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\end{table}  \textbf{Observing Parameters}  Data were calibrated and analyzed using GBTIDL. Typical system temperatures were between 105 K and 120 K. Typical rms noise in the resulting calibrated spectra was 0.20 K. Non-detections and detections are listed in Tables 2 and 3, respectively. We estimate uncertainty due to flux calibration of 20%. 20\%.  In addition to single pointings, we mapped three regions (N56, N65 2 and N77 1) that displayed strong CS emission. The map sizes were 1'x1' (N56 and N77-1) and 2'x2' (N65-2), both using a Nyquist-sampling step-size of 6.12".  
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