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Physics_Thesis_Template/content/appendixA.tex
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@@ -4,7 +4,7 @@
\centering
\tabcolsep=5pt
\begin{longtable}{lclll}
\caption{Table containing all stars of spectra type M for which flares have been found. The first column (Main Identifier) is matched with SIMBADs "MAIN\_ID" value for the star. The second column specifies the spectral type of the star according to SIMBAD (with the exception of the stars mentioned in section \ref{sec:data:sptype_identification}, which use the method described in that section). The TIC and KIC columns represent the TESS and Kepler Input Catalogues respectively. The fit type column specifies the used fit types which were found to work best for the lightcurves. The list is sorted first by spectral type, and then by main identifier.}
\caption{Table containing all main-sequence stars of spectral type M for which flares have been found. The first column (Main Identifier) is matched with SIMBADs "MAIN\_ID" value for the star. The second column specifies the spectral type of the star according to SIMBAD (with the exception of the stars mentioned in section \ref{sec:data:sptype_identification}, for which the method described in that section has been applied). The TIC and KIC columns represent the TESS and Kepler Input Catalogue identifiers respectively. The fit type column specifies the used fit types which were found to work best for the lightcurves. The list is sorted first by spectral type, and then by main identifier.}
\label{apA:list_of_m_stars}\\
\hline\hline
\multicolumn{1}{c}{Main Identifier} & \multicolumn{1}{c}{Sp. Type} & \multicolumn{1}{c}{TIC} & \multicolumn{1}{c}{KIC} & \multicolumn{1}{c}{Fit Type} \\
@@ -77,7 +77,7 @@ V* V692 Tau & M: & TIC 149923415 & - & sine \\
\centering
\tabcolsep=5pt
\begin{longtable}{lclll}
\caption{Table containing all stars of spectra type K for which flares have been found. The first column (Main Identifier) is matched with SIMBADs "MAIN\_ID" value for the star. The second column specifies the spectral type of the star according to SIMBAD (with the exception of the stars mentioned in section \ref{sec:data:sptype_identification}, which use the method described in that section). The TIC and KIC columns represent the TESS and Kepler Input Catalogues respectively. The fit type column specifies the used fit types which were found to work best for the lightcurves. The list is sorted first by spectral type, and then by main identifier.}
\caption{Table containing all main-sequence stars of spectral type K for which flares have been found. The first column (Main Identifier) is matched with SIMBADs "MAIN\_ID" value for the star. The second column specifies the spectral type of the star according to SIMBAD (with the exception of the stars mentioned in section \ref{sec:data:sptype_identification}, for which the method described in that section has been applied). The TIC and KIC columns represent the TESS and Kepler Input Catalogue idetifiers respectively. The fit type column specifies the used fit types which were found to work best for the lightcurves. The list is sorted first by spectral type, and then by main identifier.}
\label{apA:list_of_k_stars}\\
\hline\hline
\multicolumn{1}{c}{Main Identifier} & \multicolumn{1}{c}{Sp. Type} & \multicolumn{1}{c}{TIC} & \multicolumn{1}{c}{KIC} & \multicolumn{1}{c}{Fit Type} \\
@@ -122,7 +122,7 @@ V* CC Eri & K7V & TIC 142206123 & - & sine \\
\centering
\tabcolsep=5pt
\begin{longtable}{lclll}
\caption{Table containing all stars of spectra type G for which flares have been found. The first column (Main Identifier) is matched with SIMBADs "MAIN\_ID" value for the star. The second column specifies the spectral type of the star according to SIMBAD (with the exception of the stars mentioned in section \ref{sec:data:sptype_identification}, which use the method described in that section). The TIC and KIC columns represent the TESS and Kepler Input Catalogues respectively. The fit type column specifies the used fit types which were found to work best for the lightcurves. The list is sorted first by spectral type, and then by main identifier.}
\caption{Table containing all main-sequence stars of spectral type G for which flares have been found. The first column (Main Identifier) is matched with SIMBADs "MAIN\_ID" value for the star. The second column specifies the spectral type of the star according to SIMBAD (with the exception of the stars mentioned in section \ref{sec:data:sptype_identification}, for which the method described in that section has been applied). The TIC and KIC columns represent the TESS and Kepler Input Catalogues respectively. The fit type column specifies the used fit types which were found to work best for the lightcurves. The list is sorted first by spectral type, and then by main identifier.}
\label{apA:list_of_g_stars}\\
\hline\hline
\multicolumn{1}{c}{Main Identifier} & \multicolumn{1}{c}{Sp. Type} & \multicolumn{1}{c}{TIC} & \multicolumn{1}{c}{KIC} & \multicolumn{1}{c}{Fit Type} \\
@@ -167,7 +167,7 @@ HD 220186 & G9Ve & TIC 49619607 & - & sine \\
\centering
\tabcolsep=5pt
\begin{longtable}{lclll}
\caption{Table containing all stars of spectra type F for which flares have been found. The first column (Main Identifier) is matched with SIMBADs "MAIN\_ID" value for the star. The second column specifies the spectral type of the star according to SIMBAD (with the exception of the stars mentioned in section \ref{sec:data:sptype_identification}, which use the method described in that section). The TIC and KIC columns represent the TESS and Kepler Input Catalogues respectively. The fit type column specifies the used fit types which were found to work best for the lightcurves. The list is sorted first by spectral type, and then by main identifier.}
\caption{Table containing all main-sequence stars of spectral type F for which flares have been found. The first column (Main Identifier) is matched with SIMBADs "MAIN\_ID" value for the star. The second column specifies the spectral type of the star according to SIMBAD (with the exception of the stars mentioned in section \ref{sec:data:sptype_identification}, for which the method described in that section has been applied). The TIC and KIC columns represent the TESS and Kepler Input Catalogue identifiers respectively. The fit type column specifies the used fit types which were found to work best for the lightcurves. The list is sorted first by spectral type, and then by main identifier.}
\label{apA:list_of_f_stars}\\
\hline\hline
\multicolumn{1}{c}{Main Identifier} & \multicolumn{1}{c}{Sp. Type} & \multicolumn{1}{c}{TIC} & \multicolumn{1}{c}{KIC} & \multicolumn{1}{c}{Fit Type} \\
@@ -195,7 +195,7 @@ Kepler-1084 & F8V & TIC 267749737 & KIC 10857519 & sine \\
\centering
\tabcolsep=5pt
\begin{longtable}{lclll}
\caption{Table containing all stars which where analysed. The first column (Main Identifier) is matched with SIMBADs "MAIN\_ID" value for the star. The second column specifies the spectral type of the star according to SIMBAD (with the exception of the stars mentioned in section \ref{sec:data:sptype_identification}, which use the method described in that section). The TIC and KIC columns represent the TESS and Kepler Input Catalogues respectively. The list is sorted first by spectral type, and then by main identifier.}
\caption{Table containing all stars for which either no flares have been found, or which did not match the spectral types M, K, G or F. The first column (Main Identifier) is matched with SIMBADs "MAIN\_ID" value for the star. The second column specifies the spectral type of the star according to SIMBAD (with the exception of the stars mentioned in section \ref{sec:data:sptype_identification}, for which the method described in that section has been applied). The TIC and KIC columns represent the TESS and Kepler Input Catalogue identifiers respectively. The list is sorted first by spectral type, and then by main identifier.}
\label{apA:list_of_unused_stars}\\
\hline\hline
\multicolumn{1}{c}{Main Identifier} & \multicolumn{1}{c}{Sp. Type} & \multicolumn{1}{c}{TIC} & \multicolumn{1}{c}{KIC} & \multicolumn{1}{c}{Fit Type} \\
@@ -450,7 +450,7 @@ SDSS J192715.88+380808.2 & sdB+dM & - & KIC 2991403 & sine \\
\centering
\tabcolsep=5pt
\begin{longtable}{lclll}
\caption{Table containing all stars which where analysed. The first column (Main Identifier) is matched with SIMBADs "MAIN\_ID" value for the star. The second column specifies the spectral type of the star according to SIMBAD (with the exception of the stars mentioned in section \ref{sec:data:sptype_identification}, which use the method described in that section). The TIC and KIC columns represent the TESS and Kepler Input Catalogues respectively. The list is sorted first by spectral type, and then by main identifier.}
\caption{Table containing all stars which where analysed. The first column (Main Identifier) is matched with SIMBADs "MAIN\_ID" value for the star. The second column specifies the spectral type of the star according to SIMBAD (with the exception of the stars mentioned in section \ref{sec:data:sptype_identification}, for which the method described in that section has been applied). The TIC and KIC columns represent the TESS and Kepler Input Catalogue identifiers respectively. The list is sorted first by spectral type, and then by main identifier.}
\label{apA:list_of_all_stars}\\
\hline\hline
\multicolumn{1}{c}{Main Identifier} & \multicolumn{1}{c}{Sp. Type} & \multicolumn{1}{c}{TIC} & \multicolumn{1}{c}{KIC} & \multicolumn{1}{c}{Fit Type} \\