Table 4.
Values of the slope of the luminosity function used in computing the magnification bias correction.
| Bin i | Central redshift | Slope si |
|---|---|---|
| 1 | 0.2095 | 0.108 |
| 2 | 0.489 | 0.180 |
| 3 | 0.619 | 0.229 |
| 4 | 0.7335 | 0.279 |
| 5 | 0.8445 | 0.335 |
| 6 | 0.9595 | 0.400 |
| 7 | 1.087 | 0.480 |
| 8 | 1.2395 | 0.586 |
| 9 | 1.45 | 0.753 |
| 10 | 2.038 | 1.335 |
Notes. These are calculated at the central redshift of each tomographic bin. The limiting magnitude is taken to be 24.5, and the slopes are calculated with a fitting function (Euclid Collaboration 2022b) determined from the Euclid Flagship simulation.
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