ddd/bachelor-prep-presentation
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Clean up formatting

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prescientmoon 2025-03-21 12:55:41 +01:00
parent 909e0b03db
commit ea3caa20e7
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SSH key fingerprint: SHA256:UUF9JT2s8Xfyv76b8ZuVL7XrmimH4o49p4b+iexbVH4
2 changed files with 64 additions and 67 deletions

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@ -59,10 +59,8 @@ code-for-last-col = \color{blue}
\setbeamercolor{block title}{fg=white, bg=purple!50!black} \setbeamercolor{block title}{fg=white, bg=purple!50!black}
\setbeamercolor{block body}{fg=black, bg=pink!20} \setbeamercolor{block body}{fg=black, bg=pink!20}
\setbeamercolor{titlebox}{fg=black,bg=white} \setbeamercolor{titlebox}{fg=black,bg=white}
\begin{document} \begin{document}
\section{Introduction} \section{Introduction}
@ -70,7 +68,7 @@ code-for-last-col = \color{blue}
{ {
\usebackgroundtemplate{\includegraphics[height=\paperheight]{cmb.png}} \usebackgroundtemplate{\includegraphics[height=\paperheight]{cmb.png}}
\begin{frame} \begin{frame}
\begin{beamercolorbox}[center]{titlebox}% \begin{beamercolorbox}[center]{titlebox}
\titlepage \titlepage
\end{beamercolorbox} \end{beamercolorbox}
\end{frame} \end{frame}
@ -79,8 +77,7 @@ code-for-last-col = \color{blue}
\include{prerequisites} \include{prerequisites}
\include{isospectral} \include{isospectral}
\section{CMB Anisotropy of Spherical Spaces \section{CMB Anisotropy of Spherical Spaces}
}
\begin{frame}[fragile]{Homogeneous Spherical Spaces} \begin{frame}[fragile]{Homogeneous Spherical Spaces}
\begin{itemize} \begin{itemize}
@ -149,7 +146,7 @@ code-for-last-col = \color{blue}
\section{Test for anisotropy in the mean of the CMB temperature fluctuation in spherical harmonic space} \section{Test for anisotropy in the mean of the CMB temperature fluctuation in spherical harmonic space}
\begin{frame}{Statistical Isotropy and Hypothesis} \begin{frame}{Statistical Isotropy and Hypothesis}
\small \small
\textbf{Theoretical Expectation:}\\ \textbf{Theoretical Expectation:}\\
From the perspective of an Earth-based observer, we can view the CMB as a function defined on the celestial sphere $\mathbb{S}^2$.\\ From the perspective of an Earth-based observer, we can view the CMB as a function defined on the celestial sphere $\mathbb{S}^2$.\\
\begin{itemize} \begin{itemize}
@ -169,7 +166,7 @@ code-for-last-col = \color{blue}
\end{frame} \end{frame}
\begin{frame}{Methodology: Sky Masking and the Test Statistic} \begin{frame}{Methodology: Sky Masking and the Test Statistic}
\small \small
\textbf{Challenges in Real Observations:} \textbf{Challenges in Real Observations:}
\begin{itemize} \begin{itemize}
\item We cannot observe the full CMB sky due to foreground contamination. \item We cannot observe the full CMB sky due to foreground contamination.
@ -193,7 +190,7 @@ code-for-last-col = \color{blue}
\begin{frame}{Results and Interpretation} \begin{frame}{Results and Interpretation}
\small \small
\begin{columns} \begin{columns}
\column{0.5\textwidth} \column{0.5\textwidth}
\begin{figure} \begin{figure}