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Table 1.
Number of the high-z sources used in our analysis before and after applying the quality criteria (QS, Sect. 3.2) and percentages of available photometry in each wavelength window.
| Before QC |
After QC |
|||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Field | Total | Spec-z | NIR | MIRS | MIRL | FIR | Total | Spec-z | NIR | MIRS | MIRL | FIR |
| number | Percentage (%) | number | Percentage (%) | |||||||||
| CCLS | 53 | 47 | 64 | 77 | 77 | 77 | 28 | 50 | 79 | 100 | 100 | 100 |
| XMM-XXL | 54 | 52 | 91 | 78 | 50 | 37 | 39 | 44 | 95 | 82 | 49 | 39 |
| eFEDS | 42 | 57 | 45 | 100 | 79 | 26 | 22 | 82 | 73 | 100 | 73 | 41 |
| Total | 149 | 52 | 69 | 84 | 68 | 48 | 89 | 55 | 85 | 92 | 71 | 60 |
Notes. MIRS and MIRL stand for the shortest (3.4–4.6 μm) and longest (22–24 μm) MIR bands, respectively.
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