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Table 3

List of sources showing emission lines in each mask.

Name α δ R AB H AB K AB Literature z

ECDF-S 1

AGN5b 3:32:31.46 −27:46:23.20 23.32 21.18 20.90 z = 2.221
BzK25d 3:32:50.83 −27:48:04.68 23.49 23.05
BX1a 3:32:27.10 −27:46:43.25 24.65 z = 2.223
BX10a 3:32:33.78 −27:48:14.40 24.76 z = 2.618
LAE27e 3:32:52.68 −27:48:09.41 25.51 18.00 18.21 z = 3.085

ECDF-S 2

BX16a 3:32:43.63 −27:43:47.71 24.03 z = 2.317
z3LAE2e 3:32:26.94 −27:41:28.26 24.13 z = 3.114
DB8c 3:32:36.14 −27:42:23.07 24.79
DB12c 3:32:31.52 −27:43:51.38 24.51
DB22c 3:32:41.32 −27:45:49.13 26.43 24.88 25.58

SDSS−1030

AGN26 10:30:30.10 5:21:06.19 21.49 20.72 20.35
BX4 10:30:10.25 5:22:15.77 25.23 22.79
BX7 10:30:13.39 5:22:37.85 23.87 22.44 22.48
BX14 10:30:18.86 5:21:40.87 24.18 22.95 22.33
z2LAE2 10:30:07.60 5:21:39.70 25.02 22.67

EHDF-S

z2LAE3 22:33:43.67 −60:39:44.56 24.25
LBG11 22:33:22.54 −60:38:49.63 24.55 z = 3.205

Notes. Column 1: name of the source. Column 2 and 3: right ascension and declination. Columns 4−6: source R, H, and K magnitudes. Column 7: redshift if a zspec was known for that source. The sources in SDSS-1030 and E-HDFS masks all belong to the MUSYC survey. The RAB, HAB, KAB magnitudes were obtained from the references above. The literature reshifts came either from the references above or from the public GOODS spectroscopic catalog (see text). Table 4 lists our results.

(a)

Lyman Break and BX galaxies are selected following selection criteria described in Ga2006 and Gu2010.

(b)

radio catalog object, observed through a 0.5′′ wide slit.

(c)

DB source from Hayes et al. (2010).

(e)

z ≃ 3.1 LAEs from Gr2007.

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