This is template thesis structure for the Curtin University Honours dissertation in radio astronomy.
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\title{An Honours Thesis in Curtin Astronomy}
\author{Name Student Number\\Supervisor: Supervisor Name 1\\Co-Supervisor: Supervisor Name 2}
\begin{document}
\maketitle
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\begin{minipage}[H]{\textwidth}
\begin{center}
{\LARGE \textbf{Thesis Title: this is an alternative header page}}
\\[1.5cm]
{\Large
Name}\\[0.07cm]
{\large
(Curtin ID: XXXXX})\\[0.5cm]
{\Large
DATE \\[2cm]}
{\Large
Curtin University\\
%(Department)\\
International Centre for Radio Astronomy Research\\[0.5cm]
\begin{tabular}{rl}
Supervisor:& Name 1\\
Co-supervisor:& Name 1
\end{tabular}}
\end{center}
\end{minipage}
\newpage
\tableofcontents
\newpage
\begin{abstract}
An overview of my work.
\end{abstract}
\newpage
\setcounter{page}{1}
\section{Introduction}\label{sec:intro}
%The majority of studies surrounding BHs rely on examining how the presence of a BH influences the environment in which it lives.
An introduction
\section{My methodology}
\subsection{A subsection of my methodology}
A figure with label \ref{ionisation}.
\begin{figure}
\centering
\includegraphics[width=0.5\columnwidth]{ionisation}
\caption{Figure taken from \cite{1989agna.book.....O}.}
\label{ionisation}
\end{figure}
A table with label \ref{optical}.
\begin{table}
\centering
\caption{Full galaxy sample and properties.}
\begin{threeparttable}
\begin{tabular}{l c r c c r c c}
\hline\hline
I.D\tnote{1} & Name\tnote{2} & D\tnote{3} & \textit{Z}\tnote{4} & $M_*$\tnote{5} & SFR\tnote{6} & X-ray\tnote{7} & Alternate Name\\
& (SDSS) & & & & & Sources & \\
\hline
72 \tnote{8}& J024240.70$-$000047.9 & 18.6 & 8.93$\pm$0.25& 7.39 & -0.27 & $>2$ & M077\\ % 02:42:39.86 & -00:00:58.64 &
21 & J083743.48$+$513830.2 & 10.8 & 7.95$\pm$0.08 & 6.04 & -1.84 & 0 & Mrk 0094 \\ % 08:37:43.48 & 51:38:30.26 &
101 & J101624.51+375445.9 & 17.2 & 7.80$\pm$0.05 & 6.58 & -1.50 & 0 & --- \\ % 10:16:24.53 & 37:54:45.97 &
62 & J103410.15+580349.1 & 33.0 & 7.78$\pm$0.06 & 7.00 & -1.21 & 2 & Mrk 1434 \\ % 10:34:10.15 & 58:03:49.06 &
124 & J104653.98+134645.7 & 46.9& 7.92$\pm$0.09 & 6.81 & -1.15 & 0 & --- \\ % 10:46:53.99 & 13:46:45.77 &
59 & J105308.48+501704.9 & 19.2 & 7.94$\pm$0.08 & 6.04 & -2.12 & 1 & ---\\ % 10:53:10.82 & 50:16:53.21 &
178 & J111746.29+174424.6 & 21.8 & 7.90$\pm$0.09 & 6.62 & -1.44 & 2 & ---\\ % 11:17:46.30 & 17:44:24.69 &
149 & J114107.48+322537.2 & 26.6 & 7.79$\pm$0.05 & 6.04 & -1.80 & 1 & KUG 1138+327\\ % 11:41:07.49 & 32:25:37.22 &
8 & J115237.67$-$022806.3 & 15.6 & 7.84$\pm$0.09 & 6.71 & -1.45 & 2 & --- \\ % 11:52:37.68 & -02:28:06.39 &
147 & J121749.30+375155.5 & 2.7 & 7.92$\pm$0.09 & 6.02 & -2.59 & 0 & --- \\
\hline
\hline
\end{tabular}
\end{threeparttable}
\label{optical}
\end{table}
An example equation
\begin{equation}
\psi(M_{\odot} \text{ yr}^{-1})=
\begin{cases}
5.52\times10^{-22}L_{1.4\text{GHz}}, & L>L_c\\
\frac{5.52\times10^{-22}}{0.1+0.9(L/L_c)^{0.3}}L_{1.4\text{GHz}}, & L\leq L_c
\end{cases}
\label{eq:sfr-Lr}
\end{equation}
\section{Conclusion and Future Work}\label{sec:conlusion}
\begin{appendix}
\section{Appendix}\label{sec:app}
This is where we put appended information.
\end{appendix}
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