\begin{table}%T1
       \caption{\label{Halo}\label{tab1}Halo model results using the Lockman-SWIRE $w(\theta)$.}
       \vspace{-2mm}
       \small%\centering
\par
                  \begin{tabular}{ccccccccc}
            \hline\hline
            \noalign{\smallskip}
        Band & Flux density & $N_{\rm gal}$      &  $\langle z \rangle$ & $\log [M_{\rm min}/M_{\odot}]$ & $\log [M_{\rm sat}/M_{\odot}]$ & $\alpha_{\rm s}$ & $\langle b \rangle_z$ & $f_{\rm s}$ \\
                        \hline \noalign{\smallskip}
                         250~$\mu$m & $S \ga  30$~mJy & 8154 & $2.1^{+0.4}_{-0.7}$ & $12.6^{+0.3}_{-0.6}$ & $13.1^{+0.3}_{-0.5}$ & $1.3\pm0.4$ & $2.9 \pm 0.4$& $0.14 \pm 0.08$ \\
             350~$\mu$m & $S \ga  30$~mJy & 4899 &  $2.3^{+0.4}_{-0.7}$ & $12.9^{+0.4}_{-0.6}$ & $>$$13.1$ & $<$$1.8$ & $3.2 \pm 0.5$ & $<$$0.20$\\            
             500~$\mu$m & $S \ga  30$~mJy & 1680 & $2.6^{+0.3}_{-0.7}$ & $13.5^{+0.3}_{-1.0}$ & $>$$13.5$ & $<$$1.6$ & $3.6 \pm 0.8$& $<$$0.24$ \\
             Combined & $S_{\rm 350}/S_{\rm 250} \ga  0.85$ & 3333 & $2.5 \pm 0.4$  & $13.4^{+0.2}_{-0.3}$ & $>$$13.4$ & $<$$1.8$ & $3.4 \pm 0.6$& $<$$0.19$\\
            Combined & $S_{\rm 350}/S_{\rm 250} \la 0.85$ & 3194 & $1.7^{+0.5}_{-0.6}$ & $12.8^{+0.3}_{-0.5}$ &  $>$$12.9$ & $<$$1.9$  & $2.6 \pm 0.6$ & $<$$0.26$\\ 
          \noalign{\smallskip}   \hline
         \end{tabular}
	 \vspace{-1mm}
\tablefoot{See text below Eq.~(2) for  definitions of $M_{\rm min}$, $M_{\rm sat}$, $\alpha_{\rm s}$, $\langle b \rangle_z$, and $f_{\rm s}$.
The redshift range is an approximate estimate based on the colour$-$colour diagram of the source sample through a comparison to
isothermal, modified black-body SEDs with a wide range of dust temperatures and emissivity parameters (see, Fig.~\ref{pz} for an example
involving $S_{250}>30$~mJy and for the two colour cuts).}\vspace{-2mm}
   \end{table}