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Table 4

Modelling the line ratios (Hβ =1) observed by Xia et al. (2012).

ID z [OIII]5007+ [OII]3727+ V s n 0 T U O/H D Hβ abs Hβ obs
km   s-1 cm-3 104 K 10-4 1017 cm 10-3erg   cm-2   s-1 10-18erg   cm-2   s-1

339 0.602 5.07 1.38 468.41 ± 45.19
calc 5.4 1.3 200 80 2.4 5.2 1.8 1. 5.1
364 0.642 6.13 1.61 50.35 ± 7.24
calc 6.0 1.61 150 80 2.5 2. 2. 1. 2.9
246 0.696 5.32 0.196 22.90 ± 5.22
calc 5.0 0.2 250 80 3. 0.8 6.6 0.15 1.13
454 0.847 1.91 3.68 45.22 ± 13.92
calc 2.1 3.2 250 180 1.4 0.003 6.6 0.05 2.6
258 0.998 3.28 0.41 73.63 ± 35.74*
calc 3.66 0.44 280 100 3. 0.9 5.6 0.12 1.5
432 1.573 5.46 4.2 24.21 ± 11.76*
calc 5.5 4.4 200 70 2.1 7. 6.2 1.4 5.3
563 1.673 8.75 6.73 13.95 ± 9.06*
calc 8.63 6.1 200 70 2.1 7. 6.2 1.3 3.8
103 1.682 5.37 4.43 9.84 ± 7.81*
calc 5.5 4.4 200 70 2.1 7. 6.2 1.4 5.3
195 1.745 5.17 4.13 21.25 ± 8.28*
calc 5.23 4.2 200 70 2.1 7. 5. 1.44 5.23
242 2.070 5.93 7.08 13.39 ± 8.57*
calc 5.22 7.6 250 165 1.4 0.003 4.6 0.05 0.76
578 2.315 5.37 9.48 12.29 ± 10.42*
calc 5.9 9.2 250 165 1.4 0.001 4.6 0.05 0.67

Notes.

(*)

The 3σ upper limit of the Hβ line is used for galaxies with S/N< 3.

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