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\title[]{}
\date{March $13^{\text{\tiny{th}}}$, 2023}
\author{E.T. de Boone}

\begin{document}
\frame{\titlepage}

% Context
%%%%%%%%%
\begin{frame}{Airshowers from Ultra High Energy particles}
	Processes in the cosmos can produce UHE particles
\end{frame}

\begin{frame}{Radio signals and Airshowers}
	Airshower split into EM, Muon and Hadron
	\begin{columns}
		\begin{column}{0.4\textwidth}
		\end{column}
		\begin{column}{0.6\textwidth}
			\begin{figure}
				\centering
				\includegraphics[width=\textwidth]{1607.08781/fig02a_airshower+detectors.png}
				\caption{
					\cite{Schroder:2016hrv}
				}
			\end{figure}
		\end{column}
	\end{columns}
\end{frame}

\begin{frame}{Radio Interferometry}
	\begin{columns}
		\begin{column}{0.4\textwidth}
	   		\includegraphics[width=\textwidth]{Schematic_RIT_extracted.png}
		\end{column}
		\begin{column}{0.5\textwidth}
	   	\begin{figure}
	   		\includegraphics[width=\textwidth]{2006.10348/fig01.png}
	   		\caption{
	   			\cite{Schoorlemmer:2020low}
	   		}
	   	\end{figure}
		\end{column}
	\end{columns}

\end{frame}

% My Internship
%%%%%%%%%%%%%%%
\begin{frame}{Timing Constraint for Radio Interferometry}
	RI requires $\sigma_t < 1 \mathrm{ns}$\\
	GPS clock accuracy in current experiments not enough, with $\sigma_t \sim 8\mathrm{ns}$\\

	\vskip 1em
	$\mapsto$ my internship
	\\
	hardware delays\\
	beacon simulations
\end{frame}


% Towards GRAND
%%%%%%%%%%%%%%%%%%%%
\begin{frame}{Advantages of Radio Interferometry}
	trace airshower longitudinal development\\
	lower snr threshold
\end{frame}

\begin{frame}{Physics Improvement of Radio Interferometry}
	composition measurement\\
	\vskip 1em

	direction reconstruction improved\\
	relevance for $\nu$s pointing back to sources
\end{frame}


%%%%%%%%%%%%%%%
% Backup slides
%%%%%%%%%%%%%%%
\appendix
\frame{Back-up slides}


%%%%%%%%%%%%%%
% Bibliography
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\section*{References}
\begin{frame}{References}
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\end{document}

