Moved old dir to subdirectory 2018-19

.gitignore

@@ -0,0 +1,9 @@
+# LaTeX files
+*.pdf
+*.aux
+*.log
+*.dvi
+*.toc
+*.out
+*.snm
+*.nav

2018-19/presentation/presentation.tex

@@ -45,6 +45,10 @@
 \end{frame}
 
 \section{ Neutrino Astronomy }
+\begin{frame}{ Why Neutrino Astronomy }
+	\includegraphics[width=\textwidth]{images/icecube-3-fig9-multimessenger-spectrum.png}
+\end{frame}
+
 \begin{frame}{ Neutrino Astronomy: History }
 	\begin{itemize}
 		\item First observation of neutrino in 1956
@@ -53,7 +57,6 @@
 
 		\item Antarctic Muon and Neutrino Detector Array (, now part of IceCube)
 	\end{itemize}
-
 \end{frame}
 \begin{frame}{ Neutrino Astronomy: Basics }
 			\begin{itemize}
@@ -65,6 +68,7 @@
 				\begin{column}{0.9\textwidth}
 					\begin{figure}[hbtp]
 						\centering
+						\includegraphics[width=\textwidth]{images/icecube-3-fig1-initial-outline.png}
 						\includegraphics[width=0.3\textwidth]{images/prinicipal_idea_neutrino_telescope.png}
 					\caption{\small Cherenkov cone propagating through the IceCube Detector}
 					\end{figure}
@@ -82,7 +86,6 @@
 	\end{itemize}
 \end{frame}
 
-
 \section{IceCube observatory}
 \begin{frame}{IceCube observatory}
 	\includegraphics[width=0.9\textwidth]{images/icecube-array-fancy.png} 
@@ -95,11 +98,12 @@
 		\item IceCube: the main detector for $E_\nu > 100$ GeV
 		\item DeepCore: sensitive for $E_\nu \raise.17ex\hbox{$\scriptstyle\sim$} 10$ GeV due to tight spacing
 	\end{itemize}
+	\includegraphics[width=\textwidth]{images/icecube-3-fig2-architecture-and-dom.png}
 \end{frame}
 
-\begin{frame}{IceCube observatory: Digital Optical Module}
-	\includegraphics[width=\textwidth]{images/icecube-4-Aartsen_2017_DOM.pdf}
-\end{frame}
+%\begin{frame}{IceCube observatory: Digital Optical Module}
+%	\includegraphics[width=\textwidth]{images/icecube-4-Aartsen_2017_DOM.pdf}
+%\end{frame}
 
 
 \subsection{Event Detection and Background}
@@ -110,7 +114,7 @@
 	\begin{figure}[hbtp]
 		\centering
 		\includegraphics[width=0.75\textwidth]{images/icecube_veto_regions.png}
-		\caption{\ref{}}
+		%\caption{\ref{}}
 	\end{figure}
 	
 \end{frame}
@@ -143,18 +147,21 @@
 		\begin{column}{.5\textwidth}
 			\begin{block}{Tracklike}
 				\begin{itemize}
-					\item d
+					\item Mostly CC of $\nu_\mu$
+					\item Through-going Muons
 				\end{itemize}
 			\end{block}
 		\end{column}
 		\begin{column}{.5\textwidth}
 			\begin{block}{Showerlike}
 				\begin{itemize}
-					\item d
+					\item NC of all $\nu$ flavours
+					\item CC of $\nu_e$ (and $\nu_\tau$ if $E \lesssim 100 TeV$)
 				\end{itemize}
 			\end{block}
 		\end{column}
 	\end{columns}
+	both: Glashow resonance of $\overline{\nu_e}$ at $E \sim 6.3 PeV$ on $e^{-}$ to $W$
 
 	\begin{columns}[t]
 		\begin{column}{.5\textwidth}
@@ -168,7 +175,6 @@
 			\end{block}
 		\end{column}
 	\end{columns}
-
 	%\begin{figure}
 	%	\includegraphics[width=0.5\textwidth]{images/charged_and_neutral_neutrino_interactions.pdf}
 	%	\caption{From \url{http://inspirehep.net/record/1236362/files/TwoDiagrams.png}}
@@ -176,7 +182,7 @@
 
 \end{frame}
 
-\begin{frame}{Background}
+\begin{frame}{Background vs Signals}
 	\begin{itemize}
 		\item 2500 to 2900 events per second
 		\item $\sim 10^{5}$ atmospheric neutrinos vs. $\lesssim 10^3$ cosmic neutrinos per year 
@@ -187,11 +193,14 @@
 
 \section{High Energy Extraterrestrial Neutrinos}
 \begin{frame}{High Energy Extraterrestrial Neutrinos}
+	\small{ 28 neutrino candidate events, ranging from 30 to $1200 TeV$ in a 2-year dataset }
+	\includegraphics[width=\textwidth]{images/icecube-3-table1-28events.png}
+\end{frame}
+\begin{frame}{High Energy Extraterrestrial Neutrinos}
+	\includegraphics[width=\textwidth]{images/icecube-3-fig3-vertical-deposition.png}
 \end{frame}
 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
 %	Appendix
 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
-\appendix
-\bibliography{presentation}
 
 \end{document}