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Christer Watson edited Results.tex
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Eighteen sources displayed emission greater than 3$\sigma$. A typical spectrum is shown in Figure 1. Emission lines were fit using the standard Gaussian fitting routine in GBTIDL. Fitting parameters are listed in Table \ref{fitting}.
\begin{table}[]
\caption{Gaussian fitting parameters for CS detections.}
\label{fitting}
\caption{Gaussian fitting parameters for CS detections.}
\begin{tabular}{lllllll}
Name &l ($^\circ$) &b ($^\circ$) &T$_A^*$ (K) &Vel$_{LSR}$ (km/s) &$\Delta$v (km/s) &N$_{CS}$ (x10$^{14}$ cm$^{-2}$)\\
\hline