Table 2: Observed fluxes, for type 1 objects, in units of $\rm 10^{-15}~ erg ~ cm^{-2} ~ s^{-1}$.

Ion		 $\rm\lambda_{lab}~(\AA)$ Mrk 334 NGC 1097 MCG -5-13-17 Mrk 124 Mrk 1239 NGC 3227 H 1143-182 PG 1126-041 NGC 4051 NGC 4151

O I		 8446 - - - $13.59\pm1.35$ $86.61\pm6.70$ - - - $79.93\pm4.61$ $130.94\pm15.86 $
Ca II 8498 - - - - - - - - - -
$\lbrack$S III$\rbrack$ 9069 $22.69\pm0.74$ $12.08\pm3.38 $ $18.33\pm0.46$ $4.37\pm0.30 $ $25.27\pm0.80$ $91.57\pm5.41$ $5.93\pm0.49 $ $11.15\pm1.00 $ $26.92\pm2.38$ $266.76\pm6.10 $
Fe II 9127 - - - - - - $1.52\pm0.38$ - $6.70\pm1.67$ -
Fe II 9177 - - - $2.46\pm0.61$d - - $1.25\pm0.31$ - $3.31\pm0.82$ $3.36\pm2.23$k
Fe II 9202 - - - $2.30\pm0.55$ - - $1.13\pm0.28$ - $10.58\pm2.64$ -
H I 9230 - - - - - - - - - $7.49\pm2.03 $
H I 9230(b) - - - - $66.21\pm2.83$ah - $54.60\pm8.61$a $65.96\pm4.16$ ah $19.89\pm4.68$ a $39.71\pm7.40 $
$\lbrack$S III$\rbrack$ 9531 $56.91\pm0.52$ - $38.71\pm0.79$ $17.55\pm0.24 $ $103.30\pm1.21$ $247.79\pm3.40$ $17.96\pm0.60 $ $46.28\pm3.71$ $75.91\pm1.71$ $706.19\pm7.23 $
$\lbrack$C I$\rbrack$ 9824 $2.01\pm0.53$ - - - - - - $1.79\pm0.14$ - -
$\lbrack$C I$\rbrack$ 9850 $3.29\pm0.53$ - $4.64\pm1.60$ $1.00\pm0.10 $ - $13.30\pm1.74$ - $1.15\pm0.11$ $5.92\pm1.41 $ $54.04\pm5.63 $
$\lbrack$S VIII$\rbrack$ 9910 - - $6.61\pm1.54$ - $23.79\pm1.85$ $1.97\pm1.14 $ - $ 2.58\pm0.21$ $13.67\pm1.97$ $40.50\pm2.08 $
Fe II 9999 $2.04\pm0.51$ - - $2.75\pm0.17$ - - - - $11.21\pm1.63$ -
H I 10049 $2.06\pm0.22$ - - - $34.19\pm0.89$ - $14.57\pm1.94 $ - $5.35\pm0.65$ $32.17\pm1.87 $
H I 10049(b) $5.14\pm0.73$ - - - $46.26\pm1.64$ $43.84\pm7.83$a $76.06\pm5.65 $ $104.83\pm3.76$a $33.84\pm2.77$ $288.46\pm14.89^i$
He II 10122 $1.69\pm0.36$ - - - $5.53\pm0.63$ - - - $3.11\pm0.63$ $28.55\pm1.51 $
He II 10122(b) $2.79\pm0.68$ - - - $59.28\pm2.85$ $12.68\pm2.22$a $3.59\pm1.52$a - $14.25\pm2.11$ $65.57\pm7.13^j$
Fe II 10171 - - - - - - - - - -
$\lbrack$S II$\rbrack$ 10286 $1.22\pm0.12$ - - - - $13.28\pm2.68$ $ 1.14\pm0.31 $ - $1.89\pm0.60$ $28.00\pm0.28 $
$\lbrack$S II$\rbrack$ 10320 $1.39\pm0.12$ - - - - $13.73\pm2.68$ $ 1.27\pm0.31 $ - $4.00\pm0.60$ $38.35\pm0.28 $
$\lbrack$S II$\rbrack$ 10336 $0.48\pm0.12$ - - - - $13.40\pm2.68$ $ 0.82\pm0.31 $ - $1.41\pm0.60$ $24.08\pm0.28 $
$\lbrack$S II$\rbrack$ 10370 $0.44\pm0.12$ - - - - $2.78\pm1.43$ - - - $10.40\pm0.28 $
$\lbrack$N I$\rbrack$ 10404 $1.21\pm0.18$ - - - - $13.44\pm4.13$ - - $2.71\pm0.59 $ $16.10\pm0.36 $
Fe II 10500 - - - - $18.66\pm0.91$ - - $13.04\pm2.77 $ - -
He I 10830 $30.95\pm0.70$ - $57.80\pm1.88$ $7.66\pm0.21 $ $98.38\pm1.71$ $163.98\pm1.95$ $73.86\pm1.66 $ - $75.88\pm2.31$ $685.10\pm5.21 $
He I 10830(b) $33.29\pm3.83$ - $125.57\pm15.40$ $ 25.76\pm1.39 $ $173.81\pm4.28$ $298.21\pm7.37$ $255.46\pm5.22 $ $133.30\pm3.65$a $115.37\pm7.55$ $1470.29\pm56.18$
H I 10938 $7.91\pm0.58$ - $2.01\pm0.06 $ $1.13\pm0.17 $ $44.01\pm2.44$ $20.46\pm2.61$ $38.35\pm2.78 $ - $19.14\pm3.38$ $50.28\pm5.64 $
H I 10938(b) $8.56\pm1.82$ - $8.76\pm0.28 $ $9.38\pm0.71 $ $87.04\pm7.32$ $122.01\pm7.43$ $98.31\pm6.45 $ $95.82\pm4.80$a $41.47\pm7.66$ $295.02\pm50.94 $
Fe II 11126 - - - - - - - - - -
O I 11287 $6.32\pm1.03$ - - $ 10.93\pm0.79 $ $50.03\pm1.76$ - $27.93\pm0.89 $ $43.98\pm4.08 $ $47.16\pm2.27$ -
$\lbrack$P II$\rbrack$ 11460 - - - - - - - - - $6.25\pm1.17 $
$\lbrack$P II$\rbrack$ 11886 $3.89\pm0.83$ - - - - $14.76\pm3.23$ - - - $19.70\pm1.01 $
$\lbrack$S IX$\rbrack$ 12520 - - $1.97\pm0.17$ - $15.51\pm2.84$ - $ 1.02\pm0.16 $ - $11.13\pm0.77$ $39.71\pm0.91 $
$\lbrack$Fe II$\rbrack$ 12570 $8.45\pm0.21$e - $4.84\pm0.21$e $ 3.16\pm0.62$c $7.90\pm0.55$c $41.10\pm1.18$c $ 2.54\pm0.45$c - $5.26\pm0.81$c $58.80\pm2.94$c
H I 12820 $14.68\pm0.55$e - $2.14\pm0.65$e - $71.87\pm1.62$ $33.84\pm2.05$ $ 79.78\pm1.59 $ - $20.71\pm0.55$ $108.26\pm0.99 $
H I 12820(b) $18.37\pm2.05$ - $41.69\pm6.11$ 14.6dc $116.25\pm4.77$ $168.74\pm10.23$ $ 84.20\pm3.42 $ $101.83\pm3.70$ad $66.61\pm1.67$ $712.48\pm8.77 $
$\lbrack$Fe II$\rbrack$ 13201 - - - - - $26.79\pm3.72$ - - - $21.48\pm2.14 $
$\lbrack$Si X$\rbrack$ 14300 - - - - $26.15\pm1.85$ - $1.62\pm0.24 $ $5.12\pm1.90$ $22.19\pm1.05$ $37.73\pm1.55 $
$\lbrack$Fe II$\rbrack$ 16436 $6.10\pm0.29$e - - $2.82\pm0.47$c $7.92\pm1.55$c $41.0\pm3.60$c $2.45\pm0.45$c - $6.42\pm0.97$c $56.2\pm1.96$c
H I 18750 $12.59\pm0.40$ - - $ 15.20\pm0.53 $ $50.50\pm2.71$ - $ 106.56\pm1.40 $ - - -
H I 18750(b) $40.24\pm1.02$ - - $31.42\pm2.37 $ $204.60\pm8.74$ $212.11~\pm~4.38$ad $138.66\pm3.05 $ $139.53~\pm~1.84$a $111.49\pm4.27$ad $581.50\pm12.04$ad
H I 19446 - - - - - - $ 1.44\pm0.52 $ - - $6.02\pm1.16??$
H I 19446(b) $2.03\pm0.14$a - - - $31.14\pm4.07$a - $21.38\pm1.08 $ $7.58\pm2.05$a $8.52\pm0.36$a $17.92\pm4.32 $
$\rm H_2$ 19570 $3.80\pm0.23$e $6.57\pm0.64$e $2.88\pm0.36$e $0.91\pm0.16$c - $20.8\pm1.2$c - $9.17\pm2.84$ $7.51\pm0.62$c $21.2\pm2.0$c
$\lbrack$Si VI$\rbrack$ 19641 - - $5.69\pm0.62$ - - - $3.09\pm0.36 $ $1.23\pm0.37$ $12.54\pm1.19$ $68.71\pm2.05 $
$\rm H_2$ 20332 $1.35\pm0.08$e $2.22\pm0.35$e $0.59\pm0.12$e $0.36\pm0.05$c - $7.97\pm0.92$c - - $2.82\pm0.70$c $6.84\pm0.42$c
He I 20580 - - - - - - - - - -
He I 20580(b) $2.09\pm0.02$a - - - - $5.71\pm1.43$a - - - -
$\rm H_2$ 21213 $2.72\pm0.17$e $3.89\pm1.16$e $2.04\pm0.10$e $0.90\pm0.12$c - $17.7\pm1.00$c - - $5.81\pm0.37 $ $14.7\pm0.55$c
H I 21654 $4.69\pm0.15$fe - - - - $6.51\pm1.34 $ $2.49\pm0.37 $ - - $12.42\pm0.63 $
H I 21654(b) - - $0.78\pm0.06$ae $2.49\pm0.55$ca $32.00\pm1.50$ca $21.54\pm6.31$ $ 22.46\pm1.02 $ $13.33\pm0.73$a $13.1\pm0.84$ca $31.41\pm2.64 $
$\rm H_2$ 22230 - - - $0.28\pm0.08$c - $3.67\pm0.66$c - - $1.52\pm0.40$c $5.04\pm0.62$c
$\rm H_2$ 22470 - - - - - $2.32\pm0.21$c $0.24\pm0.08$c - - -
$\lbrack$Ca VIII$\rbrack$ 23218 - - - - $5.66\pm1.61 $ - - - $2.36\pm0.44 $ $15.09\pm1.02$
a Total Flux of the line.
b Broad Component of the line.
c Rodríguez-Ardila et al. (2004).
d Teluric absorption.
e Rodríguez-Ardila et al. (2005).
f Total flux. Line without broad component.
h Blend with Fe II $\lambda$9177 $\AA$ and Fe II $\lambda$9202$\AA$.
i Blend with Fe II$\lambda$ 9999 $\AA$.
j Blend with Fe II$\lambda$ 10 171 $\AA$.
k Blend with Fe II$\lambda$ 9202 $\AA$.


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