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\end{tabular}  \end{table}  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. 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 step-size of 6.12". Non-detections and detections are listed in Tables 1 2  and 2, 3,  respectively. Observations from  Hi-Galobservations  \cite{Molinari_2010}, a Herschel Space Telescope survey, of these the bubble  regions were also analyzed. Data were downloaded from the Spitzer Science Center website. Level 2 data products were used. \begin{table}  \begin{tabular}{rrr}  Name &l($^\circ$) &b($^\circ$)\\ 
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