Kolmogorov cosmic microwave background sky | Astronomy & Astrophysics (A&A)

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Table 2:

The degree of randomness $\Phi$ for the CS and the NCS.
	Cold	Northern	Gauss +
	Spot	Cold Spot	noise	Gauss
l	208 $.\!\!^\circ$ 7	294 $.\!\!^\circ$ 8
b	-55 $.\!\!^\circ$ 6	60 $.\!\!^\circ$ 8
N₁	239	243	239	239
N₂	2155	2154	2157	2157
N₃	5987	5989	5983	5984
$\Phi_1$	0.02	0.03	0.17	0.15
$\Phi_2$	0.68	0.43	0.15	0.15
$\Phi_3$	0.98	0.98	0.18	0.15

The columns contain coordinates of their centers, the pixel counts within 1 $^{\circ }$ (N₁), 3 $^{\circ }$ (N₃), and 5 $^{\circ }$ (N₅) radii, and values for $\Phi$ for each region. Mean $\Phi$ for 20 simulated Gaussian maps with superposed WMAP's noise (Gauss+noise) and without noise, i.e. isotropic map.

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