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Table 1.

Summary of the redshift measurements obtained in the LBT-MODS campaign presented in this work.

ObjID RA Dec rAB zspec Qz Class zphot, M21 zphot, new Spectral features (obs λ)
hh:mm:ss dd:mm:ss
XID 007 10:30:29.77 +05:22:32.26 25.21 2.7799 2 ELG 3.24 3.22 Lyα (4595 Å)
XID 008 10:30:28.10 +05:22:58.75 24.41 2.7797 2 ELG 3.34 2.68 Lyα (4597 Å), NV
XID 011 10:30:27.89 +05:23:13.42 26.67 2.7674 2 ELG 4.34 4.16 Lyα (4581 Å)
XID 151 10:30:41.54 +05:26:25.13 25.25 3.041 2 ELG 2.74 2.96 Lyα (4912 Å)
XID 158 10:30:28.01 +05:28:08.35 24.83 2.505 1 ELG 3.37 2.12 Lyα (4262 Å), NV
XID 378 10:30:38.13 +05:24:03.31 26.5 0 None 5.45 1.92 None
XID 381 10:30:43.12 +05:25:26.99 25.06 0 None 3.44 3.86 None

XID 029 10:30:38.00 +05:26:13.09 26.66 0 None 2.22 2.15 None
XID 066 10:30:32.31 +05:28:07.35 23.99 2.1113 2 ELG 2.15 1.84 Lyα (3783 Å), NV
XID 098 10:30:31.05 +05:27:47.32 27.3 0 None 1.49 5.21 None
XID 102 10:30:31.61 +05:29:04.44 25.6 1.1084 2 ELG 5.44 1.72 MgII, [OII], [NeV]
XID 103 10:30:29.79 +05:29:09.09 24.65 1.4990 1 ELG 1.44 1.50 [OII]
XID 153 10:30:28.29 +05:27:40.72 27.02 0 None 2.16 4.44 None
XID 198 10:30:39.95 +05:26:55.23 24.1 0 None 1.35 1.02 None
XID 206 10:30:14.76 +05:29:19.80 > 27.5 1.124 1 ELG 1.48 1.48 [OII], [NeV]
XID 214 10:30:44.59 +05:25:44.77 25.97 0 None 1.38 1.44 None
XID 365 10:30:27.88 +05:23:48.31 25.72 1.4159 1 ELG 1.83 1.73 [OII], [OIII]
XID 366 10:30:28.58 +05:32:24.61 24.52 1.0474 2 ELG 0.92 0.84 [OII], [NeIII]
XID 369 10:30:31.28 +05:28:02.30 24.7 0.8248 2 ELG 1.17 1.17 [OII], [OIII], Hγ, Hβ

Notes. The identification number is taken from the Chandra J1030 catalog (Nanni et al. 2020). Furthermore, rAB is the AUTO magnitude in the r band, as reported in Nanni et al. (2020); zspec is the source spectroscopic redshift; Qz is the quality flag for zspec (2: secure; 1: uncertain; 0: no measurement); “Class” is the spectral classification (ELG: emission line galaxy; None; no classification); and zphot, M21 is the photometric redshift computed in Marchesi et al. (2021) and used to select the high-redshift candidates, while zphot, new is the updated photometric redshift computed using the new g- and Ks-band photometric information presented in Sect. 2, as described in Appendix A.

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