Table 5
The “t” value for the octopole as defined in de Oliveira-Costa et al. (2004) using nside = 128, calculated from the observed CMB maps (top) and after subtraction of the ISW field due to 2MASS and NVSS galaxies (middle).
| Map | “t” value | Probability (%) | |
|
|
|||
| TOH | 0.9415 | 9.60 | |
| W3 | 0.9171 | 14.3 | |
| W5 | 0.9190 | 13.8 | |
| W7 | 0.9261 | 12.7 | |
| ILC W9 | 0.9329 | 11.8 | |
| TOH W1 (inp) | 0.8917 | 23.4 | |
| W3 (inp) | 0.8820 | 26.1 | |
| W5 (inp) | 0.8886 | 24.4 | |
| W5 Dela (inp) | 0.8919 | 23.4 | |
| W7 (inp) | 0.9149 | 15.1 | |
| W9 (inp) | 0.9205 | 13.6 | |
|
|
|||
| TOH − ISW | 0.8975 | 21.8 | |
| W3 − ISW | 0.8769 | 27.5 | |
| W5 − ISW | 0.8776 | 27.4 | |
| W7 − ISW | 0.8712 | 28.8 | |
| ILC W9 − ISW | 0.8764 | 27.6 | |
| TOH W1 (inp) − ISW | 0.8086 | 46.0 | |
| W3 (inp) − ISW | 0.7928 | 50.8 | |
| W5 (inp) − ISW | 0.7998 | 48.9 | |
| W5 Dela (inp) − ISW | 0.80167 | 48.0 | |
| W7 (inp) − ISW | 0.8169 | 44.1 | |
| W9 (inp) − ISW | 0.8223 | 42.7 | |
|
|
|||
| W3-ISW (due to 2MASS) | 0.9841 | 1.6 | |
| FP10 | |||
Notes. The probability is determined from 1000 Monte-Carlo simulations and compared with results from FP10 (Francis & Peacock 2010, bottom row).
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