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Table A.11:

Dereddened line intensity ratios with respect to I(H$\beta $) = 100 for regions analyzed in SBS 0948+532, SBS 1054+365, and SBS 1211+540.
Line $f(\lambda)$ SBS 0948+532 SBS 1054+365 SBS 1054+365 b SBS 1211+540
3697.15 H I 0.262 0.48: ... ... ...
3703.86 H I 0.260 1.96 $\pm$ 0.38 ... ... ...
3711.97 H I 0.259 1.25 $\pm$ 0.32 ... ... ...
3721.83 [S III] 0.257 1.57 $\pm$ 0.35 ... ... ...
3726.03 [O II] 0.257 45.4 $\pm$ 2.7 ... ... 33.0 $\pm$ 3.8
3728.00 [O II] 0.256 ... 100.2 $\pm$ 7.5 350 $\pm$ 95 ...
3728.82 [O II] 0.256 65.7 $\pm$ 3.8 ... ... 44.8 $\pm$ 4.6
3734.17 H I 0.255 2.52 $\pm$ 0.43 ... ... 2.61:
3750.15 H I 0.253 2.56 $\pm$ 0.43 ... ... 3.7 $\pm$ 1.3
3770.63 H I 0.249 2.88 $\pm$ 0.45 1.53: ... 3.2 $\pm$ 1.2
3797.90 H I 0.244 5.11 $\pm$ 0.71 2.85: ... 3.99:
3819.61 He I 0.240 0.65 $\pm$ 0.25 ... ... ...
3835.39 H I 0.237 7.74 $\pm$ 0.77 6.8 $\pm$ 1.3 ... 5.9 $\pm$ 1.5
3868.75 [Ne III] 0.230 41.6 $\pm$ 2.6 49.6 $\pm$ 4.8 ... 37.6 $\pm$ 4.0
3889.05 H I 0.226 19.7 $\pm$ 1.5 19.8 $\pm$ 2.8 ... 19.9 $\pm$ 3.0
3967.46 [Ne III] 0.210 15.0 $\pm$ 1.2 27.4 $\pm$ 2.8 ... 13.3 $\pm$ 2.1
3970.07 H I 0.210 16.2 $\pm$ 1.2 ... ... 16.1 $\pm$ 2.2
4026.21 He I 0.198 1.45 $\pm$ 0.32 ... ... ...
4068.60 [S II] 0.189 1.53 $\pm$ 0.33 2.05: ... ...
4101.74 H I 0.182 26.2 $\pm$ 1.7 26.4 $\pm$ 3.0 ... 26.2 $\pm$ 3.0
4340.47 H I 0.127 47.2 $\pm$ 2.9 47.2 $\pm$ 4.1 28.51: 47.3 $\pm$ 4.1
4363.21 [O III] 0.121 8.13 $\pm$ 0.82 9.7 $\pm$ 1.5 ... 12.2 $\pm$ 1.8
4471.48 He I 0.095 3.81 $\pm$ 0.49 3.31 $\pm$ 0.81 ... 4.6 $\pm$ 1.3
4658.10 [Fe III] 0.050 1.13: ... ... ...
4686.00 He II 0.043 1.3 $\pm$ 0.3 0.61 $\pm$ 0.23 ... ...
4711.37 [Ar IV] 0.037 0.85 $\pm$ 0.25 1.18: ... ...
4713.14 He I 0.037 ... ... ... 0.75:
4733.93 [Fe III] 0.031 0.18: ... ... ...
4740.16 [Ar IV] 0.030 0.61 $\pm$ 0.24 ... ... 0.98:
4754.83 [Fe III] 0.026 0.34: ... ... ...
4861.33 H I 0.000 100.0 $\pm$ 5.2 100.0 $\pm$ 7.4 100 $\pm$ 39 100.0 $\pm$ 7.5
4958.91 [O III] -0.024 189.5 $\pm$ 9.2 210 $\pm$ 13 75 $\pm$ 23 163 $\pm$ 10
4985.90 [Fe III] -0.031 1.49 $\pm$ 0.30 ... ... ...
5006.84 [O III] -0.036 584 $\pm$ 28 623 $\pm$ 37 183 $\pm$ 53 481 $\pm$ 29
5015.68 He I -0.038 ... ... ... 2.24:
5197.90 [N I] -0.082 ... 1.03: ... ...
5517.71 [Cl III] -0.154 0.39: ... ... ...
5537.88 [Cl III] -0.158 0.24: ... ... ...
5875.64 He I -0.215 10.76 $\pm$ 0.81 8.7 $\pm$ 1.6 ... ...
6300.30 [O I] -0.282 3.00 $\pm$ 0.31 1.12: ... 2.36:
6312.10 [S III] -0.283 1.74 $\pm$ 0.24 1.36: ... 2.8 $\pm$ 1.1
6363.78 [O I] -0.291 1.07 $\pm$ 0.23 0.65: ... 0.57:
6548.03 [N II] -0.318 2.45 $\pm$ 0.30 2.02 $\pm$ 0.74 7.66: 0.82:
6562.82 H I -0.320 278 $\pm$ 14 277 $\pm$ 17 279 $\pm$ 74 280 $\pm$ 17
6583.41 [N II] -0.323 6.21 $\pm$ 0.60 5.6 $\pm$ 1.0 20.2: 2.24 $\pm$ 0.89
6678.15 He I -0.336 2.81 $\pm$ 0.36 2.94 $\pm$ 0.96 7.40: 3.6 $\pm$ 1.1
6716.47 [S II] -0.342 ... 10.1 $\pm$ 1.2 22.4: 5.65 $\pm$ 0.88
6730.85 [S II] -0.344 ... 7.03 $\pm$ 0.97 19.6: 4.91 $\pm$ 0.82
7065.28 He I -0.387 ... 2.08 $\pm$ 0.83 ... ...
7135.78 [Ar III] -0.396 ... 8.8 $\pm$ 1.5 ... ...
Aperture size (arcsec)   3.6 6.4 5.8 3.6
Distancea (arcsec)   0 0 17.8 0
F(H$\beta $)b   8.44 $\pm$ 0.32 14.57 $\pm$ 0.68 0.66 $\pm$ 0.13 1.84 $\pm$ 0.09
C(H$\beta $)   0.35 $\pm$ 0.03 0.02 $\pm$ 0.02 0.6 $\pm$ 0.1 0.12 $\pm$ 0.01
$W_{\rm abs}$ (Å)   0.3 $\pm$ 0.1 0.8 $\pm$ 0.1 0.3 $\pm$ 0.1 1.3 $\pm$ 0.1
-W(H$\alpha $) (Å)   788 $\pm$ 43 422 $\pm$ 27 32 $\pm$ 8 705 $\pm$ 45
-W(H$\beta $) (Å)   213 $\pm$ 11 89 $\pm$ 7 8 $\pm$ 3 135 $\pm$ 10
-W(H$\gamma$) (Å)   57 $\pm$ 4 43 $\pm$ 4 2 $\pm$ 1 74 $\pm$ 7
-W([O III]) 5007 (Å)   689 $\pm$ 34 567 $\pm$ 35 12 $\pm$ 3 618 $\pm$ 38

a Relative distance of the knot with respect to the main region in the galaxy; b in units of 10-15 erg s-1 cm-2 and not corrected for extinction.


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