\begin{table}%t1
\par
\caption{\label{tab:qso_photometry}Average stacked QSO $100~\mu$m rest-frame luminosities for bins in redshift and $I$-band
absolute magnitude.  }
\small%\centering
\par
\begin{tabular}{lllllll}
\hline\hline\noalign{\smallskip}
$N$ & $z_{\rm min}$ & $z_{\rm max}$ & $I_{\rm min}$ & $I_{\rm max}$ & $\nu L_\nu(100~\mu{\rm m})$ & SFD\\
    &              &             & (AB)         & (AB)         & $/10^{12}~L_\odot$ & $/$($M_\odot$ yr$^{-1}$ Mpc$^{-3}$)\\
\hline\noalign{\smallskip} 
 6  & $0.05$       & $0.5$       &$-22$         & $-19$        &  $0.126\pm 0.069$ & $(2.0\pm1.1)\times10^{-4}$\\ %%
 72 & $0.05$       & $0.5$       &$-24$         & $-22$        &  $0.115\pm 0.019$ & $(4.94\pm0.79)\times10^{-5}$\\ %%
 29 & $0.05$       & $0.5$       &$-26$         & $-24$        &  $0.31\pm  0.13 $ & $(3.6\pm1.5)\times10^{-6}$\\ %%
 9  & $0.05$       & $0.5$       &$-28$         & $-26$        &  $0.52\pm  0.38$ & $(8.8\pm6.4)\times10^{-8}$\\ %%
 9  & $0.5$        & $1$         &$-22$         & $-19$        &  $0.028\pm 0.065$ & $(0.5\pm1.2)\times10^{-4}$\\ %%
 73 & $0.5$        & $1$         &$-24$         & $-22$        &  $0.173\pm 0.034 $ & $(1.58\pm0.31)\times10^{-4}$\\ %%
 38 & $0.5$        & $1$         &$-26$         & $-24$        &  $0.400\pm 0.084 $ & $(6.1\pm1.3)\times10^{-5}$\\ %%
 5  & $0.5$        & $1$         &$-28$         & $-26$        &  $1.54\pm  0.24$ & $(4.06\pm0.63)\times10^{-6}$\\ %%
 2  & $0.5$        & $1$         &$-32$         & $-28$        &  $5.5\pm   4.5$ & $(4.9\pm4.0)\times10^{-8}$\\ %%
 46 & $1$          & $2$         &$-24$         & $-22$        &  $0.218\pm  0.090 $ & $(2.4\pm1.0)\times10^{-4}$\\ %%
 223& $1$          & $2$         &$-26$         & $-24$        &  $0.727\pm 0.092$ & $(5.38\pm0.69)\times10^{-4}$\\ %%
 75 & $1$          & $2$         &$-28$         & $-26$        &  $1.81\pm  0.26 $ & $(8.6\pm1.2)\times10^{-5}$\\ %%
 32 & $1$          & $2$         &$-32$         & $-28$        &  $5.1\pm   1.9 $ & $(8.6\pm3.2)\times10^{-7}$\\ %%
 6  & $2$          & $4$         &$-24$         & $-22$        &  $1\pm17$ & $(0.4\pm8)\times10^{-3}$\\ %%
 52 & $2$          & $4$         &$-26$         & $-24$        &  $1.05\pm  0.54 $ & $(3.9\pm2.0)\times10^{-4}$\\ %%
 108& $2$          & $4$         &$-28$         & $-26$        &  $3.47\pm  0.68 $ & $(3.30\pm0.65)\times10^{-4}$\\ %%
 66 & $2$          & $4$         &$-32$         & $-28$        &  $5.42\pm  0.76 $ & $(9.9\pm1.4)\times10^{-6}$\\ %%
 1  & $4$          & $7$         &$-24$         & $-22$        &  $1.7\pm   1.9 $ & $(2.1\pm2.4\times10^{-5}$\\ %%
 1  & $4$          & $7$         &$-26$         & $-24$        &  $2.0\pm   2.2 $ & $(1.9\pm2.1)\times10^{-5}$\\ %%
 58 & $4$          & $7$         &$-28$         & $-26$        &  $2.32\pm  0.46 $ & $(5.6\pm1.1)\times10^{-6}$\\ %%
 64 & $4$          & $7$         &$-32$         & $-28$        &  $4.25\pm  0.69$ & $(1.95\pm0.32)\times10^{-7}$\\ 
 \hline
\end{tabular}
\tablefoot{An M~82 SED has been assumed, though the results are only very weakly
dependent on the assumed SED. The first column gives the number of QSOs in the
bin in question. The final column gives the comoving volume-averaged star formation densities  
of QSO host galaxies in each bin.}
\end{table}