diff --git a/Physics_Thesis_Template/content/chapter-conclusion.tex b/Physics_Thesis_Template/content/chapter-conclusion.tex index c60e4e8..3b0d235 100644 --- a/Physics_Thesis_Template/content/chapter-conclusion.tex +++ b/Physics_Thesis_Template/content/chapter-conclusion.tex @@ -1,3 +1,3 @@ -\chapter{Conclusion and Outlook} -\label{sec:conclusion} +\chapter{Conclusion and Outlook \label{sec:conclusion}} + diff --git a/Physics_Thesis_Template/content/chapter-results.tex b/Physics_Thesis_Template/content/chapter-results.tex index d0722fd..a374870 100644 --- a/Physics_Thesis_Template/content/chapter-results.tex +++ b/Physics_Thesis_Template/content/chapter-results.tex @@ -13,14 +13,13 @@ Looking at the same data, just with 30 instead of 10 bins (figure \ref{fig:M-Fla \begin{figure}[pt!] \centering - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/M/M-Flarecount-10_Bins.png} \caption{10 bins} \label{fig:M-Flarecount-10_Bins} \end{subfigure} - \vspace{1em} - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/M/M-Flarecount-30_Bins.png} \caption{30 bins} @@ -42,32 +41,70 @@ Increasing the bin count to 30 (see figure \ref{fig:M-Flarecount-30_Bins_1.5_pea \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/M/M_minFlarePeak_1.25-Flarecount-10_Bins.png} - \caption{Minimum flare peak 1.25, 10 bins} + \caption{10 bins} \label{fig:M-Flarecount-10_Bins_1.25_peak} \end{subfigure} - \hfill \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/M/M_minFlarePeak_1.25-Flarecount-30_Bins.png} - \caption{Minimum flare peak 1.25, 30 bins} + \caption{30 bins} \label{fig:M-Flarecount-30_Bins_1.25_peak} \end{subfigure} - \vspace{1em} + \caption{Histograms showing the amount of flares with a normalized peak of greater than 1.25 per phase for all 144 M dwarfs used in this study. The x-axis represents the normalized phase of the folded lightcurves. There are 10 (\subref{fig:M-Flarecount-10_Bins_1.25_peak}) /30 (\subref{fig:M-Flarecount-30_Bins_1.25_peak}) bins of the phase, showing the number of flares per bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase (sine curve), with the maximum at phase $0 \pi$/$2 \pi$ and the minimum at phase $1 \pi$.} + \label{fig:M-Flarecount-peaks_1.25_peak} +\end{figure} +\begin{figure}[pt!] + \centering \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/M/M_minFlarePeak_1.5-Flarecount-10_Bins.png} - \caption{Minimum flare peak 1.5, 10 bins} + \caption{10 bins} \label{fig:M-Flarecount-10_Bins_1.5_peak} \end{subfigure} - \hfill \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/M/M_minFlarePeak_1.5-Flarecount-30_Bins.png} - \caption{Minimum flare peak 1.5, 30 bins} + \caption{30 bins} \label{fig:M-Flarecount-30_Bins_1.5_peak} \end{subfigure} - \caption{Histograms showing the amount of flares with a normalized peak of greater than 1.25 (\subref{fig:M-Flarecount-10_Bins_1.25_peak} and \subref{fig:M-Flarecount-30_Bins_1.25_peak})/1.5 (\subref{fig:M-Flarecount-10_Bins_1.5_peak} and \subref{fig:M-Flarecount-30_Bins_1.5_peak}) per phase for all 144 M dwarfs used in this study. The x-axis represents the normalized phase of the folded lightcurves. There are 10 (\subref{fig:M-Flarecount-10_Bins_1.25_peak} and \subref{fig:M-Flarecount-10_Bins_1.5_peak})/30 (\subref{fig:M-Flarecount-30_Bins_1.25_peak} and \subref{fig:M-Flarecount-30_Bins_1.5_peak}) bins of the phase, showing the number of flares per bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase (sine curve), with the maximum at phase $0 \pi$/$2 \pi$ and the minimum at phase $1 \pi$.} - \label{fig:M-Flarecount-peaks} + \caption{Histograms showing the amount of flares with a normalized peak of greater than 1.5 per phase for all 144 M dwarfs used in this study. The x-axis represents the normalized phase of the folded lightcurves. There are 10 (\subref{fig:M-Flarecount-10_Bins_1.5_peak})/30 (\subref{fig:M-Flarecount-30_Bins_1.5_peak}) bins of the phase, showing the number of flares per bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase (sine curve), with the maximum at phase $0 \pi$/$2 \pi$ and the minimum at phase $1 \pi$.} + \label{fig:M-Flarecount-peaks_1.5_peak} +\end{figure} + +\begin{figure}[pt!] + \centering + \begin{subfigure}[b]{.49\textwidth} + \centering + \includegraphics[width=\linewidth]{plots/sine/M/M_maxFlarePeak_1.01-Flarecount-10_Bins.png} + \caption{10 bins} + \label{fig:M-Flarecount-10_Bins_1.01_maxpeak} + \end{subfigure} + \begin{subfigure}[b]{.49\textwidth} + \centering + \includegraphics[width=\linewidth]{plots/sine/M/M_maxFlarePeak_1.01-Flarecount-30_Bins.png} + \caption{30 bins} + \label{fig:M-Flarecount-30_Bins_1.01_maxpeak} + \end{subfigure} + \caption{Histograms showing the amount of flares with a normalized peak of less than 1.01 per phase for all 144 M dwarfs used in this study. The x-axis represents the normalized phase of the folded lightcurves. There are 10 (\subref{fig:M-Flarecount-10_Bins_1.01_maxpeak})/30 (\subref{fig:M-Flarecount-30_Bins_1.01_maxpeak}) bins of the phase, showing the number of flares per bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase (sine curve), with the maximum at phase $0 \pi$/$2 \pi$ and the minimum at phase $1 \pi$.} + \label{fig:M-Flarecount-peaks_1.01_maxpeak} +\end{figure} + +\begin{figure}[pt!] + \centering + \begin{subfigure}[b]{.49\textwidth} + \centering + \includegraphics[width=\linewidth]{plots/sine/M/M_maxFlarePeak_1.05-Flarecount-10_Bins.png} + \caption{10 bins} + \label{fig:M-Flarecount-10_Bins_1.05_maxpeak} + \end{subfigure} + \begin{subfigure}[b]{.49\textwidth} + \centering + \includegraphics[width=\linewidth]{plots/sine/M/M_maxFlarePeak_1.05-Flarecount-30_Bins.png} + \caption{30 bins} + \label{fig:M-Flarecount-30_Bins_1.05_maxpeak} + \end{subfigure} + \caption{Histograms showing the amount of flares with a normalized peak of less than 1.05 per phase for all 144 M dwarfs used in this study. The x-axis represents the normalized phase of the folded lightcurves. There are 10 (\subref{fig:M-Flarecount-10_Bins_1.05_maxpeak})/30 (\subref{fig:M-Flarecount-30_Bins_1.05_maxpeak}) bins of the phase, showing the number of flares per bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase (sine curve), with the maximum at phase $0 \pi$/$2 \pi$ and the minimum at phase $1 \pi$.} + \label{fig:M-Flarecount-peaks_1.05_maxpeak} \end{figure} \FloatBarrier @@ -79,14 +116,13 @@ Looking at the same dataset with 30 bins for the histogram (figure \ref{fig:K-Fl \begin{figure}[pt!] \centering - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/K/K-Flarecount-10_Bins.png} \caption{10 bins} \label{fig:K-Flarecount-10_Bins} \end{subfigure} - \vspace{1em} - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/K/K-Flarecount-30_Bins.png} \caption{30 bins} @@ -96,6 +132,60 @@ Looking at the same dataset with 30 bins for the histogram (figure \ref{fig:K-Fl \label{fig:K-Flarecount} \end{figure} +\begin{figure}[pt!] + \centering + \begin{subfigure}[b]{.49\textwidth} + \centering + \includegraphics[width=\linewidth]{plots/sine/K/K_minFlarePeak_1.05-Flarecount-10_Bins.png} + \caption{10 bins} + \label{fig:K-Flarecount-10_Bins_1.05_peak} + \end{subfigure} + \begin{subfigure}[b]{.49\textwidth} + \centering + \includegraphics[width=\linewidth]{plots/sine/K/K_minFlarePeak_1.05-Flarecount-30_Bins.png} + \caption{30 bins} + \label{fig:K-Flarecount-30_Bins_1.05_peak} + \end{subfigure} + \caption{Histograms showing the amount of flares with a normalized peak of greater than 1.05 per phase for all 37 K dwarfs used in this study. The x-axis represents the normalized phase of the folded lightcurves. There are 10 (\subref{fig:K-Flarecount-10_Bins_1.05_peak})/30 (\subref{fig:K-Flarecount-30_Bins_1.05_peak}) bins of the phase, showing the number of flares per bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase (sine curve), with the maximum at phase $0 \pi$/$2 \pi$ and the minimum at phase $1 \pi$.} + \label{fig:K-Flarecount-peaks_1.5_peak} +\end{figure} + +\begin{figure}[pt!] + \centering + \begin{subfigure}[b]{.49\textwidth} + \centering + \includegraphics[width=\linewidth]{plots/sine/K/K_maxFlarePeak_1.01-Flarecount-10_Bins.png} + \caption{10 bins} + \label{fig:K-Flarecount-10_Bins_1.01_maxpeak} + \end{subfigure} + \begin{subfigure}[b]{.49\textwidth} + \centering + \includegraphics[width=\linewidth]{plots/sine/K/K_maxFlarePeak_1.01-Flarecount-30_Bins.png} + \caption{30 bins} + \label{fig:K-Flarecount-30_Bins_1.01_maxpeak} + \end{subfigure} + \caption{Histograms showing the amount of flares with a normalized peak of less than 1.01 per phase for all 37 K dwarfs used in this study. The x-axis represents the normalized phase of the folded lightcurves. There are 10 (\subref{fig:K-Flarecount-10_Bins_1.01_maxpeak})/30 (\subref{fig:K-Flarecount-30_Bins_1.01_maxpeak}) bins of the phase, showing the number of flares per bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase (sine curve), with the maximum at phase $0 \pi$/$2 \pi$ and the minimum at phase $1 \pi$.} + \label{fig:K-Flarecount-peaks_1.01_maxpeak} +\end{figure} + +\begin{figure}[pt!] + \centering + \begin{subfigure}[b]{.49\textwidth} + \centering + \includegraphics[width=\linewidth]{plots/sine/K/K_maxFlarePeak_1.05-Flarecount-10_Bins.png} + \caption{10 bins} + \label{fig:K-Flarecount-10_Bins_1.05_maxpeak} + \end{subfigure} + \begin{subfigure}[b]{.49\textwidth} + \centering + \includegraphics[width=\linewidth]{plots/sine/K/K_maxFlarePeak_1.05-Flarecount-30_Bins.png} + \caption{30 bins} + \label{fig:K-Flarecount-30_Bins_1.05_maxpeak} + \end{subfigure} + \caption{Histograms showing the amount of flares with a normalized peak of less than 1.05 per phase for all 37 K dwarfs used in this study. The x-axis represents the normalized phase of the folded lightcurves. There are 10 (\subref{fig:K-Flarecount-10_Bins_1.05_maxpeak})/30 (\subref{fig:K-Flarecount-30_Bins_1.05_maxpeak}) bins of the phase, showing the number of flares per bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase (sine curve), with the maximum at phase $0 \pi$/$2 \pi$ and the minimum at phase $1 \pi$.} + \label{fig:K-Flarecount-peaks_1.05_maxpeak} +\end{figure} + \FloatBarrier \section{G dwarfs \label{sec:results:g_dwarfs}} @@ -105,14 +195,13 @@ Due to the lower number of detected flares on G type stars, the error bars in fi \begin{figure}[pt!] \centering - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/G/G-Flarecount-10_Bins.png} \caption{10 bins} \label{fig:G-Flarecount-10_Bins} \end{subfigure} - \vspace{1em} - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/G/G-Flarecount-30_Bins.png} \caption{30 bins} @@ -122,6 +211,42 @@ Due to the lower number of detected flares on G type stars, the error bars in fi \label{fig:G-Flarecount} \end{figure} +\begin{figure}[pt!] + \centering + \begin{subfigure}[b]{.49\textwidth} + \centering + \includegraphics[width=\linewidth]{plots/sine/G/G_minFlarePeak_1.05-Flarecount-10_Bins.png} + \caption{10 bins} + \label{fig:G-Flarecount-10_Bins_1.05_peak} + \end{subfigure} + \begin{subfigure}[b]{.49\textwidth} + \centering + \includegraphics[width=\linewidth]{plots/sine/G/G_minFlarePeak_1.05-Flarecount-30_Bins.png} + \caption{30 bins} + \label{fig:G-Flarecount-30_Bins_1.05_peak} + \end{subfigure} + \caption{Histograms showing the amount of flares with a normalized peak of greater than 1.05 per phase for all 71 G dwarfs used in this study. The x-axis represents the normalized phase of the folded lightcurves. There are 10 (\subref{fig:G-Flarecount-10_Bins_1.05_peak})/30 (\subref{fig:G-Flarecount-30_Bins_1.05_peak}) bins of the phase, showing the number of flares per bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase (sine curve), with the maximum at phase $0 \pi$/$2 \pi$ and the minimum at phase $1 \pi$.} + \label{fig:G-Flarecount-peaks_1.5_peak} +\end{figure} + +\begin{figure}[pt!] + \centering + \begin{subfigure}[b]{.49\textwidth} + \centering + \includegraphics[width=\linewidth]{plots/sine/G/G_maxFlarePeak_1.05-Flarecount-10_Bins.png} + \caption{10 bins} + \label{fig:G-Flarecount-10_Bins_1.05_maxpeak} + \end{subfigure} + \begin{subfigure}[b]{.49\textwidth} + \centering + \includegraphics[width=\linewidth]{plots/sine/G/G_maxFlarePeak_1.05-Flarecount-30_Bins.png} + \caption{30 bins} + \label{fig:G-Flarecount-30_Bins_1.05_maxpeak} + \end{subfigure} + \caption{Histograms showing the amount of flares with a normalized peak of less than 1.05 per phase for all 37 K dwarfs used in this study. The x-axis represents the normalized phase of the folded lightcurves. There are 10 (\subref{fig:G-Flarecount-10_Bins_1.05_maxpeak})/30 (\subref{fig:G-Flarecount-30_Bins_1.05_maxpeak}) bins of the phase, showing the number of flares per bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase (sine curve), with the maximum at phase $0 \pi$/$2 \pi$ and the minimum at phase $1 \pi$.} + \label{fig:G-Flarecount-peaks_1.05_maxpeak} +\end{figure} + \FloatBarrier \section{F dwarfs \label{sec:results:f_dwarfs}} @@ -130,14 +255,13 @@ Due to the low number of F type stars in this study, and the difficulty to detec \begin{figure}[pt!] \centering - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/F/F-Flarecount-10_Bins.png} \caption{10 bins} \label{fig:F-Flarecount-10_Bins} \end{subfigure} - \vspace{1em} - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/F/F-Flarecount-30_Bins.png} \caption{30 bins} @@ -156,14 +280,13 @@ Looking at the same data with 30 bins over the phase in figure \ref{fig:MKGF-Fla \begin{figure}[pt!] \centering - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/MKGF-Flarecount-10_Bins.png} \caption{10 bins} \label{fig:MKGF-Flarecount-10_Bins} \end{subfigure} - \vspace{1em} - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/MKGF-Flarecount-30_Bins.png} \caption{30 bins} @@ -188,14 +311,13 @@ Figure \ref{fig:BD-08_995-Flarecount-30_Bins} shows the same data just with 30 b \begin{figure}[pt!] \centering - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/BD-08_995/BD-08\space\space\space995-Flarecount-10_Bins.png} \caption{10 bins} \label{fig:BD-08_995-Flarecount-10_Bins} \end{subfigure} - \vspace{1em} - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/BD-08_995/BD-08\space\space\space995-Flarecount-30_Bins.png} \caption{30 bins} @@ -217,14 +339,13 @@ Looking at the folded TESS lightcurves of sector 5 (\ref{fig:BD-08_995-TESS5_fol \begin{figure}[pt!] \centering - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/BD-08_995/BD-08\space\space\space995_TESS-5-foldedLC-marked_fit_flares.png} \caption{TESS Sector 5} \label{fig:BD-08_995-TESS5_foldedLC} \end{subfigure} - \vspace{1em} - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/BD-08_995/BD-08\space\space\space995_TESS-32-foldedLC-marked_fit_flares.png} \caption{TESS Sector 32} @@ -243,14 +364,13 @@ Looking at the histogram with 30 bins of the same dataset (figure \ref{fig:TYC_1 \begin{figure}[pt!] \centering - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/TYC_1360-957-1/TYC 1360-957-1-Flarecount-10_Bins.png} \caption{10 bins} \label{fig:TYC_1360-957-1-Flarecount-10_Bins} \end{subfigure} - \vspace{1em} - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/TYC_1360-957-1/TYC 1360-957-1-Flarecount-30_Bins.png} \caption{30 bins} @@ -279,14 +399,12 @@ No such large flares can be seen in \subref{fig:TYC_1360-957-1-TESS45_foldedLC}, \caption{TESS Sector 44} \label{fig:TYC_1360-957-1-TESS44_foldedLC} \end{subfigure} - \vspace{1em} \begin{subfigure}[b]{.95\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/TYC_1360-957-1/TYC 1360-957-1_TESS-45-foldedLC-marked_fit_flares.png} \caption{TESS Sector 45} \label{fig:TYC_1360-957-1-TESS45_foldedLC} \end{subfigure} - \vspace{1em} \begin{subfigure}[b]{.95\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/TYC_1360-957-1/TYC 1360-957-1_TESS-46-foldedLC-marked_fit_flares.png} @@ -306,14 +424,13 @@ The histogram with 30 bins (figure \ref{fig:TYC_4595-107-1-Flarecount-30_Bins}) \begin{figure}[pt!] \centering - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/TYC_4595-107-1/TYC 4595-107-1-Flarecount-10_Bins.png} \caption{10 bins} \label{fig:TYC_4595-107-1-Flarecount-10_Bins} \end{subfigure} - \vspace{1em} - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/TYC_4595-107-1/TYC 4595-107-1-Flarecount-30_Bins.png} \caption{30 bins} @@ -335,14 +452,13 @@ Increasing the bins to 30 (figure \ref{fig:V471Tau-Flarecount-30_Bins}) does not \begin{figure}[pt!] \centering - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/V471Tau/V_star_ V471 Tau-Flarecount-10_Bins.png} \caption{10 bins} \label{fig:V471Tau-Flarecount-10_Bins} \end{subfigure} - \vspace{1em} - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/V471Tau/V_star_ V471 Tau-Flarecount-30_Bins.png} \caption{30 bins} @@ -362,14 +478,12 @@ Looking at the folded lightcurves for this star (see figures \ref{fig:V471Tau-TE \caption{TESS Sector 42} \label{fig:V471Tau-TESS42_foldedLC} \end{subfigure} - \vspace{1em} \begin{subfigure}[b]{.95\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/V471Tau/V_star_ V471 Tau_TESS-43-foldedLC-marked_fit_flares.png} \caption{TESS Sector 43} \label{fig:V471Tau-TESS43_foldedLC} \end{subfigure} - \vspace{1em} \begin{subfigure}[b]{.95\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/V471Tau/V_star_ V471 Tau_TESS-44-foldedLC-marked_fit_flares.png} @@ -401,14 +515,13 @@ The flare count in figure \ref{fig:HKAqr-Flarecount-30_Bins_Period} is very low. \begin{figure}[pt!] \centering - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/HKAqr/V_star_ HK Aqr-Flarecount-10_Bins.png} \caption{10 bins} \label{fig:HKAqr-Flarecount-10_Bins} \end{subfigure} - \vspace{1em} - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/HKAqr/V_star_ HK Aqr-Flarecount-30_Bins.png} \caption{30 bins} @@ -426,7 +539,6 @@ The flare count in figure \ref{fig:HKAqr-Flarecount-30_Bins_Period} is very low. \caption{TESS Sector 2} \label{fig:HKAqr-TESS2_foldedLC} \end{subfigure} - \vspace{1em} \begin{subfigure}[b]{.95\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/HKAqr/V_star_ HK Aqr_TESS-29-foldedLC-marked_fit_flares.png} @@ -456,14 +568,13 @@ The flare count in figure \ref{fig:HKAqr-Flarecount-30_Bins_Period} is very low. \begin{figure}[pt!] \centering - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/HKAqr/V_star_ HK Aqr-Flarecount-10_Bins_Period.png} \caption{10 bins} \label{fig:HKAqr-Flarecount-10_Bins_Period} \end{subfigure} - \vspace{1em} - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/HKAqr/V_star_ HK Aqr-Flarecount-30_Bins_Period.png} \caption{30 bins} @@ -481,7 +592,6 @@ The flare count in figure \ref{fig:HKAqr-Flarecount-30_Bins_Period} is very low. \caption{TESS Sector 29} \label{fig:HKAqr-TESS29_foldedLC_Period} \end{subfigure} - \vspace{1em} \begin{subfigure}[b]{.95\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/HKAqr/V_star_ HK Aqr_TESS-42-periodFoldedLC-marked_fit_flares.png} @@ -502,14 +612,13 @@ Increasing the bins to 30 (figure \ref{fig:KOI-256-Flarecount-30_Bins}) shows cl \begin{figure}[pt!] \centering - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/KOI-256/KOI-256-Flarecount-10_Bins.png} \caption{10 bins} \label{fig:KOI-256-Flarecount-10_Bins} \end{subfigure} - \vspace{1em} - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/KOI-256/KOI-256-Flarecount-30_Bins.png} \caption{30 bins} @@ -525,14 +634,13 @@ Looking at figure \ref{fig:KOI-256-Flarecount-30_Bins_Period} which shows the sa \begin{figure}[pt!] \centering - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/KOI-256/KOI-256-Flarecount-10_Bins_Period.png} \caption{10 bins} \label{fig:KOI-256-Flarecount-10_Bins_Period} \end{subfigure} - \vspace{1em} - \begin{subfigure}[b]{.95\textwidth} + \begin{subfigure}[b]{.49\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/KOI-256/KOI-256-Flarecount-30_Bins_Period.png} \caption{30 bins} @@ -552,7 +660,6 @@ Comparing the results of the flare peak distributions across the normalized phas \caption{Spot modulation folded} \label{fig:KOI-256-flarepeaks_1.7_spot} \end{subfigure} - \vspace{1em} \begin{subfigure}[b]{.95\textwidth} \centering \includegraphics[width=\linewidth]{plots/sine/KOI-256/KOI-256-Flarepeaks_maxY-1.3100095148043271_Period.png} diff --git a/Physics_Thesis_Template/main.pdf b/Physics_Thesis_Template/main.pdf index c55c076..4aec0f8 100644 Binary files a/Physics_Thesis_Template/main.pdf and b/Physics_Thesis_Template/main.pdf differ diff --git a/Physics_Thesis_Template/plots/sine/G/G_maxFlarePeak_1.05-Flarecount-10_Bins.png b/Physics_Thesis_Template/plots/sine/G/G_maxFlarePeak_1.05-Flarecount-10_Bins.png new file mode 100644 index 0000000..8008eff Binary files /dev/null and b/Physics_Thesis_Template/plots/sine/G/G_maxFlarePeak_1.05-Flarecount-10_Bins.png differ diff --git a/Physics_Thesis_Template/plots/sine/G/G_maxFlarePeak_1.05-Flarecount-30_Bins.png 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