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Table A.4.

Spectroscopic identification of our targets.

ID zphot zspec p a Balmer Emission σν d
abs.b linesc km s−1
Robust zspec
ZF-COS-20032 1.6 96% 1.0 [O I]6300 Hα [N II]λλ 217 ± 161
ZF-COS-20115 −0.9 100% 1.0 Yes
ZF-COS-20133 0.6 100% 1.0 Hβ [O III]λλ 60 ± 26
3D-EGS-18996 −8.3 100% 1.0 Yes [O III]λλ 530 ± 199
3D-EGS-26047 0.0 99% 1.0 [O II]λλ Hβ [O III]λλ 530 ± 263
3D-EGS-40032 −0.0 100% 1.0 Yes [O II]λλ 582 ± 236
ZF-UDS-8197 −1.2 99% 1.0 [O III]λλ 530 ± 53
3D-UDS-27939 4.5 100% 1.0 [O I]6300 Hα [N II]λλ [S II]λλ 154 ± 7

Uncertain zspec
ZF-COS-17779 1.4 77% 1.0 Hβ [O III]λλ 60 ± 26
ZF-COS-18842 −4.5 75% 1.1 [O III]λλ 60 ± 279
ZF-COS-19589 0.1 32% 0.9
3D-EGS-31322 0.5 84% 1.0 Yes

Rejected zspec
ZF-COS-10559 0.4 2% 0.9
ZF-COS-14907 −23.1 63% 1.2
3D-EGS-27584 4.3 9% 1.0
3D-EGS-34322 0.1 18% 0.9
ZF-UDS-3651 2.7 33% 1.1
ZF-UDS-4347 0.5 39% 0.9
ZF-UDS-6496 1.3 33% 1.0
ZF-UDS-7329 −0.1 25% 1.0
ZF-UDS-7542 −0.6 35% 1.0
3D-UDS-35168 −0.5 4% 1.0
3D-UDS-39102 0.2 4% 1.0
3D-UDS-41232 0.2 25% 1.0

Notes. This table is also available in electronic format at the CDS.

(a)

Fraction of the redshift probability distribution enclosed within zspec ± 0.01.

(b)

Indicates galaxies for which the redshift could be determined with p > 50% from the continuum emission alone, using Balmer absorption lines.

(c)

List of emission lines detected with a significance of at least 2σ. Line doublets names are shortened as in Table A.5.

(d)

Best-fit velocity dispersion of the emission lines (assumed identical for all the lines in a spectrum).

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