Table 3: Line fluxes and metallicities inferred from the near-IR spectra.
Name F([OIII]5007) F(H$\beta$) F([OII]3727) F([NeIII]3870) 12 + log(O/H)
  $\rm 10^{-17}~erg~s^{-1}~cm^{-2}$a  
CDFa-C9 6.83 $\pm$ 0.21 1.44 $\pm$ 0.18 2.16 $\pm$ 0.14 0.53 $\pm$ 0.13 $8.10\rm ^{+0.18}_{-0.21}$
CDFS-4414 0.95 $\pm$ 0.11 0.40 $\pm$ 0.10 0.87 $\pm$ 0.08 <0.20 $8.54\rm ^{+0.15}_{-0.14}$
CDFS-4417 2.00 $\pm$ 0.11 0.89 $\pm$ 0.09 1.17 $\pm$ 0.11 0.20 $\pm$ 0.09 $8.55\rm ^{+0.09}_{-0.10}$
CDFS-6664 2.71 $\pm$ 0.20 0.50 $\pm$ 0.16 0.40 $\pm$ 0.07 - $7.73\rm ^{+0.38}_{-0.29}$
CDFS-16767 1.90 $\pm$ 0.14 0.50 $\pm$ 0.10 0.50 $\pm$ 0.06 - $8.31\rm ^{+0.11}_{-0.17}$
CDFS-11991 2.94 $\pm$ 0.11 0.26 $\pm$ 0.10 0.62 $\pm$ 0.08 0.15 $\pm$ 0.08 $8.02\rm ^{+0.17}_{-0.23}$
CDFS-2528 1.87 $\pm$ 0.26 0.32 $\pm$ 0.18 0.67 $\pm$ 0.16 - $8.07\rm ^{+0.39}_{-0.28}$
SSA22a-M38 5.41 $\pm$ 0.31 1.48 $\pm$ 0.20 3.51 $\pm$ 0.37 <0.70 $8.34\rm ^{+0.15}_{-0.12}$
SSA22a-aug16M16 1.65 $\pm$ 0.10 0.30 $\pm$ 0.07 0.45 $\pm$ 0.11 <0.25 $7.99\rm ^{+0.26}_{-0.34}$
Compositea 4.58 $\pm$ 0.12 1.00 $\pm$ 0.10 1.50 $\pm$ 0.14 0.25 $\pm$ 0.12 $8.24\rm ^{+0.15}_{-0.20}$
The following quantities are reported in each column: Col. 1, object name; Cols. 2-5, emission line fluxes; Col. 6, gas metallicity.
Notes: a In the case of the composite spectrum fluxes are normalized to the H$\beta$ flux (which is also subject to an error as listed in the corresponding column).


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