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Christer Watson edited Results.tex
over 9 years ago
Commit id: d524c82070c9f92ab66971870b659f8855a74681
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diff --git a/Results.tex b/Results.tex
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Z_{rot} &=& .8556\; T_{ex}-0.10\\
F(T) &=& \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 (citation?). The partition
functio (Z$_{rot}$). function (Z$_{rot}$) is a linear fit to JPL data between T=NN-MM K. 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.}