\begin{table}%t1
%\centering
\par
\caption{Fluxes of selected regions in the ultraviolet, H$\alpha$, and mid-infrared (3.6, 4.5, and 8.0~$\mu$m). The "--'' symbol indicates that the region falls outside the field of view, "$\le$'' means the aperture is heavily polluted by stars and the flux is therefore likely being overestimated and "$\ge$'' means the aperture does not contain all of the object, e.g., to avoid a foreground object, the actual flux then being underestimated.}
\label{tab:fluxes}
\small\begin{tabular}{c c c c c c c c}
\hline\hline
Region&GALEX name&DM98&$F_{\rm NUV}$&$F_{{\rm H}\alpha}$&$F_{\rm IR3.6}$&$F_{\rm IR4.5}$&$F_{\rm IR8.0}$\\
&(IAU name)&&($\mu$Jy)&($10^{-18}$~W~m$^{-2}$)&($\mu$Jy)&($\mu$Jy)&($\mu$Jy)\\\hline
1&\object{J134717.57-302821.11}&&274~$\pm$~20&33.2~$\pm$~10.0&331~$\pm$~101&254~$\pm$~35&640~$\pm$~99\\
2&\object{J134722.91-302750.19}&&92~$\pm$~7&10.7~$\pm$~3.3&144~$\pm$~41&98~$\pm$~23&629~$\pm$~41\\
3&\object{J134723.00-302724.31}&a&150~$\pm$~11&18.8~$\pm$~5.7&385~$\pm$~24&251~$\pm$~32&2088~$\pm$~55\\
4&\object{J134719.76-302648.77}&&53~$\pm$~4&4.3~$\pm$~1.3&131~$\pm$~12&118~$\pm$~15.4&207~$\pm$~27\\
5&\object{J134723.86-302646.25}&c&98~$\pm$~7&5.9~$\pm$~1.9&221~$\pm$~28&179~$\pm$~35&805~$\pm$~63\\
6&\object{J134720.69-302642.66}&&14~$\pm$~2&1.5~$\pm$~0.5&31~$\pm$~5.4&28~$\pm$~7&97~$\pm$~12\\
7&\object{J134724.51-302635.91}&&14~$\pm$~1&0.6~$\pm$~0.2&53~$\pm$~12&44~$\pm$~5&73~$\pm$~12\\
8&\object{J134717.79-302634.82}&&6~$\pm$~1&1.0~$\pm$~0.3&31~$\pm$~7&31~$\pm$~3&60~$\pm$~7\\
9&\object{J134723.95-302622.21}&d&23~$\pm$~2&1.5~$\pm$~0.5&84~$\pm$~15&61~$\pm$~6&176~$\pm$~15\\
10&\object{J134726.10-302602.63}&&14~$\pm$~1&1.4~$\pm$~0.5&112~$\pm$~26&95~$\pm$~10&278~$\pm$~26\\
11&\object{J134726.66-302552.06}&e&34~$\pm$~3&2.5~$\pm$~0.8&199~$\pm$~18&138~$\pm$~8&384~$\pm$~18\\
12&\object{J134726.45-302545.78}&&31~$\pm$~3&4.3~$\pm$~1.3&229~$\pm$~34&169~$\pm$~13&509~$\pm$~34\\
13&\object{J134723.37-302524.51}&&12~$\pm$~1&1.3~$\pm$~0.4&188~$\pm$~18&135~$\pm$~8&311~$\pm$~19\\
14&\object{J134700.56-302518.62}&&62~$\pm$~5&--&--&--&--\\
15&\object{J134727.77-302504.89}&&5~$\pm$~1&0.8~$\pm$~0.3&70~$\pm$~9&50~$\pm$~5&189~$\pm$~10\\
16&\object{J134717.92-302158.54}&f&14~$\pm$~1&1.4~$\pm$~0.4&50~$\pm$~10&41~$\pm$~6&286~$\pm$~12\\
17&\object{J134718.08-302150.30}&&12~$\pm$~1&1.3~$\pm$~0.4&52~$\pm$~9&37~$\pm$~6&377~$\pm$~11\\
18&\object{J134722.47-302144.13}&g&30~$\pm$~2&3.3~$\pm$~1.0&146~$\pm$~28&104~$\pm$~13&1047~$\pm$~30\\
19&\object{J134720.94-302131.97}&&18~$\pm$~1&1.6~$\pm$~0.5&96~$\pm$~18&51~$\pm$~7&267~$\pm$~18\\
20&\object{J134717.91-302121.48}&h&87~$\pm$~6&7.8~$\pm$~2.4&287~$\pm$~58&244~$\pm$~22&1428~$\pm$~58\\
21&\object{J134720.86-302055.70}&i&259~$\pm$~18&46.3~$\pm$~13.9&638~$\pm$~38&534~$\pm$~51&5236~$\pm$~90\\
22&\object{J134718.18-302042.76}&&30~$\pm$~2&2.1~$\pm$~0.7&63~$\pm$~27&34~$\pm$~16&427~$\pm$~27\\
23&\object{J134721.66-302041.66}&&17~$\pm$~1&1.5~$\pm$~0.5&14~$\pm$~17&no detection&114~$\pm$~17\\
24&\object{J134717.07-302035.59}&&21~$\pm$~2&1.9~$\pm$~0.6&1.7~$\pm$~20&25~$\pm$~11&31~$\pm$~20\\
25&\object{J134717.97-302031.99}&&15~$\pm$~1&1.2~$\pm$~0.4&38~$\pm$~13&29~$\pm$~8&235~$\pm$~14\\
26&\object{J134721.14-302026.07}&&9~$\pm$~1&0.7~$\pm$~0.2&--&--&--\\
27&\object{J134719.74-302025.73}&j&44~$\pm$~3&4.2~$\pm$~1.3&116~$\pm$~23&100~$\pm$~14&614~$\pm$~24\\
28&\object{J134717.69-302018.20}&&33~$\pm$~3&2.3~$\pm$~0.8&--&--&--\\
29&\object{J134717.81-301958.85}&k&41~$\pm$~3&2.5~$\pm$~0.9&--&--&--\\\hline
Seashell&J134723.17-302504.23&&98~$\pm$~7&5.6~$\pm$~1.9&14412~$\pm$~84&8734~$\pm$~40&5319~$\pm$~78\\
NGC~5291&J134717.81-302424.87&&$\ge$293~$\pm$~24&$\ge$26.2~$\pm$~9.0&$\ge$48619~$\pm$~385&$\ge$29195~$\pm$~141&$\ge$24846~$\pm$~374\\
HI concentration&J134721.02-302311.33&&71~$\pm$~8&--&$\le$704~$\pm$~177&$\le$618~$\pm$~60&1520~$\pm$~179\\
\hline
\end{tabular}
\end{table}