ericteunis/m-thesis-documentation
1
0
Fork 0
mirror of https://gitlab.science.ru.nl/mthesis-edeboone/m.internship-documentation.git synced 2024-11-12 18:43:30 +01:00
Code Issues Projects Releases Packages Wiki Activity

STEP-UP: test run for group

Browse source
This commit is contained in:
Eric Teunis de Boone 2023-05-30 17:16:32 +02:00
parent c3299a322f
commit 97d9c209a2
1 changed files with 19 additions and 16 deletions
Show stats Download patch file Download diff file Expand all files Collapse all files

35
presentations/2023-06-01_step_up_interview/2023-STEP_UP.tex
View file

@ -44,15 +44,16 @@
\hypersetup{pdfpagemode=UseNone} % don't show bookmarks on initial view
\title[STEP-UP: Investigating interferometry with GRAND and BEACON]{
{ \large STEP-UP Interview}\\
\title[STEP-UP: Investigating interferometry with GRAND]{% and BEACON]{
{ \large STEP'UP Interview}\\
{
Investigating interferometry with\\
GRAND\footnote{Giant Radio Array for Neutrino Detection} and BEACON\footnote{Beam forming Elevated Array for COsmic Neutrinos}
GRAND\footnote{Giant Radio Array for Neutrino Detection}
% and BEACON\footnote{Beam forming Elevated Array for COsmic Neutrinos}
}
}
\date{May $10^{\text{\tiny{th}}}$, 2023}
\date{May $30^{\text{\tiny{th}}}$, 2023}
\author[E.T. de Boone]{
E.T. de Boone
@ -65,7 +66,7 @@
\begin{document}
{
\setbeamertemplate{footline}{} % no page number here
\section{Talk}
\section{Start}
\frame{ \titlepage }
}
@ -80,7 +81,7 @@
\quad {\small Specialisation: Particle and Astrophysics}\\
\quad {\small Minor: Computational Data Science}
\item Master's Internship (November 2021 - June 2023) \\
\item Master's Internship (November 2021 - July 2023) \\
\quad {\small Supervisor: Harm Schoorlemmer, IMAPP, Radboud University}\\
\quad {\small ``Enhancing Timing Accuracy in Air Shower Radio Detectors''}
\end{itemize}
@ -118,20 +119,22 @@
\begin{frame}{Advantages of Radio Interferometry}
\begin{columns}
\begin{column}{0.53\textwidth}
Interferometric Radio Observables:
\begin{column}{0.52\textwidth}
Interferometric Radio Observables:%
\begin{itemize}
\item<1-> Shower axis reconstruction%\; Relevant for $\nu$s pointing back to sources
\vspace*{2em}
\item<2-> Depth of airshower\\
$\mapsto$ composition measurement
\vspace*{1em}
\item<1-> Shower axis%\; Relevant for $\nu$s pointing back to sources
\vspace*{1em}
\item<2-> Depth of shower\\
$\mapsto$ composition measurement%
\\
\quad\;(Fe, p, $\gamma$, $\nu$)
\end{itemize}
\end{column}
\begin{column}{0.47\textwidth}
\begin{column}{0.48\textwidth}
\begin{figure}
\includegraphics[width=\textwidth]{2006.10348/fig01.png}
\hspace*{-1.5em}
\includegraphics[width=1.2\textwidth]{2006.10348/fig01.png}
\caption[caption]{
\centering
\tiny{
@ -183,7 +186,7 @@
\end{frame}
\section{Radio and Airshowers}
\begin{frame}{}
\begin{frame}{Advantages of Radio Interferometry}
\begin{columns}
\begin{column}{0.47\textwidth}
\includegraphics[width=\textwidth]{2006.10348/fig01.png}
@ -209,7 +212,7 @@
using physics band
\begin{itemize}
\item Pulsed beacon
\item<4-> Continuous (Sine)
\item<3-> Continuous (Sine)
\end{itemize}
\vspace{20pt}
\includegraphics[width=\textwidth]{beacon/array_setup_gps_transmitter_cows.png}