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Table 2

Line fluxes inferred from the near-IR spectra.

Name F([OIII]5007) F(Hβ) F([OII]3727) F([NeIII]3870)
10-17 erg s-1 cm-2

CDFaC9 7.23 1.49 2.36 0.60
CDFS4414 1.06 0.42 0.89 0.12
CDFS4417 1.77 0.88 1.39 0.31
CDFS6664 3.38 0.34 0.29
CDFS16767 1.99 0.46 0.60
CDFS11991 3.02 0.28 0.52 0.22
CDFS2528 1.61 0.35 0.61
CDFS16272 3.62 0.48 0.66 0.23
CDFS9313 4.45 0.54 0.72
CDFS9340 1.64 0.37 0.40
CDFS12631 2.98 0.49 2.09 1.13
CDFS14411 3.88 0.75 1.02 0.20
CDFS5161 1.23 0.17 0.17 0.11
LnA1689-2 a 0.16 0.05
LnA1689-4 a 0.45 0.05 0.06 0.02
LnA1689-1 a 0.15 0.04 0.06
Q1422D88 4.31 0.55 0.55
3C 324C3 1.15 0.26 0.46 0.31
Cosmic Eyea 0.78 0.09 0.24
SSA22aM38 5.56 1.40 3.12 1.03
SSA22aD17 1.73 0.36 1.04
SSA22aaug96M16 1.82 0.38 0.47
SSA22aC16 5.45 1.47 2.59
SSA22aC36 1.81 0.48 2.12 0.34
DSF2237bC21 0.70 1.00 1.85 0.35
DSF2237bD29 0.93 0.14 0.76
Q0302C131 2.62 0.46 0.80
Q0302C171 1.10 0.18 0.56
Q0302M80 1.32 0.40 0.56
SSA22aC30 1.28 0.26 0.30
SSA22aC6 5.50 0.76 1.21
SSA22aM4 3.66 0.69 1.46
SSA22bC5 3.28 0.50 0.27 0.38
DSF2237bD28 1.86 0.16 0.74
Compositeb 6.13 ± 0.14 1.00 ± 0.10 1.70 ± 0.12 0.39 ± 0.08

Notes.Column 1, object name; Cols. 2–5, emission line fluxes.

(a)

Values corrected for a magnification factor of 5.9 ± 1.9, 43.5 ± 4.1, 6.7 ± 2.1 (see text), and 28 ± 3 (Smail et al. 2007), respectively.

(b)

In the case of the composite spectrum fluxes were normalized to the Hβ flux (which is also subject to an error, as listed in the corresponding column).

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