diff --git a/accelerator/report/report.tex b/accelerator/report/report.tex
index d2dbf2e..b4e3878 100644
--- a/accelerator/report/report.tex
+++ b/accelerator/report/report.tex
@@ -11,7 +11,7 @@
 \usepackage{caption}
 \usepackage[export]{adjustbox}
 \usepackage{float}
-
+\usepackage{gensymb}
 
 \bibliography{/home/caes/wmu/phy-4660/adv_lab.bib}
 
@@ -44,17 +44,19 @@
 
     \begin{figure}
         \center
-        \includegraphics[width=6in]{../abundances.png}
+        \includegraphics[width=4.5in]{../abundances.png}
         \caption{Relative elemental abundances in the sun's photosphere. Lithium and fluorine are much less abundant than their neighbour elements. It is thought this is due to large probability cross-sections for a proton collision with these nuclei. \cite{Carroll&Ostlie}}
     \end{figure}
 
 \section{Nuclear Reactions and Detection Plan}
     \label{sec:beamreactions}
     
+    We expect three reactions to occur 
+
     \begin{figure}
         \center
         \includegraphics[width=4.5in]{../collision.png}
-        \caption{In general, an incident particle collides with a target nucleus, resulting in an emitted particle and a residual nucleus. The backscattering experiments in this study have $\theta = 149\pm0.05\degree$ \cite{ADVLABACCEL}}
+        \caption{In general, an incident particle collides with a target nucleus, resulting in an emitted particle and a residual nucleus. The backscattering experiments in this study have $\theta = 149\pm0.05\degree$ \cite{ADVLABACCEL}.}
     \end{figure}