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Christer Watson edited Data_were_calibrated.tex
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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 (N56 and N77-1) and 2\arcmin x2\arcmin (N65-2), both using a Nyquist-sampling step-size of 6.12\arcsec.
{\bf Observations
were used from
the Hi-Gal
\citep{Molinari2010}, \citep{Molinari2010} project, a Herschel Space Telescope imaging survey of the Galactic
plane, including plane. This survey observed all the sources
observed in this
study, in study at wavelengths between 60 $\mu$m and 600
$\mu$m. $\mu$m}. Data were downloaded from the Spitzer Science Center website. Level 2 data products were used, which have been fully calibrated.