Table A.2.
Significances of REVOLVER void temperatures on wavelet-transformed SMICA maps (with quadrupole removed).
| wav. sc. | ph. sc. | Δ23 < 0 | R > Rmedian | R > Rquartile |
| 4° | 10° | 1.0σ | 1.7σ | 3.2σ |
| 4° (0.75R) | 10° | 0.7σ | 1.9σ | 3.4σ |
| 4° (0.25R) | 10° | 1.4σ | 1.6σ | 2.7σ |
| 5° | 12.5° | 1.1σ | 1.8σ | 3.3σ |
| 3° | 7.5° | 0.9σ | 1.7σ | 3.1σ |
Notes. Standard deviations are calibrated using 1000 simulated SMICA CMB maps. Results are given for different samples, wavelet scales and fractions of void radii (results given for 1/2 void radius when not otherwise specified). Note that REVOLVER voids occupy much less sky fraction than the SPARKLING voids and therefore have a much larger uncertainty in CMB temperature and measured significance.
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