Quadrant asymmetry in the angular distribution of cosmic microwave background in the Planck satellite data

L. Santos; P. Cabella; T. Villela; A. Balbi; N. Vittorio; C. A. Wuensche

doi:10.1051/0004-6361/201322943

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Volume 569 (September 2014)

A&A, 569 (2014) A75

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Table 2

Probabilities of finding in the MC simulations the σ value higher than the value found in Planck data for the SEQ and smaller than the values found for SWQ, NEQ, and NWQ in the Planck map.

Map	σ _SEQ	P1^a	σ _SWQ	P2^b	σ _NEQ	P3^c	σ _NWQ	P4^d

SMICA + Planck mask	2090.32	19.3%	543.54	32.9%	311.03	0.5%	359.67	2.4%

Notes.

^(a)

Probability of finding σ_MC> 2090.32 in any quadrant of the simulated maps.

^(b)

Probability of finding σ_MC < 543.54 in any quadrant of the simulated maps.

^(c)

Probability of finding σ_MC < 311.03 in any quadrant of the simulated maps.

^(d)

Probability of finding σ_MC < 359.67 in any quadrant of the simulated maps.

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