Table 2.

Same as Table 1, but for a larger sky coverage of |$20\times 20~\mathrm{deg^2}$|⁠.

Statistics|$\langle A\rangle$||$\sigma (A)$||$\frac{|\langle A\rangle -1|}{\sigma (A)}$||$\langle A\rangle$||$\sigma (A)$||$\frac{|\langle A\rangle -1|}{\sigma (A)}$||$\langle A\rangle$||$\sigma (A)$||$\frac{|\langle A\rangle -1|}{\sigma (A)}$|
|$C_{\kappa \kappa }(\ell)$||$z_\mathrm{ s} = 1.5$|1.0011670.0329160.0354611.0012570.0329190.0381791.0017370.0329350.052733
|$z_\mathrm{ s} = 3.0$|0.9985820.0214750.0660381.0023980.0215570.1112391.0017490.0215430.081178
|$z_\mathrm{ s} = 1100$|0.9960260.0159260.2495131.0034490.0160430.2150141.0019490.0160200.121639
|$\langle \kappa ^2_{\theta } \rangle$||$z_\mathrm{ s} = 1.5$|0.9961210.0262830.1476051.0115790.0266920.4337971.0021970.0264420.083106
|$z_\mathrm{ s} = 3.0$|0.9962520.0177600.2110461.0084550.0179770.4703421.0010490.0178450.058763
|$z_\mathrm{ s} = 1100$|0.9950090.0119630.4172001.0080720.0121190.6661131.0000640.0120230.005318
|$\langle \kappa ^3_{\theta } \rangle$||$z_\mathrm{ s} = 1.5$|0.9802550.0656720.3006571.0212290.0683950.3103961.0075120.0674770.111333
|$z_\mathrm{ s} = 3.0$|0.9816690.0595310.3079181.0193020.0617840.3124191.0035990.0608400.059156
|$z_\mathrm{ s} = 1100$|0.9772130.0635010.3588421.0187590.0661430.2836100.9933240.0644920.103513
|$\langle \kappa ^4_{\theta } \rangle$||$z_\mathrm{ s} = 1.5$|0.9653300.1346650.2574561.0141150.1412570.0999211.0194900.1420710.137184
|$z_\mathrm{ s} = 3.0$|0.9774360.0842640.2677791.0124500.0870220.1430681.0099620.0869100.114628
|$z_\mathrm{ s} = 1100$|0.9894910.0416040.2526001.0147020.0425860.3452301.0025190.0421020.059836
Statistics|$\langle A\rangle$||$\sigma (A)$||$\frac{|\langle A\rangle -1|}{\sigma (A)}$||$\langle A\rangle$||$\sigma (A)$||$\frac{|\langle A\rangle -1|}{\sigma (A)}$||$\langle A\rangle$||$\sigma (A)$||$\frac{|\langle A\rangle -1|}{\sigma (A)}$|
|$C_{\kappa \kappa }(\ell)$||$z_\mathrm{ s} = 1.5$|1.0011670.0329160.0354611.0012570.0329190.0381791.0017370.0329350.052733
|$z_\mathrm{ s} = 3.0$|0.9985820.0214750.0660381.0023980.0215570.1112391.0017490.0215430.081178
|$z_\mathrm{ s} = 1100$|0.9960260.0159260.2495131.0034490.0160430.2150141.0019490.0160200.121639
|$\langle \kappa ^2_{\theta } \rangle$||$z_\mathrm{ s} = 1.5$|0.9961210.0262830.1476051.0115790.0266920.4337971.0021970.0264420.083106
|$z_\mathrm{ s} = 3.0$|0.9962520.0177600.2110461.0084550.0179770.4703421.0010490.0178450.058763
|$z_\mathrm{ s} = 1100$|0.9950090.0119630.4172001.0080720.0121190.6661131.0000640.0120230.005318
|$\langle \kappa ^3_{\theta } \rangle$||$z_\mathrm{ s} = 1.5$|0.9802550.0656720.3006571.0212290.0683950.3103961.0075120.0674770.111333
|$z_\mathrm{ s} = 3.0$|0.9816690.0595310.3079181.0193020.0617840.3124191.0035990.0608400.059156
|$z_\mathrm{ s} = 1100$|0.9772130.0635010.3588421.0187590.0661430.2836100.9933240.0644920.103513
|$\langle \kappa ^4_{\theta } \rangle$||$z_\mathrm{ s} = 1.5$|0.9653300.1346650.2574561.0141150.1412570.0999211.0194900.1420710.137184
|$z_\mathrm{ s} = 3.0$|0.9774360.0842640.2677791.0124500.0870220.1430681.0099620.0869100.114628
|$z_\mathrm{ s} = 1100$|0.9894910.0416040.2526001.0147020.0425860.3452301.0025190.0421020.059836
Table 2.

Same as Table 1, but for a larger sky coverage of |$20\times 20~\mathrm{deg^2}$|⁠.

Statistics|$\langle A\rangle$||$\sigma (A)$||$\frac{|\langle A\rangle -1|}{\sigma (A)}$||$\langle A\rangle$||$\sigma (A)$||$\frac{|\langle A\rangle -1|}{\sigma (A)}$||$\langle A\rangle$||$\sigma (A)$||$\frac{|\langle A\rangle -1|}{\sigma (A)}$|
|$C_{\kappa \kappa }(\ell)$||$z_\mathrm{ s} = 1.5$|1.0011670.0329160.0354611.0012570.0329190.0381791.0017370.0329350.052733
|$z_\mathrm{ s} = 3.0$|0.9985820.0214750.0660381.0023980.0215570.1112391.0017490.0215430.081178
|$z_\mathrm{ s} = 1100$|0.9960260.0159260.2495131.0034490.0160430.2150141.0019490.0160200.121639
|$\langle \kappa ^2_{\theta } \rangle$||$z_\mathrm{ s} = 1.5$|0.9961210.0262830.1476051.0115790.0266920.4337971.0021970.0264420.083106
|$z_\mathrm{ s} = 3.0$|0.9962520.0177600.2110461.0084550.0179770.4703421.0010490.0178450.058763
|$z_\mathrm{ s} = 1100$|0.9950090.0119630.4172001.0080720.0121190.6661131.0000640.0120230.005318
|$\langle \kappa ^3_{\theta } \rangle$||$z_\mathrm{ s} = 1.5$|0.9802550.0656720.3006571.0212290.0683950.3103961.0075120.0674770.111333
|$z_\mathrm{ s} = 3.0$|0.9816690.0595310.3079181.0193020.0617840.3124191.0035990.0608400.059156
|$z_\mathrm{ s} = 1100$|0.9772130.0635010.3588421.0187590.0661430.2836100.9933240.0644920.103513
|$\langle \kappa ^4_{\theta } \rangle$||$z_\mathrm{ s} = 1.5$|0.9653300.1346650.2574561.0141150.1412570.0999211.0194900.1420710.137184
|$z_\mathrm{ s} = 3.0$|0.9774360.0842640.2677791.0124500.0870220.1430681.0099620.0869100.114628
|$z_\mathrm{ s} = 1100$|0.9894910.0416040.2526001.0147020.0425860.3452301.0025190.0421020.059836
Statistics|$\langle A\rangle$||$\sigma (A)$||$\frac{|\langle A\rangle -1|}{\sigma (A)}$||$\langle A\rangle$||$\sigma (A)$||$\frac{|\langle A\rangle -1|}{\sigma (A)}$||$\langle A\rangle$||$\sigma (A)$||$\frac{|\langle A\rangle -1|}{\sigma (A)}$|
|$C_{\kappa \kappa }(\ell)$||$z_\mathrm{ s} = 1.5$|1.0011670.0329160.0354611.0012570.0329190.0381791.0017370.0329350.052733
|$z_\mathrm{ s} = 3.0$|0.9985820.0214750.0660381.0023980.0215570.1112391.0017490.0215430.081178
|$z_\mathrm{ s} = 1100$|0.9960260.0159260.2495131.0034490.0160430.2150141.0019490.0160200.121639
|$\langle \kappa ^2_{\theta } \rangle$||$z_\mathrm{ s} = 1.5$|0.9961210.0262830.1476051.0115790.0266920.4337971.0021970.0264420.083106
|$z_\mathrm{ s} = 3.0$|0.9962520.0177600.2110461.0084550.0179770.4703421.0010490.0178450.058763
|$z_\mathrm{ s} = 1100$|0.9950090.0119630.4172001.0080720.0121190.6661131.0000640.0120230.005318
|$\langle \kappa ^3_{\theta } \rangle$||$z_\mathrm{ s} = 1.5$|0.9802550.0656720.3006571.0212290.0683950.3103961.0075120.0674770.111333
|$z_\mathrm{ s} = 3.0$|0.9816690.0595310.3079181.0193020.0617840.3124191.0035990.0608400.059156
|$z_\mathrm{ s} = 1100$|0.9772130.0635010.3588421.0187590.0661430.2836100.9933240.0644920.103513
|$\langle \kappa ^4_{\theta } \rangle$||$z_\mathrm{ s} = 1.5$|0.9653300.1346650.2574561.0141150.1412570.0999211.0194900.1420710.137184
|$z_\mathrm{ s} = 3.0$|0.9774360.0842640.2677791.0124500.0870220.1430681.0099620.0869100.114628
|$z_\mathrm{ s} = 1100$|0.9894910.0416040.2526001.0147020.0425860.3452301.0025190.0421020.059836
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