mirror of
https://gitlab.science.ru.nl/mthesis-edeboone/m.internship-documentation.git
synced 2024-11-22 07:03:30 +01:00
STEP-UP: test run for group
This commit is contained in:
parent
c3299a322f
commit
97d9c209a2
1 changed files with 19 additions and 16 deletions
|
@ -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}
|
||||
|
|
Loading…
Reference in a new issue