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SGCMarkus
2025-05-14 23:10:28 +02:00
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Physics_Thesis_Template/content/chapter-gui.tex
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@@ -67,9 +67,9 @@ The checkboxes to flatten the lightcurve (figure \ref{fig:full_gui_normal_select
\FloatBarrier
\section{Data processing}
\section{Data processing \label{sec:gui:data_processing}}
Pressing the button "New FC" will start the processing of all fits files in the current loaded database. It will sequentially go through all files and apply the flare detection algorithms to the lightcurve, as well as generate the periodogram and folded lightcurves. This is done for both the SAP\_FLUX as well as the PDCSAP\_FLUX. Additionally plots for each individual lightcurve and processing step are generated. The included data includes:
Pressing the button "New FC" will start the processing of all fits files in the current loaded database. It will sequentially go through all files and apply the flare detection algorithms to the lightcurve, as well as generate the periodogram and optimized folded lightcurves. This is done for the PDCSAP\_FLUX. Additionally plots for each individual lightcurve and processing step are generated. The included data includes:
\begin{itemize}
\item Flares (peak, timestamp, datapoint index in the lightcurve, TESS/Kepler data quality flags)
@@ -77,11 +77,15 @@ Pressing the button "New FC" will start the processing of all fits files in the
\item Fits for the flares (fit, timestamps, indices in the lightcurve, TESS/Kepler data quality flags)
\item Uninterrupted timespans in the data
\item Total length of timespans in seconds
\item Rotational period
\item Spot modulation period
\item Folded lightcurve phase range
\item Folded lightcurve flare positions (phase, peak)
\item Period which was used to fold the lightcurve
\item Additional boundaries around minima and maxima
\end{itemize}
After this process is done, a new window will open. It allows to show multiple different statistics like flares per file, flares per star (total, or normalized to per 7 day period) or mean periods for each star. This window can be seen in figure \ref{fig:summary_statistics_window}.
And in the case the period and spot modulation of the star differs, it will seperately safe the folded lightcurves and related data for the stars period as well.
After this process is done, a new window will open. It allows to show multiple different statistics like flares per file, flares per star (total, or normalized to per 7 day period) or mean periods for each star. This window can be seen in figure \ref{fig:summary_statistics_window}.
The data can then be saved using the pandas (\cite{pandas}) "to\_pickle" functions and also loaded again using the "read\_pickle" function.