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Table A.5:

Dereddened line intensity ratios with respect to I(H$\beta $)=100 for knots analyzed in Mkn 5. Region A was observed using three slit positions with a PA of 0$^{\circ }$ (INT-1), 349$^{\circ }$ = -11$^{\circ }$ (INT-2), and 354$^{\circ }$ = -6$^{\circ }$ (WHT).
Line $f(\lambda)$ A-INT-1 A-INT-2 A-WHT B
3666.10 H I 0.267 1.99 $\pm$ 0.71 ... ... ...
3697.15 H I 0.262 1.16: ... ... ...
3705.04 He I 0.260 1.65: ... ... ...
3711.97 H I 0.259 ... $2.03 \pm 0.76$ ... ...
3728.00 [O II] 0.256 $191 \pm 12$ $213 \pm 12$ ... 252:
3750.15 H I 0.253 $1.79 \pm 0.68$ ... ... ...
3770.63 H I 0.249 ... $2.47 \pm 0.79$ ... ...
3797.90 H I 0.244 ... 1.54: ... ...
3819.61 He I 0.240 ... 0.65: ... ...
3835.39 H I 0.237 7.4 $\pm$ 1.7 5.6 $\pm$ 1.3 ... ...
3868.75 [Ne III] 0.230 23.1 $\pm$ 3.3 31.0 $\pm$ 2.4 ... ...
3889.05 H I 0.226 13.6 $\pm$ 2.9 17.7 $\pm$ 2.1 ... ...
3967.46 [Ne III] 0.210 18.7 $\pm$ 1.9 21.3 $\pm$ 1.8 ... ...
4026.21 He I 0.198 ... 1.55: ... ...
4068.60 [S II] 0.189 2.24 $\pm$ 0.70 2.29 $\pm$ 0.76 ... ...
4101.74 H I 0.182 26.0 $\pm$ 2.8 26.8 $\pm$ 2.1 ... ...
4168.97 He I 0.167 ... 1.06: ... ...
4340.47 H I 0.127 47.0 $\pm$ 3.2 47.0 $\pm$ 3.1 47.0 $\pm$ 2.8 ...
4363.21 [O III] 0.121 5.14 $\pm$ 0.91 5.29 $\pm$ 0.93 4.93 $\pm$ 0.74 ...
4387.93 He I 0.115 ... 0.56: 1.32 $\pm$ 0.40 ...
4416.27 [Fe II] 0.109 ... ... 0.38: ...
4471.48 He I 0.095 4.43 $\pm$ 0.85 3.96 $\pm$ 0.84 4.16 $\pm$ 0.60 ...
4658.10 [Fe III] 0.050 ... 1.10: 0.72: ...
4686.00 He II 0.043 0.92 $\pm$ 0.19 1.01: 0.82: ...
4711.37 [Ar IV] 0.037 ... 0.59: ... ...
4713.14 He I 0.037 ... ... 0.28: ...
4740.16 [Ar IV] 0.030 ... ... 0.31: ...
4861.33 H I 0.000 100.0 $\pm$ 6.3 100.0 $\pm$ 5.7 100.0 $\pm$ 5.2 100:
4921.93 He I -0.015 ... 1.70: 0.95 $\pm$ 0.36 ...
4958.91 [O III] -0.024 144.1 $\pm$ 8.5 144.7 $\pm$ 7.8 133.8 $\pm$ 7.2 70.43:
4985.90 [Fe III] -0.031 2.33 $\pm$ 0.65 2.02: 2.20: ...
5006.84 [O III] -0.036 423 $\pm$ 22 430 $\pm$ 21 374 $\pm$ 19 214 $\pm$ 69
5015.68 He I -0.038 ... ... 2.13 $\pm$ 0.62 ...
5197.90 [N I] -0.082 ... 0.46: ... ...
5875.64 He I -0.215 8.46 $\pm$ 0.83 8.41 $\pm$ 0.88 11.0 $\pm$ 1.0 ...
6300.30 [O I] -0.282 5.12 $\pm$ 0.68 4.57 $\pm$ 0.66 4.05 $\pm$ 0.58 ...
6312.10 [S III] -0.283 2.31 $\pm$ 0.55 1.92 $\pm$ 0.43 1.79 $\pm$ 0.47 ...
6363.78 [O I] -0.291 1.90 $\pm$ 0.51 1.52: 1.19 $\pm$ 0.38 ...
6548.03 [N II] -0.318 4.56 $\pm$ 0.56 5.25 $\pm$ 0.69 5.49 $\pm$ 0.63 ...
6562.82 H I -0.320 283 $\pm$ 16 284 $\pm$ 15 284 $\pm$ 14 284 $\pm$ 85
6583.41 [N II] -0.323 14.7 $\pm$ 1.2 14.0 $\pm$ 1.1 14.9 $\pm$ 1.1 10.13:
6678.15 He I -0.336 3.43 $\pm$ 0.63 3.49 $\pm$ 0.66 3.05 $\pm$ 0.51 ...
6716.47 [S II] -0.342 21.5 $\pm$ 1.5 22.2 $\pm$ 1.7 24.3 $\pm$ 1.5 67.4:
6730.85 [S II] -0.344 15.6 $\pm$ 1.2 16.0 $\pm$ 1.4 18.1 $\pm$ 1.2 51.6:
7065.28 He I -0.387 2.13 $\pm$ 0.50 2.40 $\pm$ 0.64 2.17 $\pm$ 0.45 ...
7135.78 [Ar III] -0.396 8.49 $\pm$ 0.61 8.56 $\pm$ 0.97 7.70 $\pm$ 0.52 ...
7281.35 He I -0.414 ... ... 0.41: ...
7318.39 [O II] -0.418 ... 2.87: 3.62 $\pm$ 0.54 ...
7329.66 [O II] -0.420 ... 2.57: 2.74 $\pm$ 0.44 ...
7751.10 [Ar III] -0.467 ... ... 1.64 $\pm$ 0.38 ...
Aperture size (arcsec)   $14.4 \times 1$ $16 \times 1$ $3.6 \times 1$ $6 \times 1$
Distanceb (arcsec)   0 0 0 16
F(H$\beta $)a   17.66 $\pm$ 0.73 18.13 $\pm$ 0.69 10.83 $\pm$ 0.40 0.35 $\pm$ 0.08
C(H$\beta $)   0.36 $\pm$ 0.02 0.17 $\pm$ 0.02 0.03 $\pm$ 0.02 0.30 $\pm$ 0.06
$W_{\rm abs}$ (Å)   1.1 $\pm$ 0.2 0.8 $\pm$ 0.2 0 1.5 $\pm$ 0.5
-W(H$\alpha $) (Å)   449 $\pm$ 26 435 $\pm$ 23 678 $\pm$ 35 43 $\pm$ 12
-W(H$\beta $) (Å)   75 $\pm$ 5 80 $\pm$ 5 135 $\pm$ 7 10:
-W(H$\gamma$) (Å)   43 $\pm$ 3 34 $\pm$ 2 44 $\pm$ 3 ...
-W([O III]) 5007 (Å)   320 $\pm$ 17 360 $\pm$ 18 530 $\pm$ 28 33 $\pm$ 11

a In units of 10-15 erg s-1 cm-2 and not corrected for extinction; b relative distance with respect to the center of Mkn 5.


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