deletions | additions       diff --git a/Data_were_calibrated.tex b/Data_were_calibrated.tex  index 33d8cc7..5ff9791 100644  --- a/Data_were_calibrated.tex  +++ b/Data_were_calibrated.tex 
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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\%.  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$\arcmin$x1$\arcmin$ 1\arcmin x1 \arcmin  (N56 and N77-1) and 2$\arcmin$x2$\arcmin$ 2\arcmin x2\arcmin  (N65-2), both using a Nyquist-sampling step-size of 6.12$\arcsec$. 6.12\arcsec.  Observations from Hi-Gal \citep{Molinari2010}, a Herschel Space Telescope imaging survey of the Galactic plane, including all the sources observed in this study, in wavelengths between 60 $\mu$m and 600 $\mu$m. Data were downloaded from the Spitzer Science Center website. Level 2 data products were used, which have been fully calibrated.