diff --git a/report_thesis/src/index.tex b/report_thesis/src/index.tex
index 5d175998..fdd88157 100644
--- a/report_thesis/src/index.tex
+++ b/report_thesis/src/index.tex
@@ -14,8 +14,8 @@ \subsubsection*{Acknowledgements:}
 \input{sections/related_work.tex}
 \input{sections/problem_definition.tex}
 \input{sections/background/index.tex}
-\input{sections/proposed_approach/proposed_approach.tex}
 \input{sections/baseline_replica.tex}
+\input{sections/proposed_approach/proposed_approach.tex}
 \input{sections/methodology.tex}
 \input{sections/experiment_design/index.tex}
 \input{sections/results/results.tex}
diff --git a/report_thesis/src/sections/baseline_replica.tex b/report_thesis/src/sections/baseline_replica.tex
index fdaa0b4e..3b7bab71 100644
--- a/report_thesis/src/sections/baseline_replica.tex
+++ b/report_thesis/src/sections/baseline_replica.tex
@@ -1,4 +1,4 @@
-\subsection{Baseline \& Replica}\label{sec:baseline_replica}
+\section{Baseline \& Replica}\label{sec:baseline_replica}
 For analyzing Martian geological samples, the \gls{chemcam} team currently uses the \gls{moc} model~\cite{cleggRecalibrationMarsScience2017}.
 This model integrates \gls{pls} and \gls{ica} to predict the composition of major oxides.