\begin{table}%t2
        \caption {Lorentzian fit values for the D and G~bands that 
        correspond to line position, FWHM, and intensity ratio $I$(D)/$I$(G).
        \label{loglorentz}}
\par
%\centerline
 {        \begin{tabular}{cccccc}
        \hline
        \hline
 IDP & D line position & G line position & D line FWHM & G line FWHM & $I$(D)/$I$(G)\\% & A(D)/(A(D)+A(G))    \\
        & (cm$^{-1}$)  & (cm$^{-1}$)     & (cm$^{-1}$) & (cm$^{-1}$) &\\          % &  \\
        \hline  
        F1\_1 (Stardust)                 & 1365 & 1562 & 322 & 146 & 0.73\\% & 0.60 \\
        F1\_2 (Stardust)                 & 1350 & 1595 & 248 &  86 & 1.06\\% & 0.74 \\ 
        K2 (IDP)                         & 1365 & 1570 & 256 & 130 & 0.90\\% & 0.62 \\
        N (IDP)                          & 1365 & 1585 & 256 & 100 & 1.17\\% &0.74 \\     
        11 IDPs (average)$^1$ & 1362 (1345--1393) & 1584 (1562--1594) & 296 (141--476) & 104 (72--159) & 1.02 (0.66--1.39)\\ 
        \hline
        \end{tabular}}
\par
\smallskip
$^1$ Average values of Raman parameters corresponding to 11 IDPs (Wopenka 1988), reported by 
Ferini et~al. (\cite{Ferini04}). 
\end{table}