2.11 0.60 0.02
545-2 .................................... 8.89a 0.88 0.14
545-4 .................................... 9.04a 0.90 0.13
857-2 .................................... 1.39a 0.13 0.00
WMAP K ........................... 2.26 0.38 0.03
Ka .................................... 4.52 1.05 0.56
Q1 .................................... 5.22 0.98 0.64
Q2 .................................... 5.09 0.99 0.67
V1 .................................... 6.29 0.98 1.70
V2 .................................... 5.62 1.02 1.37
W1 .................................... 7.90 0.89 1.44
W2 .................................... 9.74 0.96 1.74
W3 .................................... 9.57 0.90 1.67
W4 .................................... 10.15 1.00 1.77
Haslam 0.408 ................... 0.12b 0.10 0.03

Notes. The second column shows the rms residual outside the 93% Commander likelihood mask for each channel, while the third column shows the same, but normalized with respect to the instrumental noise rms listed in Table 1. The fourth column lists the median fractional residual in the complementary 7% of the sky, covering the Galactic plane region.

(a)

Unit is kJy sr-1.

(b)

Unit is K.

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