\begin{table}%t2
%\centering
\par
\caption {\label{tab:2}Log-normal fit parameters for various clouds.  }
    
    %\centerline
 \begin{tabular}{lcc}
    \hline\hline
      Cloud & $A_1$ & $\sigma$ \\ 
      \hline
      Lupus V & 0.15 & 0.42 \\
      Coalsack & 0.38 & 0.28 \\
      Taurus & 0.18 & 0.49 \\
      Lupus I & 0.08 & 0.43 \\
      Ophiuchus & 0.16 & 0.48 \\
      Serpens & 0.33 & 0.51 \\
      Cha I & 0.11 & 0.35 \\
      Cha II & 0.12 & 0.35 \\
      Lupus III & 0.14 & 0.35 \\
      Cor A & 0.10 & 0.44 \\
      LDN 1228 & 0.12 & 0.32 \\
      Pipe & 0.42 & 0.29\\
      \hline
    \end{tabular}
    \begin{tabular}{lcc}
    \hline\hline
      Cloud & $A_1$ & $\sigma$ \\ 
      \hline
      LDN 134 & 0.10 & 0.39 \\
      LDN 204 & 0.14 & 0.41 \\
      LDN 1333 & 0.12 & 0.38 \\
      LDN 1719 & 0.15 & 0.50 \\
      Musca & 0.08 & 0.45 \\
      Cha 3 & 0.12 & 0.46 \\
      Ori A GMC & 0.13 & 0.50 \\
      Perseus & 0.13 & 0.48 \\
      Ori B GMC & 0.11 & 0.49 \\
      Cepheus & 0.16 & 0.59 \\
      California & 0.14 & 0.51 \\
      & &\\
      \hline
    \end{tabular}
  \tablefoot{
  Data are
    from \citet{2009AetA...508L..35K} and converted into 
    \mbox{$K$-band}
    extinction parameters using a standard reddening 
    law \citep{1985ApJ...288..618R}.} 
    \end{table}