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\begin{document}
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\begin{center}
    \includegraphics[width=8cm,height=8cm,keepaspectratio]{FIG/UZH.png}
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   	\vspace{2cm}
	\Huge
	\textbf{Title}
	
	\vspace{2cm}
	\huge
	Master Thesis in Physics
	
	\vspace{2cm}	
	\Large
	\textbf{Author}
	
	\vspace{3cm}
	\normalsize	
	Supervised by \\
	\Large
	Prof. Dr. Name\\
	Ph.D. Name\\
	
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	\large
	\today
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\begin{abstract}
XXX
\end{abstract}
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\begin{center}
   \textbf{Acknowledgements}
   \begin{quotation}
   XXX
   \end{quotation}
\end{center}
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\tableofcontents
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\listoffigures
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\newpage
\section{Introduction}
\subsection{Motivation}
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\subsection{Subsection title}
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\subsubsection{Subsubsection title}
xxx
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\newpage
\section{Section title}\label{sec:sectiontitle1}
In section \ref{sec:sectiontitle1}...
\subsection{Subsection title}
\subsubsection{Subsubsection title}
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\newpage
\section{Examples of scientific writing}\label{sec:sectiontitle2}
In section \ref{sec:sectiontitle2}, examples of scientific writing are provided.

\subsection{Typefaces for symbols in scientific manuscripts}
The following rules are taken from International Organization for Standardization (ISO) International Standard ISO 80000-1:2022 (former ISO 31).  Technical publications should be typed or typeset in either italic or roman type, as follows:
\begin{itemize}
\item symbols for physical quantities and variables, universal constants and running indices -- italic;
\item symbols for units -- roman;
\item symbols for descriptive terms -- roman.
\end{itemize}
\noindent The following sections give examples of the proper typefaces for these categories.

\subsubsection{Universal constants —- italic}
\[
\begin{array}{ll}
h  & \text{the Planck constant} \\
F  & \text{the Faraday constant} \\
\end{array}
\]

\subsubsection{Units -- roman}
\[
\begin{array}{lllll}
\text{m}  & (\text{meter})      & ~ & \text{g}     & (\text{gramm}) \\
\text{cm} & (\text{centimeter}) & ~ & \upmu\text{g} & (\text{microgramm}) \\
\end{array}
\]

\subsubsection{Quantities and variables —- italic}
Symbols for quantities are italic, as are symbols for functions in general, for example, $f(x)$:
\[
\begin{array}{lllll}
t = 1~{\rm s}   & (t \text{ time, s second})        & ~ & T = 297~{\rm K}        & (T \text{ temperature, K Kelvin}) \\
r = 12~{\rm cm} & (r \text{ radius, cm centimeter}) & ~ & \lambda = 633~{\rm nm} & (\lambda \text{ wavelength, nm nanometer}) \\
\end{array}
\]

\subsubsection{Subscripts}
\noindent The following principles for the printing of subscripts apply.\\
\noindent -- A subscript that represents a physical quantity or a mathematical variable, such as a running number, is printed in italic type.\\
\noindent -- Other subscripts, such as those representing words or fixed numbers, are printed in roman type.\\
\[
\begin{array}{lllll}
\text{\bf Italic subscripts} & ~                      & ~ & \text{\bf Roman subscripts} & ~\\
C_p                 & (p: \text{ pressure})           & ~ & C_{\rm g}                   & \text{(g: gas)} \\
c_i                 & (i: \text{ running number})     & ~ & c_3                         & \text{(3: third)} \\
\sum_n a_n \omega_n & (n: \text{ running number})     & ~ & g_{\rm n}                   & \text{(n: normal)} \\
F_x                 & (x:~x \text{- component})       & ~ & \mu_{\rm r}                 & \text{(r: relative)} \\
g_{ik}              & (i, k: \text{ running numbers}) & ~ & S_{\rm m}                   & \text{(m: molar)} \\
I_{\lambda}         & (\lambda: \text{ wavelength})   & ~ & N_{\rm A}                   & \text{(A: Avogadro)} \\
\end{array}
\]

\subsubsection{Chemical elements -- roman}
\[
\begin{array}{llllllll}
\text{Ar} & (\text{argon}) & ~~~~~~~~ & \text{B} & (\text{boron}) & ~~~~~~~~ & \text{C} & (\text{carbon})\\
\end{array}
\]

\subsubsection{Vectors, tensors and matrices -- boldface italic}
Symbols for vectors are boldface italic, symbols for tensors are sans-serif bold italic, and symbols for matrices are boldface italic:
\[
\begin{array}{llllllll}
\boldsymbol{A}\cdot \boldsymbol{B} = \boldsymbol{C}  & \text{(vectors)} &  ~~~~  & \boldsymbol{T} & \text{(tensors)} & ~~~~ & \boldsymbol{A} =
\left(
\begin{array}{cc}
a_{11} & a_{12}\\
a_{21} & a_{22}\\
\end{array}
\right) & \text{(matrices)}\\
\end{array}
\]

\subsubsection{Mathematical constants, functions and operators}
\noindent Symbols representing mathematical constants that never change (for example, $\uppi$) and symbols representing explicitly defined functions or well defined operators (for example, $\Gamma (x)$ or div) - roman:
\[
\begin{array}{lllllll}
\exp{x} & ~~~~~~~~ & \sin{x} & ~~~~~~~~ & \ln{x} & ~~~~~~~~ & {\rm d} x/ {\rm d} t\\
\end{array}
\]
\[
F(q_x, q_y) = \iint f(x, y) \exp\left[(-i(q_x x + q_y y)\right] {\rm d}x {\rm d}y.
\]
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\subsection{Examples of numbered equations}
\noindent Equation (\ref{Eq:01}) shows that ...
\beq\label{Eq:01}
M_Z = (57.9 \pm 7.03) M_{\oplus} \left(\frac{M}{M_J}\right)^{(0.61 \pm 0.08)},
\eeq
\beq\label{Eq:02}
E = mc^2.
\eeq
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\subsection{Example of table}
\begin{table}[H]
    \centering
    \begin{tabular}{|c||c|c|c|c|c|}
        \hline
         $n$ & 0 & 1 & 1.5 & 2 & 2.5\\
         \hline
         $\tau_{\rm ff}$     & $\propto M^0$      & $\propto M^{1/4}$ & $\propto M^{1/2}$ & $\propto M$   & $\propto M^{5/2}$\\
         $\tau_{\rm expl}$   & $\propto M^0$      & $\propto M^{1/4}$ & $\propto M^{1/2}$ & $\propto M$   & $\propto M^{5/2}$\\
         $\tau_{\rm Alfven}$ & $\propto M^{1/3}$  & $\propto M^{1/4}$ & $\propto M^{1/6}$ & $\propto M^0$ & $\propto M^{-1/2}$\\
         $\tau_{\rm shear}$  & $\propto M^{-1/3}$ & $\propto M^{0}$   & $\propto M^{1/3}$ & $\propto M$   & $\propto M^{3}$\\
         \hline
    \end{tabular}
    \captionsetup{width = 0.8\textwidth}
    \caption[Short Caption Table 1]{Relation of the timescales with planetary mass for different density power-law indexes.}
    \label{Table1}
\end{table}
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\newpage
\subsection{Examples of figures}
\subsubsection{Scalebars and intensity bars}
Figure \ref{fig:scalebars} illustrates how every image of the sample should have a scalebar and an intensity bar.
\begin{figure}[H]
 \centering
\includegraphics[width = 0.6\textwidth]{FIG/01_Chen2021Science.png}
 \captionsetup{width = 0.8\textwidth}
 \caption[Short Caption Figure 1]{Multislice electron ptychographic reconstruction of PrScO$_3$. The figure is reprinted from Chen at al. \cite{Chen:2021}.}
 \label{fig:scalebars}
\end{figure}

\newpage
\subsubsection{Figure with multiple panels}
\begin{figure}[H]
     \centering
     \begin{subfigure}[b]{0.495\linewidth}
         \centering
         \includegraphics[width=\linewidth]{FIG/02a_cormass.png}
         \caption{\textbf{free-fall timescale}}
         \label{fig:ratio3}
     \end{subfigure}
     \begin{subfigure}[b]{0.495\linewidth}
         \centering
         \includegraphics[width=\linewidth]{FIG/02b_cormass.png}
         \caption{\textbf{expansion timescale}}
         \label{fig:ratio4}
     \end{subfigure}
     \begin{subfigure}[b]{0.495\linewidth}
         \centering
         \includegraphics[width=\linewidth]{FIG/02c_cormass.png}
         \caption{\textbf{Alfv\'{e}n timescale}}
         \label{fig:ratio5}
     \end{subfigure}
     \begin{subfigure}[b]{0.495\linewidth}
         \centering
         \includegraphics[width=\linewidth]{FIG/02d_cormass.png}
         \caption{\textbf{shear timescale}}
         \label{fig:ratio6}
     \end{subfigure}
     \captionsetup{width = 0.8\textwidth}
     \caption[Short Caption Figure 2]{Relation of the 13 MHD clumps bound mass with (a) the free-fall timescale, (b) the expansion timescale, (c) the Alfv\'{e}n timescale, and (d) the shear timescale. The black dashed and dotted lines correspond to the predicted relation for power-law index $n = 1.5$ and $n = 2$.}
\end{figure}
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\newpage
\section{Section title}\label{sec:sectiontitle3}
In section \ref{sec:sectiontitle3}...
\subsection{Subsection title}
\subsubsection{Subsubsection title}
Footnote\footnote{XXX}\\
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\newpage
\section{Conclusions $\&$ Outlook}
\subsection*{Conclusions}
\subsection*{Outlook}
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\newpage
\section{Appendix}
xxx
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