Table 2
Amplitude fits for a suite of alternative reconstructions of the lensing power spectrum and comparison to the baseline MV lensing power spectrum estimate.
Consistency test summary values | |||||||||||
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Low-L | Conservative | High-L | |||||||||
8 ≤ L< 40 | 40 ≤ L ≤ 400 | 400 <L ≤ 2048 | |||||||||
 ± σA | ΔMV ± σΔ | PTEΔMV=0 |  ± σA | ΔMV ± σΔ | PTEΔMV=0PTEbins | PTEbins |  ± σA | ΔMV ± σΔ | PTEΔMV=0 | PTEbins | |
|
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Individual estimator crosses | |||||||||||
TT × TT | 1.044 ± 0.111 | -0.035 ± 0.075 | 0.65 | 0.990 ± 0.032 | -0.003 ± 0.023 | 0.90 | 0.47 | 0.724 ± 0.096 | 0.058 ± 0.042 | 0.17 | 0.81 |
TT × TE | 1.000 ± 0.108 | 0.009 ± 0.070 | 0.91 | 0.969 ± 0.039 | 0.018 ± 0.028 | 0.54 | 0.12 | 0.628 ± 0.273 | 0.155 ± 0.243 | 0.52 | 0.52 |
TT × EE | 0.872 ± 0.149 | 0.137 ± 0.126 | 0.29 | 1.012 ± 0.055 | -0.025 ± 0.051 | 0.65 | 0.89 | 1.616 ± 0.448 | -0.833 ± 0.446 | 0.06 | 0.18 |
TT × EB | 1.105 ± 0.308 | -0.096 ± 0.295 | 0.76 | 0.988 ± 0.085 | -0.001 ± 0.081 | 0.99 | 0.83 | 1.118 ± 0.270 | -0.335 ± 0.269 | 0.22 | 0.48 |
TE × TE | 0.890 ± 0.194 | 0.118 ± 0.172 | 0.47 | 1.057 ± 0.079 | -0.070 ± 0.075 | 0.35 | 0.94 | 3.607 ± 1.472 | -2.824 ± 1.461 | 0.05 | 0.41 |
EE × TE | 1.067 ± 0.209 | -0.058 ± 0.194 | 0.77 | 0.995 ± 0.085 | -0.008 ± 0.080 | 0.93 | 0.77 | -0.441 ± 1.961 | 1.224 ± 1.964 | 0.54 | 0.18 |
TE × EB | 0.604 ± 0.424 | 0.405 ± 0.415 | 0.31 | 1.016 ± 0.157 | -0.029 ± 0.156 | 0.88 | 0.86 | 0.786 ± 1.235 | -0.003 ± 1.223 | 1.00 | 0.57 |
TT × TB | 0.496 ± 0.631 | 0.512 ± 0.630 | 0.42 | 0.890 ± 0.180 | 0.097 ± 0.178 | 0.59 | 0.76 | 1.413 ± 0.575 | -0.630 ± 0.571 | 0.26 | 0.06 |
EE × EE | 1.132 ± 0.407 | -0.124 ± 0.397 | 0.72 | 0.748 ± 0.189 | 0.239 ± 0.186 | 0.20 | 0.50 | 4.503 ± 5.723 | -3.720 ± 5.717 | 0.49 | 0.56 |
EE × EB | 1.530 ± 0.664 | -0.522 ± 0.659 | 0.44 | 0.643 ± 0.247 | 0.344 ± 0.246 | 0.15 | 0.20 | 4.131 ± 2.432 | -3.348 ± 2.429 | 0.19 | 0.29 |
TE × TB | 2.426 ± 0.837 | -1.417 ± 0.833 | 0.09 | 0.722 ± 0.297 | 0.266 ± 0.294 | 0.37 | 0.75 | 5.242 ± 2.431 | -4.459 ± 2.425 | 0.07 | 0.20 |
EE × TB | -0.981 ± 1.212 | 1.990 ± 1.209 | 0.10 | 1.288 ± 0.463 | -0.301 ± 0.463 | 0.52 | 0.01 | 3.154 ± 4.492 | -2.371 ± 4.482 | 0.61 | 0.81 |
EB × EB | 0.588 ± 1.819 | 0.421 ± 1.817 | 0.82 | 1.401 ± 0.522 | -0.414 ± 0.521 | 0.42 | 0.39 | -0.422 ± 2.274 | 1.205 ± 2.263 | 0.60 | 0.80 |
TB × EB | 0.887 ± 2.954 | 0.122 ± 2.947 | 0.95 | 0.618 ± 0.798 | 0.369 ± 0.798 | 0.63 | 0.34 | -2.591 ± 2.955 | 3.374 ± 2.945 | 0.26 | 0.43 |
TB × TB | 13.790 ± 8.353 | -12.781 ± 8.351 | 0.12 | -2.809 ± 2.189 | 3.796 ± 2.189 | 0.09 | 0.08 | -0.532 ± 8.268 | 1.315 ± 8.260 | 0.86 | 0.20 |
Crosses | 0.958 ± 0.097 | 0.051 ± 0.053 | 0.33 | 0.989 ± 0.033 | -0.002 ± 0.022 | 0.91 | 0.65 | 1.028 ± 0.193 | -0.245 ± 0.174 | 0.15 | 0.84 |
Pol.only | 1.252 ± 0.350 | -0.243 ± 0.339 | 0.46 | 0.761 ± 0.145 | 0.226 ± 0.142 | 0.11 | 0.39 | 1.787 ± 1.598 | -1.004 ± 1.586 | 0.53 | 0.84 |
Foreground tests | |||||||||||
143 GHz | 0.958 ± 0.096 | 0.029 ± 0.069 | 0.64 | 1.024 ± 0.034 | -0.034 ± 0.024 | 0.16 | 0.22 | 0.583 ± 0.122 | 0.198 ± 0.093 | 0.04 | 0.02 |
217 GHz | 0.941 ± 0.092 | 0.046 ± 0.077 | 0.57 | 0.963 ± 0.034 | 0.027 ± 0.024 | 0.30 | 0.71 | 0.929 ± 0.109 | -0.148 ± 0.088 | 0.08 | 0.80 |
NILC | 0.977 ± 0.073 | 0.010 ± 0.027 | 0.75 | 0.988 ± 0.026 | 0.002 ± 0.011 | 0.83 | 0.94 | 0.877 ± 0.082 | -0.096 ± 0.031 | 0.01 | 0.09 |
SEVEM TT †† | 1.015 ± 0.108 | 0.016 ± 0.053 | 0.78 | 1.000 ± 0.032 | -0.011 ± 0.017 | 0.53 | 0.63 | 0.758 ± 0.094 | -0.039 ± 0.047 | 0.40 | 0.73 |
Commander TT †† | 0.899 ± 0.124 | 0.132 ± 0.092 | 0.15 | 1.018 ± 0.038 | -0.029 ± 0.028 | 0.30 | 0.42 | 0.950 ± 0.113 | -0.230 ± 0.099 | 0.02 | 0.21 |
fsky = 0.8 | 1.009 ± 0.064 | -0.022 ± 0.028 | 0.36 | 0.987 ± 0.025 | 0.003 ± 0.009 | 0.73 | 0.14 | 0.761 ± 0.086 | 0.019 ± 0.031 | 0.57 | 0.22 |
fsky = 0.6 | 1.000 ± 0.078 | -0.014 ± 0.034 | 0.71 | 0.991 ± 0.026 | -0.000 ± 0.010 | 0.97 | 0.90 | 0.777 ± 0.091 | 0.004 ± 0.037 | 0.92 | 0.68 |
(SMICA)3353 GHz | 1.000 ± 0.133 | -0.013 ± 0.114 | 0.93 | 0.970 ± 0.048 | 0.021 ± 0.041 | 0.64 | 0.76 | 0.946 ± 0.134 | -0.165 ± 0.128 | 0.21 | 0.05 |
(SMICA)3353 GHzpol.only | 0.277 ± 0.996 | 1.016 ± 1.076 | 0.33 | 0.264 ± 0.451 | 0.531 ± 0.495 | 0.27 | 0.80 | 7.045 ± 5.895 | -5.056 ± 6.440 | 0.40 | 0.31 |
Noise tests | |||||||||||
143 × 217 GHz | 0.949 ± 0.077 | 0.038 ± 0.050 | 0.44 | 0.999 ± 0.027 | -0.008 ± 0.015 | 0.61 | 0.97 | 0.755 ± 0.095 | 0.025 ± 0.056 | 0.66 | 0.94 |
HM1 × HM2 | 1.028 ± 0.081 | -0.041 ± 0.050 | 0.39 | 0.981 ± 0.029 | 0.009 ± 0.016 | 0.63 | 0.67 | 0.827 ± 0.090 | -0.047 ± 0.058 | 0.40 | 0.88 |
Noise scaling | 0.989 ± 0.070 | -0.002 ± 0.030 | 0.93 | 0.994 ± 0.026 | -0.003 ± 0.011 | 0.73 | 1.00 | 0.779 ± 0.084 | 0.001 ± 0.037 | 0.94 | 1.00 |
Analysis choices | |||||||||||
ℓmin = 1000 | 1.136 ± 0.104 | -0.149 ± 0.081 | 0.06 | 0.990 ± 0.036 | 0.000 ± 0.029 | 1.00 | 0.08 | 0.718 ± 0.153 | 0.063 ± 0.128 | 0.57 | 0.44 |
ℓmax = 1500 | 1.013 ± 0.086 | -0.026 ± 0.060 | 0.67 | 0.985 ± 0.035 | 0.006 ± 0.022 | 0.76 | 0.19 | 0.625 ± 0.181 | 0.156 ± 0.160 | 0.41 | 0.31 |
Apodization | 1.009 ± 0.088 | -0.001 ± 0.023 | 0.98 | 0.985 ± 0.026 | 0.002 ± 0.008 | 0.85 | 0.58 | 0.753 ± 0.097 | 0.030 ± 0.042 | 0.50 | 0.91 |
Bias-hardened estimators | |||||||||||
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1.117 ± 0.120 | -0.073 ± 0.054 | 0.17 | 0.968 ± 0.039 | 0.022 ± 0.021 | 0.30 | 0.33 | 0.451 ± 0.136 | 0.273 ± 0.098 | 0.01 | 0.11 |
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1.068 ± 0.116 | -0.024 ± 0.036 | 0.52 | 0.986 ± 0.036 | 0.004 ± 0.014 | 0.79 | 0.79 | 0.651 ± 0.103 | 0.074 ± 0.035 | 0.04 | 0.09 |
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1.082 ± 0.118 | -0.038 ± 0.045 | 0.43 | 0.982 ± 0.038 | 0.008 ± 0.017 | 0.64 | 0.62 | 0.617 ± 0.107 | 0.107 ± 0.045 | 0.01 | 0.06 |
Notes. The measured overall lensing amplitude  is given for the conservative (40 ≤ L ≤ 400) multipole range, as well as the lower signal-to-noise bins on either side. The difference between the test amplitudes and the corresponding MV result (with amplitudes of ,
, and
for the three multipole ranges) is given as ΔMV. The quoted uncertainty on the difference is obtained using Monte Carlo simulations and therefore accounts for any correlations between the MV and test estimates. The PTE values are estimated by comparison of the χ2 values to the distribution from simulations. PTEs are given for the square of the overall amplitude difference, as well as for the χ2 of the difference between the bandpowers of the binned spectra.
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