\begin{table}%t5
\caption{Derived/estimated properties for optical dropout ERO galaxies with near-IR and Spitzer 
detections.
Listed are the object ID (Col.~1), the photometric redshift estimate (Col.~2), the extinction (Col.~3),
the type of the best fit template (Col.~4), the distance modulus corresponding to \zphot\ 
(Col.~5),
the absolute $K\rm s$-band magnitude non-corrected for lensing (Col.~6), 
the absolute rest-frame $K\rm s$-band magnitude non-corrected for lensing (Col.~7),
the estimated stellar mass (from scaling the SED fit or from $M^{\rm rest}(K\rm s)$ assuming
$L_K/M=3.2$, Col.~8), the estimated star formation rate  non-corrected for lensing (Col.~9),
and the age of the stellar population (Col.~10).
To correct the above mentioned absolute quantities for gravitational magnification the appropriate
magnification factors listed in Table~\ref{t_mu} must be used.
\label{t_props}}
%\centerline
 {\begin{tabular}{lllllllll}
\hline
\hline
Object & \zphot\ & \av\ & Template & DM$^a$ & $M^{\rm rest}(K{\rm s})-2.5\log(\mu)$ & ${\rm Mass}\times \mu$ & ${\it SFR}\times \mu$ & Stellar age  \\
       &         & [mag]&          & [mag]  & [mag]  & \msun& \msunyr & [Gyr] \\
\hline 
\noalign{\smallskip}
%ds-updated 19 oct 2006 --> #1
A1835-\#1  & $\sim$0.4--1.5    & ?       &    \multicolumn{5}{l}{Fits uncertain -- see text} \\
%ds-updated 19 oct 2006 --> #2
A1835-\#2  & $\sim$2.8--3 & 2.4--3  & young burst & 47.0 & --27.7 & $\sim$$ 1.2 \times 10^{12}$ & $\sim$2100 & $<$0.36 \\
%ds-updated 19 oct 2006 --> #4
A1835-\#4  & $\sim$1.2    & 0--1.6  & burst/elliptical & 44.60 & --21.6 & $\sim $$1.7 \times 10^{10}$ & $\sim$5 & 0.7 to 4.5 \\
%ds-updated 19 oct 2006 --> #17
A1835-\#17 & $\sim$0.7--0.8 & $\sim$3.8  & burst     & 43.0 & --21.7 & $\sim 1.3 \times 10^{10}$? & $\sim$0.9 &  ? (see text)\\  %0.01, 1 or 7.5 Gyr?\\ 
\\
%ds-updated 18 jan 2007 --> AC114#1
AC114-\#1  & $\sim$1.3--1.6& $\sim$1.6--2.8 & burst & 44.84 & --26.4 & $(1.3{-}2.6) \times 10^{12}$ &  & $\sim$0.9--4.5 Gyr \\
AC114-\#1  & $\sim$1.0     & +3.8      & M51         & 44.03 & --25.9 &                      & $\sim$48 & \\
\hline
\end{tabular}}
\par
\smallskip
{$^a$ Distance modulus computed for minimum redshift.} 
\end{table}