\begin{table}%t1
\caption{Physical properties of the sample.} 
{{\small 
{
\begin{tabular}{cccccccccccccccc}
\hline\hline
\noalign{\smallskip}
Galaxy  & $d$ & $i$  & $L_{\rm 1.4~GHz}$ & $L_{\rm FIR}$ & $L_{\rm B_{T}^{0}}$   & $L_{\rm UV}$  & $L_{\rm H\alpha}$  & $L_{\rm X,soft}$ &${\it SFR}_{\rm FIR}$ & ${\it SFR}_{\rm H\alpha}$ & $\dot{E}_{\rm A}^{\rm tot}$ & $L_{\rm FIR}/D_{25}^{2}$& $M_{\rm bar}$ & $M_{\ion{H}{i}}$ & $M_{\rm dust}$  \\ 
 & [Mpc]& $[\degr]$& [$10^{38}~{\rm erg\ s^{-1}}$] & \multicolumn{3}{c}{[$10^{43}~{\rm erg\ s^{-1}}$]} & \multicolumn{2}{c}{[$10^{40}~{\rm erg\ s^{-1}}$]} & \multicolumn{2}{c}{[${M}_{\odot}\ {\rm yr}^{-1}$]} & [$10^{-3}~{\rm erg~s^{-1} cm^{-2}}$] & [$10^{40}~{\rm erg\ s^{-1}\ kpc^{-2}}$] &  \multicolumn{2}{c}{[$10^{10}~{M}_{\odot}$]} & [$10^{6}~{M}_{\odot}$] \\
\noalign{\smallskip}
(1) & (2)& (3) & (4) & (5) & (6) & (7) & (8) & (9) & \multicolumn{2}{c}{(10)} & (11) & (12) & (13) & (14) & (15) \\ 
\noalign{\smallskip}
\hline
NGC~0891 &  9.5& 88& 1.19$^{a}$& 9.62&5.59&0.11 &   3.54$^{h}$&  0.70$^{r}$    &4.32& 0.28& 3.90$^{u}$ & 6.92 & 10.6 & 0.45 & 2.02 \\
NGC~3044 & 17.2& 84& 0.62$^{b}$& 4.06&3.61&---  &   8.83$^{j}$&  0.09$^{r}$    &1.83& 0.70& 0.94$^{g}$ & 8.52 &3.28  & 0.64 & 0.49 \\
NGC~3221 & 54.8& 77& 3.29$^{b}$& 36.0&8.28&---  &        ---  &  1.07$^{r}$    &16.2& --- & 2.20$^{u}$ & 13.5 & 1.63 & 1.70 & 6.55 \\
NGC~3628 & 10.0& 80& 0.93$^{b}$& 7.66&6.54&0.12 &   2.30$^{k}$&  0.74$^{r}$    &3.45& 0.18& 12.2$^{u}$ & 8.24 & 11.3 & 0.38 & 0.85 \\
NGC~3877 & 12.1& 83& 0.10$^{b}$& 1.92&2.34&0.12 &   ---       &  0.02$^{r}$    &0.86& --- & 0.77$^{u}$ & 5.14 & 1.28 & 0.17 & 0.52 \\
NGC~4631 &  7.5& 86& 1.22$^{b}$& 6.63&7.00&1.15 &   14.3$^{k}$&  0.78$^{r}$    &2.99& 1.13& 0.83$^{g}$ & 7.76 & 2.56 & 0.68 & 0.69 \\
NGC~4634 & 19.1& 83& 0.21$^{c}$& 2.53&1.46&0.14 &   6.40$^{j}$&  0.15$^{r}$    &1.14& 0.51& 2.62$^{u}$ & 12.4 & 1.63 & 0.05 & 0.58 \\
NGC~4666 & 20.2& 80& 2.64$^{b}$& 23.0&7.56&1.01 &   57.5$^{d}$&  1.42$^{r}$    &10.3& 4.55& 4.46$^{g}$ & 31.9 & 5.44 & 0.61 & 3.77 \\
NGC~5775 & 26.7& 84& 2.82$^{b}$& 25.7&8.05&---  &   23.4$^{l}$&  1.55$^{r}$    &11.6& 1.85& 3.26$^{g}$ & 24.6 & 6.09 & 0.97 & 4.39 \\
\noalign{\smallskip}                                           
\hline                                     
M~82     &  3.6& 82& 2.10$^{b}$& 20.9&16.7& 0.06&   14.4$^{h}$& 5.15$^{k}$     &9.39& 1.14& 19.6$^{\ ~}$ & 151  & 1.86 & 0.16 & 0.54 \\
NGC~0253 &  2.6& 79& 0.53$^{b}$& 7.93&3.42& 0.11&   4.90$^{h}$& 0.55$^{k}$     &3.57& 0.39& 2.74$^{\ ~}$ & 18.3 & 10.6 & 0.60 & 0.41 \\
NGC~1482 & 22.1& 58& 3.04$^{b}$& 20.1&10.4& --- &   9.60$^{k}$& 3.70$^{k}$     &9.65& 0.76& 64.9$^{\ ~}$ & 80.7  & 3.58 & 0.06 & 1.16 \\
NGC~3079 & 17.1& 85& 5.88$^{b}$& 21.3&6.94& 0.76&   9.00$^{k}$& 3.20$^{k}$     &9.60& 0.71& 33.6$^{\ ~}$ & 13.7 & 14.1 & 1.10 & 2.74 \\
NGC~4244 &  3.6& 85&0.002$^{c}$& 0.11&0.54& 0.01&   0.42$^{k}$& 0.007$^{k}$    &0.05&0.03& 0.05$^{g}$ & 0.36 & 0.62 & 0.09 & 0.06 \\
NGC~4945 &  3.7& 78& 1.51$^{c}$& 12.5&5.05& --- &   2.40$^{k}$& 0.34$^{k}$     &5.62& 0.19& 4.50$^{u}$ & 27.1 & 5.24 & 0.09 & 1.69 \\
NGC~6503 &  5.2& 75& 0.03$^{b}$& 0.46&0.69& 0.11&   0.76$^{k}$& 0.07$^{k}$     &0.21& 0.06& 1.00$^{\ ~}$ & 4.04 & 1.17 & 0.13 & 0.13 \\
\noalign{\smallskip}                                           
\hline                                         
NGC~0055 & 1.6 & 80& \hspace{0.03cm}0.02$^{a}$& 0.95&0.79& 0.09&   2.00$^{m}$&\hspace{0.07cm}0.31$^{s}$ & 0.12 & 0.16 & 0.11$^{\ }$ & 1.12 & 5.65 & 0.16 & 0.05 \\
NGC~1511 & 17.5& 72& 0.82$^{f}$& 10.1&3.21& --- &   3.63$^{n}$& 0.26$^{n}$     &4.54& 0.29& 0.34$^{n}$ & 32.4 & 0.92 & 0.54 & 0.77 \\
NGC~3556 & 14.1& 79& 1.71$^{b}$& 9.92&8.05& 0.62& \hspace{0.1cm}7.60$^{i}$& 2.00$^{t}$     &4.46& 0.60 & 2.85$^{e}$ & 6.96 & 3.97 & 0.93 & 1.70 \\
NGC~4522 & 16.0& 79& 0.10$^{c}$& 0.60&1.42& 0.10&   1.30$^{o}$& 0.89$^{o}$     &0.27& 0.10& \hspace{0.03cm}0.58$^{\ ~}$ & 2.00 & 1.55 & 0.05 & 0.21 \\
NGC~4565 & 9.7 & 89& 0.22$^{b}$& 1.60&7.47& 0.07&   1.20$^{p}$& 0.26$^{p}$     &0.72& 0.09& 0.09$^{g}$ & 0.80 & 16.5 & 1.30 & 1.19 \\
NGC~4656 & 7.5 & 90& 0.02$^{b}$& 0.48&1.78& 0.02&   1.41$^{v}$& 0.03$^{p}$     &0.22& 0.11& 0.05$^{g}$ & 0.44 & 1.81 & 0.39 & 0.04 \\
NGC~5907 & 14.9& 86& 0.35$^{b}$& 4.32&2.74& 0.01& \hspace{0.035cm}5.57$^{q}$& 0.05$^{p}$     &1.89& 0.44& 0.14$^{g}$ & 1.63 & 15.4 & 1.38 & 2.56 \\
\hline
\end{tabular}}
\smallskip
{Notes:  Columns~(1) to~(3): name, distance, and inclination of the target; Col.~(4): radio continuum luminosities measured at~1.49~GHz; Col.~(5): FIR-luminosities calculated from revised IRAS~$S_{60}$ and $S_{100}$ flux densities \citep{Sa03}; Col.~(6): total $B_{\rm {T}}^{\rm 0}$ luminosities calculated from RC3 \citep{rc3} and corrected for redshift, Galactic, and internal extinction, assuming reddening values from \citep{BH}; Col.~(7): de-reddened UV-continuum luminosities measured at~1650~\AA\ \citep{Rif95} and~1550~\AA\ \citep{CW82}, respectively. The UV flux for NGC~4656 has been determined at~2270~\AA\ \citep{Ma96}. No correction for redshift has been applied; Col.~(8): H$\alpha+[\ion{N}{ii}]$-luminosities, uncorrected for extinction and [\ion{N}{ii}]-contamination; Col.~(9): integrated (disk+halo) diffuse X-ray luminosities obtained from spectral fitting between 0.3 and 2.0~keV, for NGC~3221 and NGC~3877 disk only; Col.~(10): total star formation rate, based on FIR and H$\alpha$ luminosities according to \citep{ken98}; Col.~(11): SN energy input rates per unit area \citep{Da95,Co92} for $M>5~M_{\odot}$; Col.~(12):~the optical diameter of the 25th~magnitude isophote ($D_{25}$) was taken from RC3 \citep{rc3}; Col.~(13): baryonic masses were calculated according to \citet{bj01}; Col.~(14):~to derive the \ion{H}{i} gas mass, we used $M_{\ion{H}{i}}=4.78\times 10^5~d^2~S(\ion{H}{i})$, where $S(\ion{H}{i})$, the total \ion{H}{i} flux in units of [Jy~km~s$^{-1}$] has been taken from \citet{HR89};  Col.~(15): dust masses were calculated following \citet{Hb83}. \\
References:\quad  {\small $(a)$} \citet{Co96}; {\small $(b)$} \citet{Co90}; {\small $(c)$} \citet{Co98}; {\small $(d)$} \citet{Da97}; {\small $(e)$} \citet{Ir99}; {\small $(f)$} \citet{Da01}; {\small $(g)$} \citet{Da95}; {\small $(h)$}~\citet{Bell03}; {\small $(i)$} \citet{Yo96}; {\small $(j)$} \citet{Ro00}; {\small $(k)$} \citet{St04a}; {\small $(l)$} \citet{lehe}; {\small $(m)$} \citet{Fe96}; {\small $(n)$} \citet{Da03}; {\small $(o)$} \citet{keko}; {\small $(p)$} \citet{Vo96}; {\small $(q)$} Rand (priv. com.); {\small $(r)$} \citet{Tu05}; {\small $(s)$} \citet{schlegel}; {\small $(t)$} \citet{Wa03}; {\small $(u)$} \citet{Ro03}; {\small $(v)$} Aldering (priv. com.).}}}  
\label{tab1}
\end{table}