\begin{table}%t2
    \small  \caption{Measured fluxes and albedos}
         \label{FluxAlb}
        %\centerline
{ \begin{tabular}{l c c c c c c}
            \hline\hline
            \noalign{\smallskip}
            Date  & $\lambda$ & Color & Flux$^{ {b}}$ & $\Delta$Flux
	          & $p_{\lambda}^{ {b,c}}$ & $\Delta$$p_{\lambda}$ \\
	      & ($\mu$m) & Corr.$^{ {a}}$ & ($\mu$Jy) & ($\mu$Jy) &
	      &  \\
                       \hline
                       5 Feb. 2006 & 3.6 & 1.0046 & 4.41 & 0.47 & 0.228 & 0.024 \\
                       & 4.5 & 1.0131 & 3.18 & 0.53 & 0.250 & 0.042 \\
                       & 5.8 & 1.0137 & $<$18.54 &  & $<$2.39 & \\
                       & 8.0 & 1.0305 & $<$26.58 &  & $<$6.24 & \\
            \noalign{\smallskip}
            9 Feb. 2006 & 3.6 & 1.0014 & 3.31 & 0.41 & 0.172 & 0.021 \\
                       & 4.5 & 1.0039 & 2.79 & 0.59 & 0.220 & 0.047 \\
                       & 5.8 & 1.0137 & $<$15.03 &  & $<$1.94 & \\
                       & 8.0 & 1.0305 & $<$32.67 &  & $<$7.69 & \\
                        \hline
         \end{tabular}}
\smallskip
 $^{{a}}$ Aperture photometry has been divided by this factor;  $^{{b}}$ Values for 5.8 and 8.0~$\mu$m are 3$\sigma$ upper limits; $^{{c}}$ Geometric albedo.  Assumes $R=722$~km
(consistent with $p_{{\rm v}}=0.15$).
   \end{table}