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Table 4
Predictions for different filters of the JWST telescope.
| Instr. | Filter | z | S/N CAN | S/N MKDP |
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| NIRCam | F115W | 3 | 47 | 194 |
| NIRCam | F200W | 3 | 47 | 215 |
| NIRCam | F480M | 3 | 7 | 52 |
| MIRI | F1000W | 3 | 0.4 | 4 |
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| NIRCam | F115W | 6 | 14 | 76 |
| NIRCam | F200W | 6 | 15 | 83 |
| NIRCam | F480M | 6 | 2 | 16 |
| MIRI | F1000W | 6 | 0.1 | 1 |
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| NIRCam | F115W | 9 | 6 | 36 |
| NIRCam | F200W | 9 | 7 | 42 |
| NIRCam | F480M | 9 | 1 | 7 |
| MIRI | F1000W | 9 | 0.06 | 0.5 |
Notes. All values are computed for an initial stellar mass of 108 M⊙ and for reference the CAN IMF and the MKDP IMF are considered. The S/N values can be reached within a total integration time of ≈3 h. Section 3.6 gives more details.
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