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Table E.1.

Redshift-dependent performance of Euclid photometry AGN selection criteria (Euclid Collaboration: Bisigello et al. 2024) applied to our samples of EWS and EDS AGN.

Survey Target Class Photometry Redshift Selected AGN C log10(Lbol/erg s−1)
EWS Unobscured AGN Euclid 0.0 ≤ z < 0.5 2.1 × 105 0.13 43.6 ± 0.6
0.5 ≤ z < 1.0 7.3 × 105 0.13 44.4 ± 0.7
1.0 ≤ z < 1.5 1.2 × 106 0.24 45.2 ± 0.6
1.5 ≤ z < 2.0 1.2 × 106 0.37 45.4 ± 0.5
2.0 ≤ z < 2.5 7.2 × 105 0.39 45.6 ± 0.5
2.5 ≤ z < 3.0 3.9 × 105 0.34 45.8 ± 0.4
3.0 ≤ z < 3.5 2.1 × 105 0.29 45.8 ± 0.4
3.5 ≤ z < 4.0 9.9 × 104 0.22 45.9 ± 0.4
4.0 ≤ z < 4.5 3.6 × 104 0.12 45.9 ± 0.3
4.5 ≤ z < 5.0 2.0 × 103 0.01 45.8 ± 0.2
5.0 ≤ z < 5.5 3 0.00 45.7 ± 0.1
EWS ∪ Euclid, Rubin/LSST 0.0 ≤ z < 0.5 4.3 × 105 0.26 43.6 ± 0.6
0.5 ≤ z < 1.0 1.7 × 106 0.28 44.1 ± 0.7
1.0 ≤ z < 1.5 2.1 × 106 0.38 44.9 ± 0.6
1.5 ≤ z < 2.0 2.0 × 106 0.56 45.3 ± 0.5
2.0 ≤ z < 2.5 1.1 × 106 0.53 45.5 ± 0.5
2.5 ≤ z < 3.0 5.2 × 105 0.44 45.7 ± 0.4
3.0 ≤ z < 3.5 2.1 × 105 0.29 45.8 ± 0.4
3.5 ≤ z < 4.0 9.9 × 104 0.22 45.9 ± 0.4
4.0 ≤ z < 4.5 3.6 × 104 0.12 45.9 ± 0.3
4.5 ≤ z < 5.0 2.0 × 103 0.01 45.8 ± 0.2
5.0 ≤ z < 5.5 3 0.00 45.7 ± 0.1
EDS Unobscured AGN Euclid 0.0 ≤ z < 0.5 3.0 × 102 0.04 43.5 ± 0.5
0.5 ≤ z < 1.0 2.4 × 103 0.06 44.0 ± 0.7
1.0 ≤ z < 1.5 5.5 × 103 0.13 44.7 ± 0.7
1.5 ≤ z < 2.0 4.5 × 103 0.17 45.2 ± 0.7
2.0 ≤ z < 2.5 2.5 × 103 0.17 45.4 ± 0.6
2.5 ≤ z < 3.0 1.2 × 103 0.14 45.6 ± 0.4
3.0 ≤ z < 3.5 6.5 × 102 0.13 45.6 ± 0.4
3.5 ≤ z < 4.0 2.2 × 102 0.08 45.6 ± 0.4
4.0 ≤ z < 4.5 78 0.04 45.9 ± 0.3
EDS ∪ Euclid, Rubin/LSST 0.0 ≤ z < 0.5 1.5 × 103 0.23 43.5 ± 0.5
0.5 ≤ z < 1.0 6.2 × 103 0.15 43.9 ± 0.7
1.0 ≤ z < 1.5 7.5 × 103 0.18 44.7 ± 0.7
1.5 ≤ z < 2.0 9.4 × 103 0.35 45.0 ± 0.6
2.0 ≤ z < 2.5 6.4 × 103 0.43 45.2 ± 0.6
2.5 ≤ z < 3.0 2.6 × 103 0.30 45.4 ± 0.5
3.0 ≤ z < 3.5 6.8 × 102 0.14 45.6 ± 0.4
3.5 ≤ z < 4.0 2.2 × 102 0.08 45.6 ± 0.4
4.0 ≤ z < 4.5 78 0.04 45.9 ± 0.3

Notes. For the Euclid-only unobscured AGN criterion and union (∪) of all Euclid and Rubin/LSST selection criteria we report the number of selected AGN, completeness (C) at the 5σ level in the relevant filters, and the median bolometric luminosity (±1σ) in each redshift bin. These data are visualised in Fig. 13.

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