deletions | additions       diff --git a/begin_table_begin_tabular_c__.tex b/begin_table_begin_tabular_c__.tex  deleted file mode 100644  index c630852..0000000  --- a/begin_table_begin_tabular_c__.tex  +++ /dev/null 
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%\begin{table}   % \begin{tabular}{ c c c c c c c c c }  % VCA distance metric & W1T1t0.1 & W1T2t0.1 & W2T2t0.1 & W2T2t0 & W2T3t0.1 & W2T3t0 & W2T4t0.1 & W2T4t0 \\   % W1T1t0.1 & & 2.35895032377 & 3.60284821 & 3.92072276543 & 2.46116474051 & 4.18662658571 & 2.45864823628 & 4.1895110631 \\   % W1T2t0.1 & & & 2.1967058224 & 2.69722834426 & 0.469357147375 & 3.06748255822 & 0.46623044093 & 3.07162966596 \\   % W2T2t0.1 & & & & .411749410402 & 1.422848601 & 1.05249581738 & 1.42469197537 & 1.05642820665 \\   % W2T2t0 & & & & & 1.82971764726 & 0.69378454325 & 1.83137693797 & 0.697776023091 \\   % W2T3t0.1 & & & & & & 2.29708476337 & .00241706552385 & 2.30079256792 \\   % W2T3t0 & & & & & & & 2.29847122302 & 0.00366418929705 \\   % W2T4t0.1 & & & & & & & & 2.30217758285 \\   % W2T4t0 & & & & & & & & \\   % \end{tabular}   % \caption{VCA distance metrics via TurbuStat}   %\end{table}  %\section{Velocity Channel Analysis (VCA) or Velocity Coordinate SPectrum (VCS)}  %\textit{Definition:} How similar two maps are that are integrated over some velo%city channel range  %{\it Note:} Attempts to isolate how fluctuations in velocity contribute to differences between spectral cubes.  %When gas is optically thin density and velocity fluctuations are correlated; when gas is optically thick, they are uncorrelated and fluctuations are only in velocity.  %{\it References:} VCA: Lazarian \& Pogosyan 2000, 2004; Esquivel et al. 2003, Lazarian et al. 2001, Padoan et al. 2003, Stanimiric \& Lazarian 2001