Review Article
Testing Gaussianity, Homogeneity, and Isotropy with the Cosmic Microwave Background
Table 2
Final probabilities of obtaining, in a random
CDM Universe, a chi-square value smaller or equal to
, as given by full-sky temperature maps.
| | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 |
| | 2 | 81.1% | 73.7% | 54.1% | 6.1% | 80.7% | 46.4% | 36.9% | 47.5% | 81.8% | | 4 | 74.0% | 72.6% | 55.0% | 39.6% | 74.2% | 93.2% | 51.6% | 55.4% | 56.3% | | 6 | 78.1% | 80.7% | 69.3% | 52.3% | 33.6% | 80.0% | 95.0% | 50.3% | 82.2% | | 8 | 63.5% | 87.7% | 18.8% | 51.5% | 21.4% | 66.4% | 31.6% | 27.5% | 82.3% | | 10 | 67.9% | 50.0% | 61.0% | 8.7% | 37.7% | 59.5% | 36.6% | 29.2% | 35.7% |
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