\begin{table}%t1
%\centering
\par
\caption{\label{tab:zbins}Mean values for SMGs in redshift bins.}
\par
\begin{tabular}{ccccccccc}
\hline\hline \noalign{\smallskip}
& Volume & $\log\rho_{\rm IR}$  & $\rho_{\rm SFR}$ & & $\log\rho_{*}$ & & & $\log\rho_{\rm dust}$\\
$z$  & ($10^6$~Mpc$^3$) & $(L_\odot~\mbox{Mpc}^{-3})$ & $(M_\odot~\mbox{yr}^{-1}~\mbox{Mpc}^{-3})$ & \multicolumn{1}{c}{\%} & $(M_\odot~\mbox{Mpc}^{-3})$ & \% & $q$ & $(M_\odot~\mbox{Mpc}^{-3})$\\
(1)  & (2) &  (3) & (4) &  (5) & (6) & (7) & (8) & (9)\\
\hline
$0.080{-}0.500$ & $0.12$ & $7.03_{\rm -0.14}^{+0.11}$ & $0.0018\pm0.0005$ & $
           5_{\rm -           2}^{+           3}$ & $6.35_{\rm -0.16}^{+0.21}$ & $
           1_{\rm -           0.2}^{+           0.4}$ & $2.54\pm 0.12$ & $
4.06_{\rm -0.06}^{+0.05}$ \\
$0.510{-}1.316$ & $1.03$ & $7.81_{\rm -0.07}^{+0.06}$ & $0.0111\pm0.0016$ & $
           9_{\rm -           2}^{+           2}$ & $7.16_{\rm -0.08}^{+0.13}$ & $
           5_{\rm -           1}^{+           2}$ & $2.52\pm 0.06$ & $
4.32_{\rm -0.05}^{+0.04}$ \\
$1.408{-}2.142$ & $1.63$ & $8.12_{\rm -0.05}^{+0.05}$ & $0.0228\pm0.0027$ & $          11_{\rm -           3}^{+           3}$ & $7.18_{\rm -0.11}^{+0.16}$ & $
          11_{\rm -           3}^{+           6}$ & $2.29\pm 0.08$ & $3.84_{\rm -0.04}^{+0.04}$ \\
$2.148{-}2.565$ & $0.89$ & $8.45_{\rm -0.05}^{+0.05}$ & $0.0486\pm0.0054$ & $          18_{\rm -           5}^{+           7}$ & $7.61_{\rm -0.08}^{+0.12}$ & $
          51_{\rm -          11}^{+          20}$ & $2.27\pm 0.09$ & $4.35_{\rm -0.04}^{+0.04}$ \\
$2.578{-}3.623$ & $2.17$ & $8.30_{\rm -0.05}^{+0.05}$ & $0.0341\pm0.0040$ & $          20_{\rm -           4}^{+           5}$ & $7.28_{\rm -0.07}^{+0.12}$ & $
          31_{\rm - 7}^{+14}$ & $2.25\pm 0.08$ & $3.86_{\rm -0.03}^{+0.03}$ \\
\hline
\end{tabular}
\tablefoot{Column~(\zrangecol):~redshift range of the bins. Column~(\volcol):~comoving volume of these bins (calculated in Sect.~\ref{sec:bins}). Column~(\lirdcol):~IR luminosty density of SMGs. Column~(\sfrdcol):~Resulting IR SFR density of SMGs (Sect.~\ref{sec:sfrd}). Column~(\sfrdcontrcol):~contribution of SMGs to the cosmic SFR density (calculated in Sect.~\ref{sec:bins}). Column~(\mstardcol):~stellar mass density of SMGs (Sect.~\ref{sec:mstard}). Column~(\mstardcontrcol):~contribution of SMGs to the cosmic $M_*$ density (calculated in Sect.~\ref{sec:bins}). Column~(\qavcol):~mean (and error of the mean) IR-radio correlation parameter for SMGs (Sect.~\ref{sec:firr}). Column~(\mdustdcol):~dust mass density of SMGs (Sect.~\ref{sec:dust}). Columns~(3--7) and (9) have been corrected for incompleteness by a factor of $3.5$ (Sect.~\ref{sec:bins}).}
\vspace*{-3mm}
\end{table}