Table 2.
Open in new tab

Summary of all bias measurements. Bias measurements for the various sample and mask combinations, using the quasar autocorrelation (top half) and CMB lensing cross-correlations (bottom half). Measurements are made by fitting the model to the data over the range 40 < l < 400 or 0| $_{.}^{\circ}$|04 < θ < 0| $_{.}^{\circ}$|4. Samples with an asterisk have had the masks developed with both ALLSKY and ALLWISE samples applied. Values in parentheses in the bottom half are from measurements with the Planck DR1 data, and all others use the DR2 data. These results are shown in Fig. 6.

ALLSKYALLWISEALLSKY*ALLWISE*Both
Quasar autocorrelation
bq all IR2.20 ± 0.061.93 ± 0.122.01 ± 0.101.87 ± 0.121.92 ± 0.12
bq obscured2.39 ± 0.142.06 ± 0.192.41 ± 0.171.93 ± 0.212.13 ± 0.21
bq unobscured1.87 ± 0.151.86 ± 0.121.91 ± 0.151.83 ± 0.131.88 ± 0.15
CMB lensing cross-correlation
bq all IR(2.18 ± 0.17) 1.94 ± 0.14(1.95 ± 0.15) 1.82 ± 0.14(2.10 ± 0.13)1.86 ± 0.141.87 ± 0.14
bq obscured(2.27 ± 0.25) 2.06 ± 0.21(2.22 ± 0.21) 1.82 ± 0.20(2.25 ± 0.22)2.12 ± 0.222.06 ± 0.22
bq unobscured(1.85 ± 0.24) 1.78 ± 0.17(1.74 ± 0.20) 1.79 ± 0.19(1.93 ± 0.16)1.70 ± 0.191.72 ± 0.18
ALLSKYALLWISEALLSKY*ALLWISE*Both
Quasar autocorrelation
bq all IR2.20 ± 0.061.93 ± 0.122.01 ± 0.101.87 ± 0.121.92 ± 0.12
bq obscured2.39 ± 0.142.06 ± 0.192.41 ± 0.171.93 ± 0.212.13 ± 0.21
bq unobscured1.87 ± 0.151.86 ± 0.121.91 ± 0.151.83 ± 0.131.88 ± 0.15
CMB lensing cross-correlation
bq all IR(2.18 ± 0.17) 1.94 ± 0.14(1.95 ± 0.15) 1.82 ± 0.14(2.10 ± 0.13)1.86 ± 0.141.87 ± 0.14
bq obscured(2.27 ± 0.25) 2.06 ± 0.21(2.22 ± 0.21) 1.82 ± 0.20(2.25 ± 0.22)2.12 ± 0.222.06 ± 0.22
bq unobscured(1.85 ± 0.24) 1.78 ± 0.17(1.74 ± 0.20) 1.79 ± 0.19(1.93 ± 0.16)1.70 ± 0.191.72 ± 0.18
Table 2.
Open in new tab

Summary of all bias measurements. Bias measurements for the various sample and mask combinations, using the quasar autocorrelation (top half) and CMB lensing cross-correlations (bottom half). Measurements are made by fitting the model to the data over the range 40 < l < 400 or 0| $_{.}^{\circ}$|04 < θ < 0| $_{.}^{\circ}$|4. Samples with an asterisk have had the masks developed with both ALLSKY and ALLWISE samples applied. Values in parentheses in the bottom half are from measurements with the Planck DR1 data, and all others use the DR2 data. These results are shown in Fig. 6.

ALLSKYALLWISEALLSKY*ALLWISE*Both
Quasar autocorrelation
bq all IR2.20 ± 0.061.93 ± 0.122.01 ± 0.101.87 ± 0.121.92 ± 0.12
bq obscured2.39 ± 0.142.06 ± 0.192.41 ± 0.171.93 ± 0.212.13 ± 0.21
bq unobscured1.87 ± 0.151.86 ± 0.121.91 ± 0.151.83 ± 0.131.88 ± 0.15
CMB lensing cross-correlation
bq all IR(2.18 ± 0.17) 1.94 ± 0.14(1.95 ± 0.15) 1.82 ± 0.14(2.10 ± 0.13)1.86 ± 0.141.87 ± 0.14
bq obscured(2.27 ± 0.25) 2.06 ± 0.21(2.22 ± 0.21) 1.82 ± 0.20(2.25 ± 0.22)2.12 ± 0.222.06 ± 0.22
bq unobscured(1.85 ± 0.24) 1.78 ± 0.17(1.74 ± 0.20) 1.79 ± 0.19(1.93 ± 0.16)1.70 ± 0.191.72 ± 0.18
ALLSKYALLWISEALLSKY*ALLWISE*Both
Quasar autocorrelation
bq all IR2.20 ± 0.061.93 ± 0.122.01 ± 0.101.87 ± 0.121.92 ± 0.12
bq obscured2.39 ± 0.142.06 ± 0.192.41 ± 0.171.93 ± 0.212.13 ± 0.21
bq unobscured1.87 ± 0.151.86 ± 0.121.91 ± 0.151.83 ± 0.131.88 ± 0.15
CMB lensing cross-correlation
bq all IR(2.18 ± 0.17) 1.94 ± 0.14(1.95 ± 0.15) 1.82 ± 0.14(2.10 ± 0.13)1.86 ± 0.141.87 ± 0.14
bq obscured(2.27 ± 0.25) 2.06 ± 0.21(2.22 ± 0.21) 1.82 ± 0.20(2.25 ± 0.22)2.12 ± 0.222.06 ± 0.22
bq unobscured(1.85 ± 0.24) 1.78 ± 0.17(1.74 ± 0.20) 1.79 ± 0.19(1.93 ± 0.16)1.70 ± 0.191.72 ± 0.18
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