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Table 3
χ2-test with Nd = 15 degrees of freedom applied to the measurements of GGL shown in Fig. 3.
| Low-z | High-z | |||||||
| G11 | H15 | B06 | L12 | G11 | H15 | B06 | L12 | |
|
|
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| sm1 | 1.25 | 1.27 | 6.07 | 7.80 | 0.68 | 0.71 | 2.61 | 2.98 |
| sm2 | 0.54 | 0.56 | 4.58 | 7.97 | 1.26 | 1.23 | 3.00 | 4.58 |
| sm3 | 2.43 | 2.36 | 6.78 | 11.49 | 0.45 | 0.46 | 3.75 | 6.59 |
| sm4 | 0.93 | 1.11 | 5.37 | 7.08 | 1.11 | 1.64 | 7.09 | 7.71 |
| sm5 | 2.30 | 1.77 | 2.12 | 1.84 | 1.06 | 0.88 | 1.62 | 1.28 |
| sm6 | 1.26 | 0.97 | 1.00 | 0.92 | 1.79 | 1.63 | 1.49 | 1.55 |
|
|
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Notes. Each number quotes the reduced χ2/Nd for the corresponding model and stellar mass bin. Bold values indicate a tension between CFHTLenS and a SAM at the 95% confidence level.
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