Table 5: Observed flux for type 2 and Starburst galaxies, in units of $\rm 10^{-15}~ erg ~ cm^{-2} ~ s^{-1}$.

Ion		 $\rm\lambda_{lab}~(\AA)$ NGC 34 NGC 262 Mrk 993 NGC 591 Mrk 573 NGC 1144 Mrk 1066 NGC 1275 NGC 1614

$\lbrack$S III]		 9069 $16.57\pm2.90$ $47.76\pm0.68$ $7.11\pm0.98 $ $34.95\pm1.05$ $38.92\pm1.09$ $3.77\pm0.23$ $65.66\pm0.52$ $72.93\pm2.39$ $100.39\pm1.57$
$\lbrack$S III] 9531 $18.47\pm1.01$ $128.13\pm1.20$ $16.51\pm0.07 $ $92.63\pm0.95$ $108.65\pm0.69$ $7.11\pm0.16$ $178.79\pm1.02$ $188.73\pm1.55$ $278.66\pm1.22$
$\lbrack$C I] 9824 $2.55\pm0.94$ $1.70\pm0.52$ $0.36\pm0.11 $ $3.38\pm0.70$ $0.59\pm0.05 $ - $5.72\pm0.27 $ $5.38\pm0.57$ -
$\lbrack$C I] 9850 $7.40\pm0.94$ $4.13\pm0.52$ $2.10\pm0.20 $ $7.23\pm0.70$ $2.57\pm1.23$ - $12.54\pm0.27 $ $17.26\pm0.59$ -
$\lbrack$S VIII] 9910 - $2.65\pm0.59$ $0.76\pm0.17$ $2.52\pm0.23 $ $6.10\pm0.10$ - - - -
H I 10049 - $2.26\pm0.52$ - $2.54\pm0.58 $ $3.27\pm0.16$ - $9.74\pm0.30$ $13.32\pm1.08 $ $17.28\pm0.67$
He II 10122 - $3.78\pm0.54$ - $4.28\pm0.83 $ - - $5.36\pm0.55$ $4.00\pm0.78 $ -
$\lbrack$S II] 10286 - $5.85\pm0.55$ - $1.98\pm0.57 $ $3.58\pm0.22$ - $5.52\pm0.38$ $33.05\pm1.30 $ -
$\lbrack$S II] 10320 - $8.18\pm0.55$ - $4.52\pm0.57 $ $2.78\pm0.22$ - $7.88\pm0.38$ $42.16\pm1.30 $ -
$\lbrack$S II] 10336 - $4.02\pm0.55$ - $1.91\pm0.57 $ $1.67\pm0.22$ - $3.76\pm0.38$ $34.65\pm1.30 $ -
$\lbrack$S II] 10370 - $2.06\pm0.55$ - $1.86\pm0.57 $ $1.22\pm0.22$ - $2.16\pm0.38$ $17.64\pm1.30 $ -
$\lbrack$N I] 10404 - $1.94\pm0.38$ - $1.99\pm0.73 $ $1.80\pm0.44$ - $1.54\pm0.36$ $42.82\pm1.38 $ -
He I 10830 $20.71\pm1.30$ $66.98\pm0.61$ $32.41\pm1.89$ $53.20\pm0.75$ $50.95\pm0.40$ - $102.69\pm1.39$ $588.47\pm5.14$ $238.51\pm4.60$
H I 10938 - $5.82\pm0.62$ $15.39\pm2.46$ $5.70\pm0.56$ $6.11\pm0.41$ - $25.53\pm1.20$ $83.53\pm4.25$ $53.67\pm4.79$
$\lbrack$P II] 11470 - $1.71\pm0.36$ - - $2.17\pm0.19$ - $4.51\pm0.20$ $5.21\pm0.41 $ -
He II 11626 - $0.76\pm0.19$ - - $1.77\pm0.12$d - $1.51\pm0.30$ $3.24\pm0.39 $ -
$\lbrack$P II] 11886 $8.85\pm2.33$ $3.68\pm0.39$ - $5.35\pm0.77 $ $2.18\pm0.69$d - $16.31\pm1.45$ $18.95\pm0.50 $ -
$\lbrack$S IX] 12520 - $2.28\pm0.58$ - - $4.85\pm0.13$ - $4.81\pm0.32$ - -
$\lbrack$Fe II] 12570 $13.76\pm1.24$e $11.59\pm0.52$e $5.05\pm0.30$e $17.19\pm0.75$e $5.90\pm0.14$e $0.91\pm0.23$e $38.53\pm0.25$e $63.49\pm1.51$e $35.02\pm1.22$e
H I 12820 $12.83\pm1.13$e $10.75\pm0.33$e $14.90\pm2.66$e $15.14\pm0.49$e $9.58\pm0.17$e - $54.07\pm0.24$e $60.66\pm3.15$e $129.28\pm1.14$e
$\lbrack$Fe II] 12950 - $1.61\pm0.33$ - $2.15\pm0.40 $ - - $5.59\pm0.71$ $12.13\pm2.62 $ -
$\lbrack$Fe II] 13209 - $3.34\pm0.81$ - $6.41\pm1.09 $ - - $13.70\pm0.54$ $18.48\pm1.64 $ -
$\lbrack$Si X] 14300 - $2.03\pm0.50$ - $3.16\pm0.42 $ $7.54\pm0.25$ - $4.25\pm1.07$ - -
$\lbrack$Fe II] 15342 - $2.32\pm0.22$ - - - - $6.61\pm0.64$ $8.82\pm0.94 $ -
$\lbrack$Fe II] 16436 $11.00\pm2.87$e $9.09\pm0.31$e - $14.19\pm0.73$e $4.11\pm0.09$e - $37.07\pm0.34$e $61.49\pm0.65$e $20.84\pm2.91$e
$\lbrack$Fe II] 16773 - - - - - - $3.97\pm0.50$ $8.97\pm0.53 $ -
H I 16806 - - - - - - $3.98\pm0.55$ - -
H I 18750 $62.75\pm0.43$ $35.26\pm1.05$ - $60.10\pm0.77$ $45.57\pm0.28$ - $145.74\pm1.60$ $145.14\pm2.52$ $295.45\pm6.86$
H I 19446 - - - $0.93\pm0.08 $ $1.37\pm0.06$ - $8.67\pm0.04$ $13.98\pm2.06 $ $20.50\pm3.48$
$\rm H_2$ 19570 $12.43\pm1.02$e $2.09\pm0.18$e $1.63\pm0.10$e $6.82\pm0.63$e $1.44\pm0.17$e - $15.17\pm0.38$e $43.15\pm0.67$e $11.18\pm3.97$e
$\lbrack$Si VI] 19641 - $4.43\pm0.19$ - $8.07\pm0.76 $ $10.17\pm0.18$ - $3.53\pm0.34$ - -
$\rm H_2$ 20332 $4.66\pm0.23$e $0.60\pm0.09$e $0.92\pm0.12$e $2.66\pm0.22$e $0.75\pm0.24$e $0.47\pm0.06$e $4.83\pm0.10$e $15.26\pm0.33$e -
He I 20580 - - - $1.42\pm0.19 $ $0.53\pm0.06$ - $6.83\pm0.19$ $9.62\pm1.14 $ $25.99\pm0.56$
$\rm H_2$ 21213 $12.15\pm1.27$e $1.61\pm0.05$e $1.01\pm0.17$e $6.52\pm0.14$e $1.82\pm0.19$e $0.94\pm0.04$e $13.41\pm0.16$e $42.95\pm0.37$e $5.70\pm0.77$e
H I 21654 $7.12\pm0.13$e $1.09\pm0.11$e - $3.55\pm0.22$e $2.77\pm0.09$e - $14.16\pm0.22$e $9.77\pm0.41$e $42.45\pm0.74$e
$\rm H_2$ 22230 - - - $1.77\pm0.16$e - - $2.66\pm0.06$e $11.81\pm0.30$e -
$\rm H_2$ 22470 - - - $0.70\pm0.16$e - - $1.77\pm0.03$e $4.51\pm0.33$e -
$\lbrack$Ca VIII] 23218 - - - - $3.18\pm0.29$ - - - -
Ion $\rm\lambda_{lab}~(\AA)$ NGC 2110 ESO 428-G014 NGC 3310 NGC 5728 NGC 5929 NGC 5953 NGC 7674 NGC 7682 NGC 7714

$\lbrack$S III]		 9069 $50.08\pm1.63 $ $143.16\pm0.89$ $35.21\pm1.82 $ - $14.70\pm1.22$ $18.21\pm2.73$ $56.85\pm1.68$ $32.27\pm1.01$ $82.46\pm2.57$
$\lbrack$S III] 9531 $125.39\pm0.88 $ $371.27\pm2.39$ $92.45\pm1.33 $ $62.15\pm0.70$ $34.32\pm0.95$ $34.85\pm2.32$ $143.23\pm5.73$ $85.25\pm0.35$ $202.45\pm1.54$
$\lbrack$C I] 9824 $8.38\pm0.64 $ $7.50\pm0.32$ - - - - - - $2.72\pm0.54$
$\lbrack$C I] 9850 $20.67\pm0.64 $ $12.76\pm0.32$ - - - - $6.84\pm0.64 $ - $3.18\pm0.35$
$\lbrack$S VIII] 9910 - $6.03\pm0.31$ - - - - $4.03\pm0.98$ $1.69\pm0.71$ -
H I 10049 $3.00\pm0.27 $ $9.19\pm0.63$ $3.44\pm0.51 $ $5.45\pm1.42 $ - - $8.38\pm0.67 $ $1.18\pm0.18$ $11.47\pm0.63$
He II 10122 - $20.18\pm0.80$ $12.59\pm1.34 $ $7.03\pm1.58 $ - $4.9\pm1.05$ $10.21\pm0.67$ $3.62\pm0.31$ -
$\lbrack$S II] 10286 $16.89\pm1.16 $ $9.53\pm0.20$ - - - - $4.58\pm0.60 $ $3.91\pm0.77$ -
$\lbrack$S II] 10320 $19.75\pm1.16 $ $13.45\pm0.20$ - - - - $4.73\pm0.60 $ $5.39\pm0.77$ -
$\lbrack$S II] 10336 $13.50\pm1.16 $ $7.55\pm0.20$ - - - - $3.09\pm0.60 $ $2.31\pm0.77$ -
$\lbrack$S II] 10370 $8.40\pm1.16 $ $2.53\pm0.20$ - - - - $0.49\pm0.60 $ $1.96\pm0.77$ -
$\lbrack$N I] 10404 $25.94\pm1.65 $ $0.91\pm0.12$ - - - - $6.26\pm1.45 $ $2.09\pm1.00$ -
He I 10830 $102.30\pm1.00 $ $178.01\pm0.90$ - $32.69\pm1.38$ $20.70\pm0.69$ $18.73\pm1.63$ $56.48\pm0.57$ $49.09\pm1.50$ $128.83\pm2.39$
H I 10938 $12.66\pm1.03 $ $31.04\pm1.15$ - $3.80\pm1.05$ $3.79\pm0.27$d - $13.87\pm1.31$ $4.98\pm1.12$ $26.70\pm2.12$
$\lbrack$P II] 11470 - $4.55\pm0.71$ - - - - $1.52\pm0.13 $ - -
He II 11626 - $2.92\pm0.51$ - - - - $0.65\pm0.08 $ - -
$\lbrack$P II] 11886 $14.49\pm2.75 $ $15.18\pm0.74$ - - - - $5.69\pm0.30 $ - -
$\lbrack$S IX] 12520 - $5.15\pm0.80$ - $1.19\pm0.59$ - - $4.11\pm1.48 $ - -
$\lbrack$Fe II] 12570 $81.24\pm1.02$e $30.24\pm0.62$e $10.70\pm0.87$c $5.08\pm0.50$c $8.44\pm0.36$e $19.06\pm0.66$e $10.81\pm0.92$e $4.58\pm0.74$e $17.35\pm0.53$e
H I 12820 $14.91\pm0.86$e $45.26\pm0.57$e $31.74\pm1.03$c $7.37\pm1.16$c $7.68\pm0.20$e - $10.36\pm0.58$e $9.92\pm0.65$e $59.73\pm1.38$
$\lbrack$Fe II] 12950 $13.03\pm1.18 $ $5.94\pm0.89$ - - - - - - -
$\lbrack$Fe II] 13209 $30.76\pm0.63 $ $22.26\pm2.06$ - - $3.50\pm0.76$ $13.89\pm2.11$ - - -
$\lbrack$Si X] 14300 - - - - - - $3.53\pm0.25 $ - -
$\lbrack$Fe II] 15342 $14.62\pm1.33 $ $7.82\pm0.82$ - - - - - - -
$\lbrack$Fe II] 16436 $70.17\pm0.55$e $28.47\pm1.05$e $11.12\pm1.57$c $4.96\pm0.61$c $7.83\pm0.37$e $15.21\pm1.89$e $9.74\pm0.47$e - $14.84\pm2.08$e
$\lbrack$Fe II] 16773 $8.80\pm1.18 $ $3.83\pm0.20$ - - - - $24.07\pm5.31$ - -
H I 16806 - $8.22\pm0.29$ - - - - $25.66\pm4.52$ - -
H I 18750 $32.95\pm4.50 $ $102.05\pm0.78$ $112.98\pm1.57 $ $20.63\pm1.92$ - $19.82\pm0.83$ $32.06\pm1.09$ $31.82\pm0.81$ $117.94\pm2.35$
H I 19446 - $3.00\pm0.49$ $4.04\pm0.83 $ - - - $3.38\pm0.51 $ - -
$\rm H_2$ 19570 $11.35\pm0.28$e $8.29\pm0.55$e - $6.04\pm0.56$c $3.07\pm0.60$e $6.67\pm1.85$ed $4.05\pm0.56$e $9.40\pm0.51$e -
$\lbrack$Si VI] 19641 - $21.09\pm0.66$ - $7.08\pm0.88$ - - $10.71\pm1.11$ $2.96\pm0.63$ -
$\rm H_2$ 20332 $4.22\pm0.21$e $3.06\pm0.27$e $1.24\pm0.25$c $2.40\pm0.20$c $1.33\pm0.23$e $2.28\pm0.72$e $1.20\pm0.23$e $3.50\pm0.22$e -
He I 20580 $1.67\pm0.22$ $2.14\pm0.08$ $6.69\pm0.52 $ - - - $1.27\pm0.27 $ - $8.83\pm0.31$
$\rm H_2$ 21213 $8.39\pm0.19$e $8.27\pm0.12$e $1.54\pm0.32$c $6.28\pm0.12$c $2.88\pm0.22$e $3.54\pm0.51$e $2.12\pm0.12$e $9.78\pm0.14$e $3.31\pm0.43$e
H I 21654 $2.50\pm0.22$e $8.98\pm0.14$e $10.79\pm0.33$c $2.11\pm0.19$c $1.35\pm0.25$e - $3.13\pm0.25$e $1.94\pm0.11$e $15.47\pm0.28$
$\rm H_2$ 22230 $2.70\pm0.36 $ - - $1.68\pm0.20$c $0.80\pm0.26$e - - $2.51\pm0.30$e -
$\rm H_2$ 22470 - - - $0.89\pm0.20$c - - $0.67\pm0.11$e - -
$\lbrack$Ca VIII] 23218 - - - - - - $1.45\pm0.14 $ - -
a Total Flux of the line.
c Rodríguez-Ardila et al. (2004).
d Teluric absorption.
e Rodríguez-Ardila et al. (2005).


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