Table D.2.
Expected number of AGN detectable with Euclid photometry in the EWS and EDS, broken down into the redshift ranges 0.01 ≤ z ≤ 4 and 4 < z ≤ 7.
| Survey | Band | 0.01 ≤ z ≤ 4 | 4 < z ≤ 7 | ||||
|---|---|---|---|---|---|---|---|
| Total | Unobscured | Obscured | Total | Unobscured | Obscured | ||
| EWS | IE | 3.0 × 107 | 1.1 × 107 | 1.9 × 107 | 1.1 × 106 | 7.5 × 105 | 3.5 × 105 |
| YE | 2.1 × 107 | 8.1 × 106 | 1.3 × 107 | 8.4 × 105 | 5.8 × 105 | 2.6 × 105 | |
| JE | 2.9 × 107 | 8.9 × 106 | 2.0 × 107 | 1.0 × 106 | 7.3 × 105 | 3.1 × 105 | |
| HE | 3.4 × 107 | 9.1 × 106 | 2.5 × 107 | 1.1 × 106 | 7.8 × 105 | 3.7 × 105 | |
| (IE | YE | JE | HE) | 3.9 × 107 | 1.1 × 107 | 2.7 × 107 | 1.4 × 106 | 9.2 × 105 | 4.7 × 105 | |
| (IE ∧ YE ∧ JE ∧ HE) | 2.0 × 107 | 7.9 × 106 | 1.2 × 107 | 7.2 × 105 | 5.1 × 105 | 2.2 × 105 | |
| EDS | IE | 1.8 × 105 | 4.5 × 104 | 1.4 × 105 | 6.8 × 103 | 3.3 × 103 | 3.4 × 103 |
| YE | 1.5 × 105 | 4.0 × 104 | 1.2 × 105 | 5.3 × 103 | 3.4 × 103 | 1.9 × 103 | |
| JE | 1.9 × 105 | 4.1 × 104 | 1.5 × 105 | 6.3 × 103 | 3.7 × 103 | 2.6 × 103 | |
| HE | 2.1 × 105 | 4.2 × 104 | 1.8 × 105 | 7.6 × 103 | 3.8 × 103 | 3.8 × 103 | |
| (IE | YE | JE | HE) | 2.3 × 105 | 4.5 × 104 | 1.8 × 105 | 8.7 × 103 | 3.9 × 103 | 4.7 × 103 | |
| (IE ∧ YE ∧ JE ∧ HE) | 1.5 × 105 | 3.9 × 104 | 1.1 × 105 | 4.8 × 103 | 3.1 × 103 | 1.7 × 103 | |
Notes. The former of these ranges corresponds to where the XLF adopted in this work is well constrained by data, whilst the latter marks regions where the XLF was extrapolated. We present total numbers as well as splits by optical obscuration class. Numbers are reported on a per-filter basis as well as the number of AGN detectable in at least one Euclid filter, (IE | YE | JE | HE), and the number of AGN detectable in all Euclid filters, (IE ∧ YE ∧ JE ∧ HE).
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