\begin{table}%t2
\caption{Comparison between two sets of model runs for coronene
(C$_{24}$H$_{12}$) in different exciting RFs. For each model 
run and each band, we list the absolute integrated flux and, in parentheses, 
the flux fraction.
\label{coronene_jobmul_table}}
%\centerline
 {
\begin{tabular}{ccccccc}
\hline \hline 
\noalign{\smallskip}
& \multicolumn{2}{c}{ISRF} & \multicolumn{2}{c}{Red Rectangle} & 
\multicolumn{2}{c}{IRAS~21282+5050}\\
Peak & model~1$^{a}$ & model~2$^{b}$ & model~1$^{a}$ & model~2$^{b}$ & 
model~1$^{a}$ & model~2$^{b}$ \\
($\mu$m) & (W$ $sr$^{-1}$) (\%) & (W$ $sr$^{-1}$) (\%) & (W$ $sr$^{-1}$) (\%) & 
(W$ $sr$^{-1}$) (\%) & (W$ $sr$^{-1}$) (\%) & (W$ $sr$^{-1}$) (\%) \\
\hline \noalign{\smallskip}
3.26 & $3.8 \times 10^{-27}$ (37.96) & $3.9 \times 10^{-27}$ (38.15) & 
$5.8 \times 10^{-26}$ (24.76) & $6.3 \times 10^{-26}$ (25.36) & 
$4.3 \times 10^{-22}$ (46.68) & $4.2 \times 10^{-22}$ (46.50) \\
3.29 & $2.6 \times 10^{-28}$ (2.58) & $2.6 \times 10^{-28}$ (2.56) & 
$4.0 \times 10^{-27}$ (1.72) & $4.2 \times 10^{-27}$ (1.70) & 
$2.9 \times 10^{-23}$ (3.18) & $2.9 \times 10^{-23}$ (3.16) \\
6.24 & $5.2 \times 10^{-28}$ (5.15) & $5.4 \times 10^{-28}$ (5.21) & 
$1.3 \times 10^{-26}$ (5.47) & $1.4 \times 10^{-26}$ (5.51) & 
$4.6 \times 10^{-23}$ (5.01) & $4.5 \times 10^{-23}$ (5.00) \\
6.69 & $9.2 \times 10^{-30}$ (0.09) & $9.7 \times 10^{-30}$ (0.09) & 
$2.4 \times 10^{-28}$ (0.10) & $2.6 \times 10^{-28}$ (0.11) & 
$8.0 \times 10^{-25}$ (0.09) & $6.9 \times 10^{-25}$ (0.08) \\
7.21 & $1.1 \times 10^{-28}$ (1.07) & $1.1 \times 10^{-28}$ (1.08) & 
$2.8 \times 10^{-27}$ (1.22) & $3.1 \times 10^{-27}$ (1.24) & 
$9.1 \times 10^{-24}$ (0.99) & $8.8 \times 10^{-24}$ (0.97) \\
7.63 & $6.6 \times 10^{-28}$ (6.59) & $7.0 \times 10^{-28}$ (6.77) & 
$1.7 \times 10^{-26}$ (7.49) & $1.9 \times 10^{-26}$ (7.73) & 
$5.5 \times 10^{-23}$ (6.05) & $5.5 \times 10^{-23}$ (6.10) \\
8.25 & $3.0 \times 10^{-28}$ (2.92) & $3.0 \times 10^{-28}$ (2.93) & 
$8.0 \times 10^{-27}$ (3.42) & $8.7 \times 10^{-27}$ (3.53) & 
$2.4 \times 10^{-23}$ (2.63) & $2.4 \times 10^{-23}$ (2.64) \\
8.78 & $3.1 \times 10^{-28}$ (3.10) & $3.3 \times 10^{-28}$ (3.21) & 
$8.8 \times 10^{-27}$ (3.79) & $9.5 \times 10^{-27}$ (3.82) & 
$8.8 \times 10^{-23}$ (2.75) & $2.5 \times 10^{-23}$ (2.75) \\
11.57 & $3.4 \times 10^{-27}$ (33.25) & $3.5 \times 10^{-27}$ (33.89) & 
$9.9 \times 10^{-26}$ (42.48) & $1.1 \times 10^{-25}$ (42.72) & 
$2.6 \times 10^{-22}$ (27.89) & $2.5 \times 10^{-22}$ (28.02) \\
12.43 & $1.1 \times 10^{-29}$ (0.11) & $1.1 \times 10^{-29}$ (0.11) & 
$3.3 \times 10^{-28}$ (0.14) & $3.7 \times 10^{-28}$ (0.15) & 
$8.0 \times 10^{-25}$ (0.09) & $8.3 \times 10^{-25}$ (0.09) \\
12.90 & $1.6 \times 10^{-28}$ (1.56) & $1.6 \times 10^{-28}$ (1.60) & 
$4.7 \times 10^{-27}$ (2.03) & $5.3 \times 10^{-27}$ (2.12) & 
$1.2 \times 10^{-23}$ (1.29) & $1.2 \times 10^{-23}$ (1.30) \\
18.21 & $3.9 \times 10^{-28}$ (3.91) & $4.1 \times 10^{-28}$ (4.01) & 
$1.2 \times 10^{-26}$ (5.29) & $1.3 \times 10^{-26}$ (5.44) & 
$2.8 \times 10^{-23}$ (3.04) & $2.8 \times 10^{-23}$ (3.11) \\
%$[18.46]$ & $2.5 \times 10^{-30}$ (0.03) & & $6.3 ~~ 10^{-29}$ (0.04) & & \textemdash{} &\\
%$[19.11]$ & $1.6 ~~ 10^{-30}$ (0.02) & & $4.2 ~~ 10^{-29}$ (0.02) & & \textemdash{} &\\
%$[20.07]$ & $4.1 ~~ 10^{-30}$ (0.04) & & $8.8 ~~ 10^{-29}$ (0.05) & & \textemdash{} &\\
%$[20.97]$ & $2.2 ~~ 10^{-30}$ (0.02) & & $5.2 ~~ 10^{-29}$ (0.03) & & \textemdash{} &\\
%$[21.15]$ & $2.2 ~~ 10^{-30}$ (0.02) & & $5.1 ~~ 10^{-29}$ (0.03) & & \textemdash{} &\\
%$[22.28]$ & $6.0 ~~ 10^{-30}$ (0.06) & \textemdash& $1.8 ~~ 10^{-28}$ (0.08) & \textemdash& \textemdash& \textemdash\\
26.20 & $2.8 \times 10^{-29}$ (0.28) & $2.3 \times 10^{-29}$ (0.22) & 
$9.7 \times 10^{-28}$ (0.42) & $7.8 \times 10^{-27}$ (0.32) & 
$1.8 \times 10^{-24}$ (0.19) & $1.5 \times 10^{-24}$ (0.16)\\
%$[27.34]$ & $9.5 ~~ 10^{-30}$ (0.09) & \textemdash& $3.1 ~~ 10^{-28}$ (0.13) & \textemdash& \textemdash{} & \textemdash\\
%$[33.59]$ & $1.4 ~~ 10^{-29}$ (0.13) & \textemdash& $4.1 ~~ 10^{-28}$ (0.18) & \textemdash& \textemdash{} & \textemdash\\
%$[34.34]$ & $1.5 ~~ 10^{-29}$ (0.15) & \textemdash& $4.4 ~~ 10^{-28}$ (0.19) & \textemdash& \textemdash{} & \textemdash\\
%$[44.57]$ & $1.0 ~~ 10^{-29}$ (0.10) & \textemdash& $2.9 ~~ 10^{-28}$ (0.12) & \textemdash& \textemdash{} & \textemdash\\
%$[61.10]$ & $1.3 ~~ 10^{-29}$ (0.13) & \textemdash& $3.1 ~~ 10^{-28}$ (0.13) & \textemdash& \textemdash{} & \textemdash\\
80.60 & $2.4 \times 10^{-29}$ (0.24) & $1.6 \times 10^{-29}$ (0.16) & 
$8.4 \times 10^{-28}$ (0.36) & $6.0 \times 10^{-28}$ (0.24) & 
$1.0 \times 10^{-24}$ (0.11) & $7.6 \times 10^{-25}$ (0.08)\\
 \hline
\end{tabular}}
\par
\smallskip
$^{a}$ Results from the present model based on \citet{mul98}, neglecting 
the possibility of ionisation for a consistent comparison (see text);\\ 
$^{b}$ Results from the corrected (see text) model of \citet{job02}.
\end{table}