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Table 1.

Main features of the C IV emitters.

ID Dec [J2000] RA [J2000] z AGN He II C III] O III] C IV EW0 [Å]
CDFS000303 −27.937461 53.069643 3.6137 × < 0.6 1.2 ± 0.3 < 1.2 1.0 ± 0.2 3.7 ± 0.9
CDFS003839 −27.875749 53.144602 3.458 ✓ 1.6 ± 0.6 < 1.2 < 2.2 3.4 ± 0.8 14 ± 3
CDFS006327 −27.850722 53.178278 3.4937 ✓ 1.4 ± 0.4 1.0 ± 0.4 < 0.6 1.7 ± 0.4 7.8 ± 1.7
CDFS012637 −27.795843 53.122588 3.4655 ? < 0.8 1.3 ± 0.4 < 1.8 1.6 ± 0.5 6 ± 2
CDFS014277 −27.785081 53.231559 3.3616 × < 1.2 4.4 ± 1.5 < 1.8 5.9 ± 0.7 9.8 ± 1.3
CDFS021733 −27.724985 53.055324 3.1087 × < 1.7 < 3 < 1.9 6.2 ± 1.4 29 ± 8
CDFS021776 −27.724619 53.098507 4.741 × < 2.0 − < 4.0 2.6 ± 0.8 13 ± 5
CDFS025178 −27.689563 53.184370 2.806 ? < 1.4 < 1.6 < 1.9 4.4 ± 0.9 5.1 ± 1.0
CDFS025760 −27.696507 53.069094 4.79 × 92 ± 5 − 67 ± 14 32 ± 3 20 ± 2
CDFS028933 −27.848752 53.029622 3.7795 × < 1.0 1.9 ± 0.3 < 1.0 2.2 ± 0.2 9.4 ± 1.0
CDFS029763 −27.825989 53.238443 3.105 ? < 0.4 < 0.5 0.8 ± 0.2 0.7 ± 0.3 8 ± 3
CDFS032490 −27.754031 53.219545 3.0747 ? < 0.6 1.1 ± 0.4 < 0.4 1.1 ± 0.4 9 ± 3
CDFS128455 −27.745586 53.003635 3.4813 × < 1.5 3.9 ± 1.2 < 2.1 7 ± 3 3.5 ± 1.4
CDFS202937 −27.963161 53.218947 3.735 ✓ 4.2 ± 0.6 3.1 ± 0.8 < 2.1 4.3 ± 0.6 8.9 ± 1.3
CDFS203861 −27.956412 53.215551 4.7502 × < 5.0 − < 3.8 5.0 ± 1.7 19 ± 7
CDFS203989 −27.955446 53.019099 3.1366 × 1.4 ± 0.4 4.1 ± 0.5 1.8 ± 0.3 4.5 ± 0.7 8.8 ± 1.4
CDFS208175 −27.923411 53.266337 3.462 ? < 1.4 1.1 ± 0.4 < 1.8 3.6 ± 1.2 3.8 ± 1.3
CDFS209144 −27.916473 53.070682 4.4286 × < 2.0 − < 1.9 2.5 ± 0.9 8 ± 3.1
CDFS212043 −27.894033 52.994478 3.395 × < 1.6 4.2 ± 0.8 < 1.4 2.9 ± 0.9 3.4 ± 1.1
CDFS231741 −27.747690 53.287112 4.0068 × < 0.9 3.6 ± 1.2 2.8 ± 0.6 2.9 ± 0.7 6.3 ± 1.4
CDFS247279 −27.676973 53.206236 3.2959 × < 1.8 4.0 ± 0.6 < 2.6 4.3 ± 0.8 7.4 ± 1.5
CDFS009384⋆ −27.823526 53.078521 3.5480 × 0.8 ± 0.2 < 1.6 < 1.5 0.33 ± 0.11 1.1 ± 0.4
CDFS025002⋆ −27.688314 53.066713 3.7915 ? < 1.6 1.7 ± 0.8 < 19 1.9 ± 0.5 4.4 ± 1.3
UDS000184 −5.275796 34.489558 4.3722 × < 2.7 < 15 6.6 ± 1.1 6.5 ± 1.3 10 ± 2
UDS003724 −5.255394 34.395118 3.4616 × < 1.3 3.8 ± 0.9 < 4.4 4.5 ± 0.7 7.6 ± 1.2
UDS018872 −5.171582 34.371472 4.8799 × < 3.7 − < 5.4 3.3 ± 1.1 10 ± 4
UDS020394 −5.163315 34.535879 3.3018 × < 1.1 3.9 ± 0.4 < 5.0 2.5 ± 0.8 5.1 ± 1.6
UDS021234 −5.158691 34.420972 4.6008 × 2.2 ± 0.6 − < 15 5.7 ± 1.0 17 ± 4
UDS021291 −5.158290 34.295009 3.625 × < 0.9 2.6 ± 1.0 < 1.3 1.9 ± 0.6 5.5 ± 1.9
UDS033733 −5.162411 34.406837 3.1424 × < 0.8 < 1.5 < 0.6 1.4 ± 0.5 12 ± 5
UDS034251 −5.153870 34.581079 3.61 ? < 1.3 < 1.6 < 1.4 2.1 ± 0.8 6 ± 2
UDS034333 −5.152631 34.404969 3.927 × < 0.8 < 2.1 < 2.0 2.5 ± 0.6 14 ± 4
UDS145830 −5.336489 34.556466 3.2094 ✓ 8.3 ± 1.0 3.5 ± 1.2 < 3.4 5.5 ± 1.3 18 ± 6
UDS283510 −5.368315 34.388651 4.5092 × < 2.7 − < 3.7 5.3 ± 1.1 18 ± 5
UDS313619 −5.287081 34.242560 3.188 × < 2.4 10.7 ± 1.8 4.6 ± 1.7 6.6 ± 1.9 7 ± 2
UDS379641 −5.110200 34.334556 4.1161 × < 1.8 < 4.7 < 3.5 2.9 ± 1.0 9 ± 3
UDS395442 −5.070635 34.434154 3.589 × < 1.3 < 2.5 < 1.1 2.6 ± 0.9 2.3 ± 0.8
UDS020932⋆ −5.160535 34.518914 3.6005 × < 2.4 < 10 < 3.1 3.2 ± 0.9 3.5 ± 1.0
UDS140603⋆ −5.361135 34.393002 3.4146 ? < 3.0 < 4.2 < 3.0 5.0 ± 1.0 5.6 ± 1.2
UDS152744⋆ −5.303281 34.393005 2.7243 ? < 3.2 < 1.9 < 2.4 5.2 ± 1.1 2.4 ± 0.5
UDS312746⋆ −5.289354 34.243205 3.5207 × < 2.1 < 6.8 < 5.4 2.2 ± 0.7 3.2 ± 1.1
UDS315235⋆ −5.282526 34.473701 3.5976 × < 2.4 < 4.1 < 4.4 1.8 ± 0.6 2.6 ± 0.9
UDS388069⋆ −5.089615 34.339181 3.4550 ? < 1.7 < 2.0 < 1.1 2.3 ± 0.4 3.7 ± 0.7

Notes. AGN indicates the nature of the sources: ✓ for X-ray/BLAGN, ? for a possible AGN and × for a purely SF galaxy. The measured He II, C III], O III] and C IV rest-frame line fluxes are in units of ×10−18erg s−1 cm−2, and the EW0 of the C IV line is un units of Å. The sources with the asterisk are the ones reanalyzed with slinefit and not contained in Talia & Schreiber (2023). The sources in red are the best candidates to be strong LyC leakers (as discussed in Sect. 6).

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