this is for holding javascript data
Christer Watson edited sectionAnalysis__sub.tex
over 8 years ago
Commit id: a503e990fb66114819caefcd98e7fa26ff14670f
deletions | additions
diff --git a/sectionAnalysis__sub.tex b/sectionAnalysis__sub.tex
index d6f345a..8fdb253 100644
--- a/sectionAnalysis__sub.tex
+++ b/sectionAnalysis__sub.tex
...
\section{Analysis}
\subsection{CS Abundance}
In order to calculate the abundance of CS, we first must estimate the total gas column density along each line of sight. We used FIR
{\bf (60$\mu$m-600$\mu$m)} imaging taken as part of the HiGal survey. Within CASA, we measured the integrated emission in all five survey bands in regions exactly coincident with the GBT beamsize, centered at each source of CS emission. The emission was then modeled as a modified blackbody:
\begin{equation*}
B_{mod} =B_0 \frac{h^2\nu^{3+\beta}}{c^3}\frac{1}{e^{\frac{h\nu}{kT}}-1}