deletions | additions       diff --git a/Results.tex b/Results.tex  index 2343b8d..704779a 100644  --- a/Results.tex  +++ b/Results.tex 
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g_K= g_I &=& 1\\  \mu^2_{el} S &=& 3.8 Debye^2\\  Z_{rot} &=& .8556\; T_{ex}-0.10\\  F(T) &=& \frac{1}{e^{h\nu/k_BT}-1}\\ \frac{1}{e^{h\nu/k_BT}-1}.\\  \end{eqnarray}  The dipole moment line strength ($\mu^2_{el}$ S) is taken from the JPL spectral line catalog (citation?), as is the equation for the partition functio (Z$_{rot}$). T$_{bg}$ was taken to be the cosmic microwave background temperature, 2.725 K.  \begin{table}[]  \label{fitting}  \caption{Gaussian fitting parameters for CS detections.}