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SGCMarkus 96debcc729 update result description part 1 2025-05-16 23:37:11 +02:00
SGCMarkus a06f142f08 add used star list 2025-05-16 18:07:52 +02:00
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Physics_Thesis_Template/bib-refs.bib
+7
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@@ -1,3 +1,10 @@
@misc{spectral_type_color_table,
title={Intrinsic colours as a function of spectral type},
url={https://www.stsci.edu/~inr/intrins.html},
author={Neill Reid},
urldate = {2025-05-15}
}
@misc{pyqt5,
title={PyQt5},
url={https://www.riverbankcomputing.com/static/Docs/PyQt5/introduction.html},
Physics_Thesis_Template/content/appendixA.tex
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\chapter{List of stars \label{chap:list_of_stars}}
\chapter{Literature values for \Kepler systems \label{chap:appendixExtensiveTables}}
\label{sec:appendix}
%\section*{Authors' Note}
%\lipsum[4]
%\section{Literature values for \Kepler-systems}\label{sec:appendixA}
\physit{[This appendix has been published as Appendix\,C of \cite{Beck2018}].}
The parameters for eclipsing binaries are taken from the dynamical solution of G16. For the list of heartbeat stars (B14), radius and mass were inferred from seismic scaling relations and corrected for the systematic mass overestimate of 15\% reported by G16. Surface rotation periods were adopted from G14, B14 and B18. For four stars of B14, KIC\,7431665, KIC\,11044668, KIC\,8803882, and KIC\,7799540, no orbital parameters have yet been published.
\section{Compilation of literature values}
We refer to the cited literature for details on the applied methodology.
\Table{tab:longTable} contains the following parameters,
\begin{itemize}
\item \textit{KIC} specifies the target identification number in the \Kepler Input Catalog.
\item \textit{Type} indicates if a binary system is an eclipsing binary (EB), a heartbeat system (HB), or an eclipsing heartbeat system (eHB). 'NO' indicates that the star belongs to the four non-oscillating stars of G14/G16.
\item P$_{\mathrm{orbit}}$ is the measured orbital period.
\item $e$ is the orbital eccentricity.
\item $\nu_{\mathrm{max}}$ is the peak frequency of the excess of oscillation power.
\item $R$/$R_{\odot}$ is the stellar radius in solar units. Values from B14 are seismically inferred and corrected for the 5\% overestimate of seismic radius. Values from G16 originate from a dynamical solution.
\item $M$/$M_{\odot}$ is the stellar mass in solar units. Values from B14 are seismically inferred and corrected for the 15\% overestimate of seismic mass. Values from G16 originate from a dynamical solution.
\item {$q=M_2$/$M_1$} is the mass ratio between the two stellar components in the system. '?' indicates if $q$ has not been determined for a given system.
\item $T_{\mathrm{eff}}$ is the effective temperature.
\item \textit{P$_{\mathrm{rot}}$} specifies the time scale of the flux modulation, identified as the surface rotation period. The sources of the values are G14 and B18. We round all period values to the next full day.
\item The dimensionless number \textit{\varR} is proportional to the inverse of the time scale of tidal circularisation (see Eq. XX). If no value of the mass ratio is specified, \varR is calculated for $q=0.5$.
\item REF: the last column is specifying the literature references. If several papers are reporting on a given system, values of the most recent paper are cited. Previous references are given in brackets.
\end{itemize}
\begin{landscape}
%\begin{able}
\label{tab:longTable}
{
\centering
\tabcolsep=2pt
\begin{longtable}{rrrrrrrrrrrl}
\caption{Literature Parameters of red-giant binaries in the \Kepler sample. } \\
\tabcolsep=8pt
\label{apA:list_of_m_stars}
\begin{longtable}{llll}
\caption{Table containing all stars used in this study of spectral type M. 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.} \\
\hline\hline
\multicolumn{1}{c}{KIC} &
\multicolumn{1}{c}{Type} &
\multicolumn{1}{c}{P$_{\mathrm{orb}}$} &
\multicolumn{1}{c}{$e$} &
\multicolumn{1}{c}{$\nu_{\mathrm{max}}$} &
\multicolumn{1}{c}{R/R$_\odot$} &
\multicolumn{1}{c}{M/M$_\odot$} &
\multicolumn{1}{c}{$q$} &
\multicolumn{1}{c}{T} &
\multicolumn{1}{c}{P$_{\mathrm{rot}}$} &
\multicolumn{1}{c}{$\varepsilon_{\mathrm{R}}$} &
REF \\
& &
\multicolumn{1}{c}{[days]} &
\multicolumn{1}{c}{[]} &
\multicolumn{1}{c}{[$\mu$Hz]} &
\multicolumn{1}{c}{[]} &
\multicolumn{1}{c}{[]} &
\multicolumn{1}{c}{[]}&
\multicolumn{1}{c}{[K]} &
\multicolumn{1}{c}{[days]} &
\multicolumn{1}{c}{[]} & \\
\multicolumn{1}{c}{Main Identifier} & \multicolumn{1}{c}{Spectral Type} & \multicolumn{1}{c}{TIC} & \multicolumn{1}{c}{KIC} \\
\hline
\endfirsthead
\caption{Literature Parameters of red-giant binaries in the \Kepler sample. (continued) }\\
\hline\hline
\multicolumn{1}{c}{KIC} &
\multicolumn{1}{c}{Type} &
\multicolumn{1}{c}{P$_{\mathrm{orb}}$} &
\multicolumn{1}{c}{$e$} &
\multicolumn{1}{c}{\numax} &
\multicolumn{1}{c}{R/R$_\odot$} &
\multicolumn{1}{c}{M/M$_\odot$} &
\multicolumn{1}{c}{$q$} &
\multicolumn{1}{c}{T} &
\multicolumn{1}{c}{P$_{\mathrm{rot}}$} &
\multicolumn{1}{c}{\varR} &
REF \\
& &
\multicolumn{1}{c}{[days]} &
\multicolumn{1}{c}{[]} &
\multicolumn{1}{c}{[$\mu$Hz]} &
\multicolumn{1}{c}{[]} &
\multicolumn{1}{c}{[]} &
\multicolumn{1}{c}{[]}&
\multicolumn{1}{c}{[K]} &
\multicolumn{1}{c}{[days]} &
\multicolumn{1}{c}{[]} & \\
\multicolumn{1}{c}{Main Identifier} & \multicolumn{1}{c}{Spectral Type} & \multicolumn{1}{c}{TIC} & \multicolumn{1}{c}{KIC} \\
\hline
\endhead
\hline
2444348 & HB & 103.50 $\pm$ 0.01 & 0.48 $\pm$ 0.01 & 30.5 $\pm$ 0.3 & 14.2 $\pm$ 0.3 & 1.6 $\pm$ 0.1 & ? & 4565 & - & -0.53 & B14 \\ % 14.9 1.94 -0.29264836 23617660210411000.0 0.5
2697935 & eHB & 21.50 $\pm$ 0.02 & 0.41 $\pm$ 0.02 & $\sim$ 405.6 & $\sim$ 3.1 & $\sim$ 1.2 & ? & 4883 & - & -0.73 & B14 \\ % 3.26 1.45 -0.187737261 1193550610212.7 0.5
2720096 & HB & 26.70 $\pm$ 0.01 & 0.49 $\pm$ 0.01 & 110.1 $\pm$ 0.7 & 6.6 $\pm$ 0.1 & 1.3 $\pm$ 0.1 & ? & 4812 & - & 0.83 & B14 \\ % 6.98 1.54 -6.735778437 169548153353192.0 0.5
3955867 & EB,\,NO & 33.65685 $\pm$ 0.00007 & 0.019 $\pm$ 0.002 & $-$ & 7.9 $\pm$ 0.1 & 1.10 $\pm$ 0.06 & 0.84 $\pm$ 0.05 & 4884 & 33 & 1.14 & G16 (G14) \\ % 0.92 0.03 -13.83929209 530109950860996.0 0.836363636
4569590 & EB,\,NO & 41.3710 $\pm$ 0.0001 & 0.004 $\pm$ 0.001 & $-$ & 14.1 $\pm$ 0.2 & 1.6 $\pm$ 0.10 & 0.66 $\pm$ 0.05 & 4706 & 41 & 1.67 & G16 (G14) \\ % 1.05 0.04 -47.17584985 23026610543707600.0 0.65625
4663623 & EB & 358.09 $\pm$ 0.0003 & 0.43 $\pm$ 0.01 & 54.1 $\pm$ 0.2 & 9.7 $\pm$ 0.2 & 1.36 $\pm$ 0.09 & 0.99 $\pm$ 0.08 & 4812 & - & -4.08 & G16 (G14) \\ % 1.34 0.07 -8.34456E-05 2016961378909580.0 0.985294118
5006817 & HB & 94.812 $\pm$ 0.002 & 0.71 $\pm$ 0.01 & 145.9 $\pm$ 0.5 & 5.5 $\pm$ 0.1 & 1.3 $\pm$ 0.1 & 0.199 $\pm$ 0.001 & 5000 & - & -2.80 & B14 \\ % 5.84 1.49 -0.001598043 53105792890595.8 0.199
5039392 & HB & 236.70 $\pm$ 0.02 & 0.44 $\pm$ 0.01 & 6.2 $\pm$ 0.1 & 22.8 $\pm$ 0.7 & 0.8 $\pm$ 0.1 & ? & 4110 & - & -0.01 & B14 \\ % 24 0.98 -0.967120434 525980261009751000.0 0.5
5179609 & EB & 43.93108 $\pm$ 0.000002 & 0.150 $\pm$ 0.001 & 322 $\pm$ 1.0 & 3.50 $\pm$ 0.03 & 1.18 $\pm$ 0.03 & 0.51 $\pm$ 0.02 & 5003 & 182 & -1.96 & G16 (G14) \\ % 0.60 0.01 -0.01088514 2646650293458.1 0.508474576
5308778 & EB & 40.5661 $\pm$ 0.0003 & 0.006 $\pm$ 0.005 & 49 $\pm$ 1.1 & 10.1 $\pm$ 0.3 & 1.5 $\pm$ 0.1 & 0.43 $\pm$ 0.03 & 4900 & 39 & 0.80 & G16 (G14) \\ % 0.64 0.01 -6.305804877 2623890671999020.0 0.426666667
5786154 & EB & 197.918 $\pm$ 0.0004 & 0.3764 $\pm$ 0.0009 & 29.8 $\pm$ 0.2 & 11.4 $\pm$ 0.2 & 1.06 $\pm$ 0.06 & 0.96 $\pm$ 0.07 & 4747 & - & -1.85 & G16 (G14) \\ % 1.02 0.04 -0.014007755 5771174080581860.0 0.962264151
7037405 & EB & 207.1083 $\pm$ 0.0007 & 0.238 $\pm$ 0.004 & 21.8 $\pm$ 0.1 & 14.1 $\pm$ 0.2 & 1.25 $\pm$ 0.04 & 0.91 $\pm$ 0.03 & 4516 & - & -1.62 & G16 (G14) \\ % 1.14 0.02 -0.023721231 23026610543707600.0 0.912
7377422 & EB & 107.6213 $\pm$ 0.0004 & 0.4377 $\pm$ 0.0005 & 40 $\pm$ 2.1 & 9.5 $\pm$ 0.2 & 1.05 $\pm$ 0.08 & 0.81 $\pm$ 0.07 & 4938 & 55 & -0.96 & G16 (G14) \\ % 0.85 0.03 -0.109828309 1761141547380960.0 0.80952381
% 7431665 & HB & 281.4 $\pm$ ? & - $\pm$ - & 54.0 $\pm$ 0.7 & 8.9 $\pm$ 0.1 & 1.2 $\pm$ 0.1 & ? & 4580 & - & -3.59 & B14 \\ % 9.4 1.36 -0.000258751 1177217175096960.0 0.5
% 7799540 & HB & 71.8 $\pm$ ? & - $\pm$ - & 347.2 $\pm$ 5 & $\sim$ 3.5 & $\sim$ 1.3 & ? & 5177 & - & -3.28 & B14 \\ % 3.64 1.52 -0.000521441 2446607317192.6 0.5
7943602 & EB,\,NO & 14.69199 $\pm$ 0.00004 & 0.001 $\pm$ 0.003 & $-$ & 6.6 $\pm$ 0.2 & 1.0 $\pm$ 0.10 & 0.78 $\pm$ 0.09 & 5096 & 15 & 2.70 & G16 (G14) \\ % 0.78 0.05 -497.4981512 164454064905904.0 0.78
8054233 & EB & 1058.16 $\pm$ 0.02 & 0.2718 $\pm$ 0.0004 & 46.5 $\pm$ 0.3 & 10.7 $\pm$ 0.1 & 1.60 $\pm$ 0.06 & 0.69 $\pm$ 0.04 & 4971 & - & -6.61 & G16 (G14) \\ % 1.10 0.04 -2.46436E-07 3820339730270180.0 0.6875
8095275 & HB & 23.00 $\pm$ 0.01 & 0.32 $\pm$ 0.01 & 69.3 $\pm$ 0.3 & 7.4 $\pm$ 0.1 & 1.0 $\pm$ 0.1 & ? & 4622 & - & 1.86 & B14 \\ % 7.78 1.21 -73.23309501 343614465988859.0 0.5
8144355 & HB & 80.55 $\pm$ 0.01 & 0.76 $\pm$ 0.01 & 179.0 $\pm$ 2 & 4.7 $\pm$ 0.1 & 1.1 $\pm$ 0.1 & ? & 4875 & - & -2.41 & B14 \\ % 4.9 1.26 -0.003890391 16942236650096.4 0.5
8210370 & HB & 153.50 $\pm$ 0.01 & 0.70 $\pm$ 0.01 & 44.1 $\pm$ 0.8 & 10.0 $\pm$ 0.2 & 1.2 $\pm$ 0.1 & ? & 4585 & - & -1.92 & B14 \\ % 10.5 1.4 -0.012117691 2419561133683660.0 0.5
8410637 & EB & 408.3 $\pm$ 0.5 & 0.689 $\pm$ 0.001 & 46.0 $\pm$ 0.2 & 10.7 $\pm$ 0.1 & 1.56 $\pm$ 0.3 & 0.85 $\pm$ 0.16 & 4800 & - & -4.34 & F13 \\ % 1.32 0.02 -4.60123E-05 3820339730270180.0 0.846153846
\endfoot
8430105 & EB & 63.32713 $\pm$ 0.00003 & 0.2564 $\pm$ 0.0002 & 76.7 $\pm$ 0.6 & 7.65 $\pm$ 0.05 & 1.31 $\pm$ 0.02 & 0.63 $\pm$ 0.01 & 5042 & 122 & -0.73 & G16 (G14) \\ % 0.83 0.01 -0.187065661 429981267052472.0 0.633587786
\hline
8702921 & EB & 19.38446 $\pm$ 0.00002 & 0.0964 $\pm$ 0.0008 & 195.6 $\pm$ 0.5 & 5.32 $\pm$ 0.05 & 1.67 $\pm$ 0.05 & 0.16 $\pm$ 0.01 & 5058 & 98 & 0.26 & G16 (G14) \\ % 0.274 0.009 -1.815382661 40410880990330.7 0.164071856
% 8803882 & HB & 89.7 $\pm$ ? & - $\pm$ - & 347.0 $\pm$ 3 & 3.5 $\pm$ 0.1 & 1.2 $\pm$ 0.1 & ? & 5043 & - & -3.64 & B14 \\ % 3.68 1.4 -0.00023094 2627021107627.9 0.5
8912308 & HB & 20.17 $\pm$ 0.01 & 0.23 $\pm$ 0.01 & $\sim$ 350.0 0 & $\sim$ 4.0 & $\sim$ 1.7 & ? & 4872 & - & -0.39 & B14 \\ % 4.2 2.02 -0.407215935 6210794263470.3 0.5
9151763 & HB & 437.51 $\pm$ 0.03 & 0.73 $\pm$ 0.01 & 13.8 $\pm$ 0.2 & 16.7 $\pm$ 0.4 & 1.0 $\pm$ 0.1 & ? & 4290 & - & -2.62 & B14 \\ % 17.6 1.19 -0.002379785 69836381728503000.0 0.5
9163796 & HB & 121.30 $\pm$ 0.01 & 0.69 $\pm$ 0.002 & 165.3 $\pm$ 1.3 & 5.1 $\pm$ 0.1 & 1.2 $\pm$ 0.1 & 0.985 $\pm$ 0.005 & 4960 & 130 & -3.17 & B18 (B14) \\ % 5.35 1.39 -0.00066911 30017697979301.3 0.985221675
9246715 & EB & 171.27688 $\pm$ 0.00001 & 0.3559 $\pm$ 0.0003 & 106.4 $\pm$ 0.8 & 8.30 $\pm$ 0.04 & 2.149 $\pm$ 0.007 & 0.990 $\pm$ 0.005 & 5030 & 93 & -3.54 & R16 (G14) \\ % 2.171 0.007 -0.000289876 731159241518636.0 1.01023732
9291629 & EB,\,NO & 20.68643 $\pm$ 0.00004 & 0.007 $\pm$ 0.002 & $-$ & 7.99 $\pm$ 0.05 & 1.14 $\pm$ 0.03 & 0.96 $\pm$ 0.03 & 4713 & 21 & 2.26 & G16 (G14) \\ % 1.1 0.02 -180.6275087 570680621599525.0 0.964912281
9408183 & HB & 49.70 $\pm$ 0.01 & 0.42 $\pm$ 0.01 & 164.8 $\pm$ 0.2 & 4.8 $\pm$ 0.1 & 1.0 $\pm$ 0.1 & ? & 4900 & - & -1.18 & B14 \\ % 5.02 1.23 -0.065346161 19832408593602.6 0.5
9540226 & eHB & 175.4439 $\pm$ 0.0006 & 0.3880 $\pm$ 0.0002 & 27.1 $\pm$ 0.2 & 12.8 $\pm$ 0.1 & 1.33 $\pm$ 0.05 & 0.74 $\pm$ 0.04 & 4692 & - & -1.64 & G16\,(B14,\,G14) \\ % 0.98 0.03 -0.023126672 12267342609935500.0 0.736842105
9970396 & EB & 235.2985 $\pm$ 0.0002 & 0.194 $\pm$ 0.007 & 63.7 $\pm$ 0.2 & 8.0 $\pm$ 0.2 & 1.14 $\pm$ 0.03 & 0.89 $\pm$ 0.03 & 4916 & - & -3.38 & G16 (G14) \\ % 1.02 0.02 -0.000418992 575346410047194.0 0.894736842
10001167 & EB & 120.3903 $\pm$ 0.0005 & 0.159 $\pm$ 0.003 & 19.9 $\pm$ 0.1 & 12.7 $\pm$ 0.3 & 0.81 $\pm$ 0.05 & 0.98 $\pm$ 0.07 & 4700 & - & 0.03 & G16 (G14) \\ % 0.79 0.03 -1.077727137 11656705266394900.0 0.975308642
10614012 & eHB & 132.13 $\pm$ 0.01 & 0.71 $\pm$ 0.01 & 70.2 $\pm$ 0.9 & 8.2 $\pm$ 0.2 & 1.3 $\pm$ 0.1 & ? & 4715 & - & -2.23 & B14 \\ % 8.6 1.49 -0.005849059 659749667940527.0 0.5
% 11044668 & HB & 139.5 $\pm$ ? & - $\pm$ - & 50.2 $\pm$ 0.2 & 7.8 $\pm$ 0.1 & 0.8 $\pm$ 0.1 & ? & 4565 & - & -1.85 & B14 \\ % 8.18 0.99 -0.014152208 476231666115527.0 0.5
\hline
\end{longtable}
%\end{table}%
\end{landscape}
\section{Tidal properties of selected systems}
Table\,\ref{tab:10th} lists the following parameters for the systems' red-giant primary with known $P_{\mathrm{rot}}$,
\begin{itemize}
\item $\delta_{\mathrm{10}}$ is the 10$^{\mathrm{th}}$ percentile of the logarithm of the ratio between the dissipation of the equilibrium and the dynamical tide, $\delta$\,=\,$\log (\mathcal{D}_{\mathrm{eq}}$\,/\,$<$$\mathcal{D}$$>$$_\omega)$.
\item $\tau_{\mathrm{conv,10}}$ is the corresponding convective turnover timescale computed in the middle of the convective zone.
\item $P_{\mathrm{tide}}$ > $\tau_{\mathrm{conv,10}}$ indicates if the tidal period is longer than the convective turnover timescale (Yes / No).
\end{itemize}
\vspace {5mm}
\begin{table}[h!]
\caption{Evolution of $\delta_{\mathrm{10}}$ for the systems with know rotation period.}
\label{tab:10th}
%\centering
\tabcolsep=10pt
\hfill\begin{tabular}{rrccc}
\hline\hline
\multicolumn{1}{c}{KIC} &
\multicolumn{1}{c}{$P_{\mathrm{tide}}$} & $\tau_{\mathrm{conv,10}}$ & $P_{\mathrm{tide}}$ > $\tau_{\mathrm{conv,10}}$ & $\delta_{\mathrm{10}}$\\
& \multicolumn{1}{c}{[days]} & [days] & & \\
\endlastfoot
2MASS J18460555+4332131 & M & TIC 123317330 & KIC 7800087 \\
2MASS J18472701+4348011 & M & TIC 123410529 & KIC 8007234 \\
2MASS J18491356+4619042 & M & TIC 123447780 & KIC 9631548 \\
2MASS J18511354+4227227 & M & TIC 164411695 & KIC 6925256 \\
2MASS J18511902+4837594 & M & TIC 48216443 & KIC 11069034 \\
2MASS J18512069+4846013 & M & TIC 48216303 & KIC 11122350 \\
2MASS J18524238+4828368 & M & TIC 48304549 & KIC 10960823 \\
2MASS J18525314+4818044 & M & TIC 48304703 & KIC 10905192 \\
2MASS J18525455+4634012 & M & TIC 164457389 & KIC 9754582 \\
2MASS J18531060+4050093 & M & TIC 237158804 & KIC 5597695 \\
2MASS J18535987+4741070 & M & TIC 164525174 & KIC 10452840 \\
2MASS J18541728+4305206 & M & TIC 164529739 & KIC 7422811 \\
2MASS J18545269+4107528 & M & TIC 350987684 & KIC 5855808 \\
2MASS J18561787+4457391 & M & TIC 164670879 & KIC 8737443 \\
2MASS J18565158+4448162 & M & TIC 164671055 & KIC 8673358 \\
2MASS J18570619+4516101 & M & TIC 164677934 & KIC 8935942 \\
2MASS J18572876+4035369 & M & TIC 120251682 & KIC 5342558 \\
2MASS J18574689+4115593 & M & TIC 120254207 & KIC 5941226 \\
2MASS J18592859+4351465 & M & TIC 164786997 & KIC 8012943 \\
2MASS J19000393+4109460 & M & TIC 120419969 & KIC 5858361 \\
2MASS J19001025+4045358 & M & TIC 120422710 & KIC 5515142 \\
2MASS J19005916+4400190 & M & TIC 164889286 & KIC 8150479 \\
2MASS J19011064+4206175 & M & TIC 164886887 & KIC 6672948 \\
2MASS J19011256+4152067 & M & TIC 399822429 & KIC 6425989 \\
2MASS J19020142+4110533 & M & TIC 120576193 & KIC 5859365 \\
2MASS J19023480+4539052 & M & TIC 352013620 & KIC 9205855 \\
2MASS J19024516+4429007 & M & TIC 352012319 & KIC 8417053 \\
2MASS J19030585+4046008 & M & TIC 120579026 & KIC 5516671 \\
2MASS J19033576+3941263 & M & TIC 120684614 & KIC 4544623 \\
2MASS J19034709+4317208 & M & TIC 158166384 & KIC 7592133 \\
2MASS J19035284+4338273 & M & TIC 158165866 & KIC 7877209 \\
2MASS J19041026+4530403 & M & TIC 158172860 & KIC 9142714 \\
2MASS J19053703+4235308 & M & TIC 158218091 & KIC 7018323 \\
2MASS J19061507+5029221 & M & TIC 399825094 & KIC 12004872 \\
2MASS J19061662+4502422 & M & TIC 158274889 & KIC 8807085 \\
2MASS J19063685+4928043 & M & TIC 399825963 & KIC 11498106 \\
2MASS J19064350+5020087 & M & TIC 399825217 & KIC 11955208 \\
2MASS J19064648+4931162 & M & TIC 399825921 & KIC 11550428 \\
2MASS J19074075+3752413 & M & TIC 121022434 & KIC 2557669 \\
2MASS J19081745+3902346 & M & TIC 121085753 & KIC 3940372 \\
2MASS J19083962+4221137 & M & TIC 158388172 & KIC 6849112 \\
2MASS J19085407+4320395 & M & TIC 158423632 & KIC 7670700 \\
2MASS J19103260+4322147 & M & TIC 158551504 & KIC 7671594 \\
2MASS J19104382+4039368 & M & TIC 121329525 & KIC 5435958 \\
2MASS J19110814+4024571 & M & TIC 121333779 & KIC 5262561 \\
2MASS J19114749+4048205 & M & TIC 121461193 & KIC 5608002 \\
2MASS J19130891+5127421 & M & TIC 298961665 & KIC 12505054 \\
2MASS J19135561+4319299 & M & TIC 158725435 & KIC 7673428 \\
2MASS J19141052+4559479 & M & TIC 158787568 & KIC 9396972 \\
2MASS J19143720+4243450 & M & TIC 158795349 & KIC 7190459 \\
2MASS J19152845+5001374 & M & TIC 299088298 & KIC 11808734 \\
2MASS J19160242+4726491 & M & TIC 158983853 & KIC 10332732 \\
2MASS J19170322+4953087 & M & TIC 299159305 & KIC 11708034 \\
2MASS J19200001+3844383 & M & TIC 122225323 & KIC 3640527 \\
2MASS J19200978+4954168 & M & TIC 267747418 & KIC 11760021 \\
2MASS J19205088+5018194 & M & TIC 406950619 & KIC 11961075 \\
2MASS J19210354+4523201 & M & TIC 159303166 & KIC 9017693 \\
2MASS J19213187+4459115 & M & TIC 159387244 & KIC 8749769 \\
2MASS J19230963+3739397 & M & TIC 122672447 & KIC 2300039 \\
2MASS J19232149+5107053 & M & TIC 417655942 & KIC 12356051 \\
2MASS J19233077+5035350 & M & TIC 417656504 & KIC 12060710 \\
2MASS J19233788+4518061 & M & TIC 159520226 & KIC 9019435 \\
2MASS J19240851+3747169 & M & TIC 122781970 & KIC 2441562 \\
2MASS J19242752+5106364 & M & TIC 350738203 & KIC 12356489 \\
2MASS J19255059+4532219 & M & TIC 159761686 & KIC 9153754 \\
2MASS J19291103+4821243 & M & TIC 424864617 & KIC 10921009 \\
2MASS J19304396+4112528 & M & TIC 137759349 & KIC 5962956 \\
2MASS J19304840+4142454 & M & TIC 137758161 & KIC 6366739 \\
2MASS J19335656+4010546 & M & - & KIC 5016904 \\
2MASS J19343395+4137235 & M & TIC 138222062 & KIC 6290811 \\
2MASS J19353467+3943573 & M & TIC 138436033 & KIC 4662431 \\
2MASS J19353874+4708324 & M & TIC 270790828 & KIC 10146539 \\
2MASS J19365745+4628121 & M & TIC 270957843 & KIC 9716117 \\
2MASS J19374745+4341098 & M & TIC 271047224 & KIC 7898781 \\
2MASS J19421615+4928069 & M & TIC 27531488 & KIC 11515276 \\
2MASS J19423900+5108356 & M & TIC 27639064 & KIC 12365719 \\
2MASS J19433653+4758149 & M & TIC 27645448 & KIC 10676126 \\
2MASS J19443380+4843497 & M & TIC 27770198 & KIC 11147271 \\
2MASS J19444493+4720327 & M & TIC 272279258 & KIC 10285642 \\
2MASS J19450930+4754591 & M & TIC 27771932 & KIC 10677397 \\
2MASS J19451164+4345265 & M & TIC 272270363 & KIC 7973675 \\
2MASS J19454134+3906345 & M & TIC 184471264 & KIC 4077867 \\
2MASS J19471875+4123248 & M & TIC 239228371 & KIC 6060845 \\
2MASS J19471987+4747258 & M & TIC 272841049 & KIC 10548508 \\
2MASS J19480997+4310160 & M & TIC 272943707 & KIC 7547969 \\
2MASS J19503771+4705359 & M & TIC 273378083 & KIC 10091786 \\
2MASS J19503804+4041450 & M & TIC 169816129 & KIC 5471468 \\
2MASS J19505785+4630250 & M & TIC 273379615 & KIC 9786877 \\
2MASS J19510637+4505045 & M & TIC 273383619 & KIC 8836388 \\
2MASS J19525571+4743328 & M & TIC 273874034 & KIC 10553513 \\
2MASS J19542833+4420425 & M & TIC 268158580 & KIC 8387621 \\
2MASS J19543981+4814406 & M & TIC 264508845 & KIC 10880514 \\
2MASS J19550625+4009192 & M & TIC 171101426 & KIC 5041192 \\
2MASS J19553603+4805356 & M & TIC 416528859 & KIC 10753072 \\
2MASS J19561258+4335485 & M & TIC 268485803 & KIC 7847566 \\
2MASS J19584764+4711122 & M & TIC 269029909 & KIC 10165815 \\
2MASS J20000387+4531405 & M & TIC 239234887 & KIC 9179906 \\
ATO J285.1153+45.7850 & M & TIC 164882037 & KIC 9267818 \\
KOI-1654 & M & TIC 48355200 & KIC 11546211 \\
UCAC4 639-062929 & M & TIC 120963868 & KIC 2284919 \\
UCAC4 643-073385 & M & TIC 138647610 & KIC 3454793 \\
UCAC4 651-066418 & M & TIC 120354289 & KIC 4904647 \\
UCAC4 661-082974 & M & TIC 268288304 & KIC 6720765 \\
UCAC4 664-071715 & M & TIC 158430593 & KIC 7104739 \\
UCAC4 668-073165 & M & TIC 158432884 & KIC 7741987 \\
UCAC4 683-066189 & M & TIC 351897570 & KIC 9692206 \\
UCAC4 707-062317 & M & TIC 299097784 & KIC 12403318 \\
1RXS J060224.9-163451 & M0 & TIC 95328477 & - \\
V* MY Tau & M0.5e & TIC 348638763 & - \\
WOH S 209 & M0: & TIC 179038379 & - \\
Kepler-210 & M0V & TIC 63283780 & KIC 7447200 \\
MCC 428 & M0V & TIC 434136638 & - \\
V* HK Aqr & M0Ve & TIC 5656273 & - \\
HG 7-26 & M1 & TIC 345454031 & - \\
V* OT Ser & M1.0V & TIC 355793860 & - \\
V* V631 Tau & M1.5 & TIC 348638813 & - \\
2MASS J18563342+4513481 & M1.5V & TIC 164670606 & KIC 8935655 \\
G 6-33 & M1.5V & TIC 434160946 & - \\
V* FF And & M1Ve+M1Ve & TIC 267802440 & - \\
HD 197481 & M1VeBa1 & TIC 441420236 & - \\
{[LM84]} 3-13 & M2 & TIC 165124012 & - \\
V* AX Cnc & M2.0 & TIC 175233993 & - \\
2MASS J19412234+5104273 & M2.1 & TIC 27454242 & KIC 12314646 \\
1RXS J004211.1-425245 & M2.2 & TIC 80427281 & - \\
2MASS J04133314-5231586 & M2.4 & TIC 219229275 & - \\
PM J19399+3950 & M2.5 & TIC 138893136 & KIC 4758595 \\
UCAC4 647-065171 & M2.5 & TIC 121215155 & KIC 4142890 \\
G 10-29 & M2.5V & TIC 396951485 & - \\
LP 474-124 & M2.5V & TIC 348663808 & - \\
2MASS J19130537+5020559 & M2.5Ve & TIC 298962893 & KIC 11957647 \\
ASAS J232857-6802.4 & M2.5Ve & TIC 229807000 & - \\
2MASS J19324802+4200580 & M2.7 & TIC 275496670 & KIC 6610837 \\
2MASS J19445931+4812415 & M2.8 & TIC 27772498 & KIC 10872868 \\
V* V497 Tau & M2.9 & TIC 258032026 & - \\
CD-51 13128 & M2Ve & TIC 140045538 & - \\
2MASS J19183060+4153031 & M3 & TIC 122067236 & KIC 6436291 \\
{[PS78]} 219 & M3+ & TIC 11652986 & - \\
UCAC4 698-065839 & M3.0 & TIC 48504458 & KIC 11495571 \\
G 9-11 & M3.0V & TIC 21246336 & - \\
UCAC4 673-078334 & M3.0Ve & TIC 272272592 & KIC 8507979 \\
G 209-3 & M3.4 & TIC 28231379 & KIC 10877432 \\
V* LT Tau & M3.5 & TIC 258067389 & - \\
BD-15 6290 & M3.5V & TIC 188580272 & - \\
LP 426-35 & M3.5V & TIC 197247983 & - \\
LP 737-14 & M3.5V & TIC 335628483 & - \\
2MASS J22371494-2622332 & M3.5Ve & TIC 326446019 & - \\
BD+16 2708 & M3V & TIC 258105174 & - \\
KOI-256 & M3V & TIC 48528261 & KIC 11548140 \\
LAMOST J192817.82+410412.2 & M3V & TIC 137410897 & KIC 5791720 \\
2MASS J18535530+4310389 & M3Ve & TIC 164529625 & KIC 7505644 \\
2MASS J18592696+4548446 & M3Ve & TIC 164784762 & KIC 9328653 \\
2MASS J19015564+4134218 & M3Ve & TIC 120576760 & KIC 6187812 \\
CD-43 9546 & M3Ve & TIC 334524122 & - \\
CD-56 1032A & M3Ve & TIC 220433363 & - \\
2MASS J04534379-5836247 & M3e & TIC 220432563 & - \\
2MASS J22534969-1721358 & M4 & TIC 188586529 & - \\
LP 873-37 & M4 & TIC 99566892 & - \\
1RXS J185504.7+425952 & M4.0V & TIC 164644375 & KIC 7341653 \\
HG 8-80 & M4.0V & TIC 435916078 & - \\
V* EV Lac & M4.0Ve & TIC 154101678 & - \\
2MASS J01275875-6032243 & M4.2 & TIC 237910557 & - \\
2MASS J19150930+5101139 & M4.5V & TIC 299089441 & KIC 12302994 \\
2MASS J19573917+4554182 & M4.5V & TIC 268711231 & KIC 9426508 \\
G 6-7 & M4.5V & TIC 456938518 & - \\
UCAC4 683-069625 & M4.5V & TIC 159171299 & KIC 9705079 \\
2MASS J18432784+4727325 & M4Ve & TIC 123205792 & KIC 10318386 \\
2MASS J18474286+4218039 & M4Ve & TIC 123408865 & KIC 6837702 \\
2MASS J18535193+4327449 & M4Ve & TIC 164529313 & KIC 7734382 \\
2MASS J19005766+4428279 & M4Ve & TIC 164889852 & KIC 8416220 \\
2MASS J19045588+3738361 & M4Ve & TIC 120825083 & KIC 2283749 \\
CD-56 1032B & M4Ve & TIC 220433364 & - \\
Kepler-1646 & M4Ve & TIC 158552258 & KIC 7350067 \\
2MASS J21484123-4736506 & M5 & TIC 147421845 & - \\
UCAC3 53-724 & M5.5V & TIC 425937691 & - \\
G 205-40 & M5V & TIC 164458193 & KIC 9201463 \\
LP 357-206 & M5e & TIC 14079970 & - \\
LP 760-3 & M6.5V & - & - \\
2MASS J19202351+5037161 & M6Ve & TIC 267746625 & KIC 12108566 \\
V* V692 Tau & M: & TIC 149923415 & - \\
\end{longtable}
}
{
\centering
\tabcolsep=8pt
\label{apA:list_of_k_stars}
\begin{longtable}{llll}
\caption{Table containing all stars used in this study of spectral type K. 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.} \\
\hline\hline
\multicolumn{1}{c}{Main Identifier} & \multicolumn{1}{c}{Spectral Type} & \multicolumn{1}{c}{TIC} & \multicolumn{1}{c}{KIC} \\
\hline
7943602 & 357 & 20 & Y & 2.3-3.4 \\
7377422 & 56 & 20 & Y & 3.7-4.8\\
3955867 & 845 & 20-23 & Y & 2.6-3.7\\
9291629 & 692 & 20-23 & Y & 2.3-3.4 \\
5179609 & 28 & 23 & Y & 4.7-5.8 \\
9163796 & 906 & 23 & Y & 3.8-4.9 \\
8430105 & 65 & 23-26 & Y & 4.4-5.5 \\
5308778 & 505 & 12 & Y & 3.0-4.1\\
4569590 & 2285 & 12 & Y & 2.4-3.5\\
8702921 & 12 & 12 & N & 4.2-5.3\\
9246715 & 101 & 14 & Y & 4.1-5.2 \\
\endfirsthead
\hline\hline
\multicolumn{1}{c}{Main Identifier} & \multicolumn{1}{c}{Spectral Type} & \multicolumn{1}{c}{TIC} & \multicolumn{1}{c}{KIC} \\
\hline
\end{tabular}\hfill~
\end{table}
\endhead
\hline
\endfoot
\hline\hline
\endlastfoot
1RXS J064643.6-770027 & K & TIC 177255827 & - \\
2MASS J18524052+4156057 & K & - & KIC 6500181 \\
2MASS J18534407+4208274 & K & - & KIC 6668646 \\
2MASS J18535462+4135227 & K & - & KIC 6183672 \\
2MASS J19004200+3903124 & K & TIC 399794444 & KIC 3935803 \\
2MASS J19082791+4337114 & K & TIC 158389986 & KIC 7879384 \\
2MASS J19324909+4229041 & K & TIC 275495685 & KIC 6953069 \\
2MASS J19404949+5046469 & K & TIC 27398219 & KIC 12166457 \\
ATO J296.1841+42.6311 & K & TIC 272184059 & KIC 7133807 \\
CPD-19 878 & K & TIC 93125144 & - \\
KOI-7449 & K & TIC 279918401 & KIC 11495989 \\
KOI-8047 & K & TIC 290034561 & KIC 11294822 \\
Kepler-1259 & K & TIC 273592350 & KIC 10028535 \\
Kepler-1782 & K & TIC 123202646 & KIC 8142942 \\
Kepler-1856 & K & TIC 27687265 & KIC 12469800 \\
Kepler-1966 & K & TIC 137627194 & KIC 5962262 \\
Kepler-246 & K & TIC 272484980 & KIC 7134976 \\
Kepler-693 & K & TIC 237159318 & KIC 5164255 \\
PM J07058-5848 & K & TIC 279615427 & - \\
TYC 1360-957-1 & K & TIC 247117382 & - \\
HD 245924 & K0IV & TIC 19934471 & - \\
2MASS J19200703+4335050 & K0V & TIC 159220196 & KIC 7816999 \\
BD+41 3306 & K0V & TIC 394172596 & KIC 6278762 \\
CD-26 1578 & K0V & TIC 44797824 & - \\
TYC 553-33-1 & K0V:e & TIC 405405298 & - \\
RX J1925.0+4429 & K1V & TIC 159721038 & KIC 8429280 \\
V* V4371 Sgr & K1V & TIC 151839506 & - \\
HD 215341 & K1Ve & TIC 145752454 & - \\
TYC 582-114-1 & K1Ve & TIC 344163180 & - \\
V* LQ Hya & K1Vp & TIC 46907042 & - \\
Kepler-1558 & K2 & TIC 158322085 & KIC 10000941 \\
HD 283750 & K2.5Ve & TIC 125838647 & - \\
CD-52 381 & K2V(e) & TIC 229151691 & - \\
V* V471 Tau & K2V+DA & TIC 456863710 & - \\
Kepler-411 & K3V & TIC 399954349 & KIC 11551692 \\
BD-13 6131 & K3Ve & TIC 437696706 & - \\
V* BY Dra & K4Ve+K7.5Ve & TIC 47579336 & - \\
2MASS J19400800+4923036 & K5 & TIC 27390487 & KIC 11461764 \\
V* CC Eri & K7V & TIC 142206123 & - \\
\end{longtable}
}
{
\centering
\tabcolsep=8pt
\label{apA:list_of_g_stars}
\begin{longtable}{llll}
\caption{Table containing all stars used in this study of spectral type G. 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.} \\
\hline\hline
\multicolumn{1}{c}{Main Identifier} & \multicolumn{1}{c}{Spectral Type} & \multicolumn{1}{c}{TIC} & \multicolumn{1}{c}{KIC} \\
\hline
\endfirsthead
\hline\hline
\multicolumn{1}{c}{Main Identifier} & \multicolumn{1}{c}{Spectral Type} & \multicolumn{1}{c}{TIC} & \multicolumn{1}{c}{KIC} \\
\hline
\endhead
\hline
\endfoot
\hline\hline
\endlastfoot
2MASS J18425375+4345336 & G & TIC 123198563 & KIC 7936748 \\
2MASS J18495232+4309276 & G & TIC 123489639 & KIC 7503439 \\
2MASS J18525868+4530560 & G & TIC 164458315 & KIC 9137611 \\
2MASS J18582492+4446498 & G & TIC 164779298 & KIC 8609289 \\
2MASS J19012927+4104159 & G & TIC 120496415 & KIC 5773205 \\
2MASS J19043346+4427484 & G & TIC 158171605 & KIC 8417863 \\
2MASS J19061691+4654395 & G & TIC 158272786 & KIC 10000509 \\
2MASS J19065549+3937268 & G & TIC 121012476 & KIC 4546541 \\
2MASS J19080680+4450500 & G & TIC 158391683 & KIC 8678334 \\
2MASS J19100183+4257041 & G & TIC 158552191 & KIC 7350021 \\
2MASS J19182441+4439465 & G & TIC 159097797 & KIC 8554173 \\
2MASS J19184939+4418233 & G & TIC 159107064 & KIC 8359762 \\
2MASS J19185028+4633324 & G & TIC 159171504 & KIC 9765670 \\
2MASS J19250540+3734332 & G & TIC 137097085 & KIC 2159377 \\
2MASS J19280249+3911165 & G & TIC 137402956 & KIC 4058829 \\
2MASS J19283146+3837123 & G & TIC 137484235 & KIC 3547283 \\
2MASS J19313155+4628249 & G & TIC 63452929 & KIC 9712781 \\
2MASS J19320792+3933052 & G & TIC 137972488 & KIC 4469481 \\
2MASS J19350077+4608423 & G & TIC 270698467 & KIC 9531002 \\
2MASS J19354814+4118464 & G & TIC 138431713 & KIC 6049426 \\
2MASS J19354900+4623499 & G & TIC 270789534 & KIC 9654338 \\
2MASS J19364457+4403341 & G & TIC 270859571 & KIC 8172597 \\
2MASS J19370439+4626209 & G & TIC 270957778 & KIC 9716208 \\
2MASS J19390861+4046149 & G & TIC 138725759 & KIC 5544024 \\
2MASS J19395042+4622296 & G & TIC 271354512 & KIC 9657062 \\
2MASS J19415575+4522369 & G & TIC 271664690 & KIC 9032578 \\
2MASS J19450785+5108395 & G & TIC 27778260 & KIC 12367153 \\
2MASS J19484658+5002007 & G & TIC 28084005 & KIC 11825619 \\
2MASS J19491761+4638356 & G & TIC 273131067 & KIC 9845711 \\
2MASS J19535154+4211197 & G & TIC 274119294 & KIC 6719122 \\
2MASS J19551628+4145582 & G & TIC 171093514 & KIC 6390935 \\
2MASS J19553242+4737586 & G & TIC 268382866 & KIC 10491422 \\
2MASS J19562459+4408276 & G & TIC 268606798 & KIC 8257716 \\
2MASS J19572618+4520510 & G & TIC 268712881 & KIC 9048032 \\
2MASS J19583564+4352320 & G & TIC 269121724 & KIC 8055957 \\
2MASS J20060991+4417004 & G & TIC 185335830 & KIC 8332459 \\
ATO J285.5682+44.5725 & G & TIC 352012409 & KIC 8481574 \\
BD-08 995 & G & TIC 43472154 & - \\
KOI-1747 & G & TIC 159717069 & KIC 7032421 \\
KOI-2324 & G & TIC 159105557 & KIC 7746958 \\
KOI-5796 & G & TIC 63070665 & KIC 10470779 \\
KOI-5810 & G & TIC 123494489 & KIC 10581308 \\
KOI-5825 & G & TIC 27183790 & KIC 10737437 \\
KOI-5952 & G & TIC 27845077 & KIC 12071775 \\
KOI-741 & G & TIC 272840512 & KIC 10418797 \\
Kepler-1060 & G & TIC 120691237 & KIC 4544907 \\
Kepler-1198 & G & TIC 158843826 & KIC 8681734 \\
Kepler-1839 & G & TIC 27082730 & KIC 11818607 \\
Kepler-513 & G & TIC 48503953 & KIC 11802615 \\
Kepler-725 & G & TIC 164652841 & KIC 8672910 \\
Kepler-739 & G & TIC 159225155 & KIC 9766437 \\
TYC 4595-107-1 & G & TIC 394030788 & - \\
UCAC4 640-067417 & G & TIC 122517231 & KIC 2709412 \\
UCAC4 686-075120 & G & TIC 269030397 & KIC 10098932 \\
V* V452 Lyr & G & - & KIC 7742289 \\
BD-01 2318 & G0 & TIC 78234015 & - \\
HD 295290 & G0 & TIC 53417036 & - \\
TYC 3560-458-1 & G0 & TIC 26815845 & KIC 10922836 \\
TYC 3557-1509-1 & G0.5V & TIC 273379797 & KIC 9726613 \\
TYC 3139-951-1 & G0V & TIC 138215507 & KIC 4660797 \\
Kepler-1424 & G1.5Vb & TIC 122706631 & KIC 5096590 \\
KOI-6202 & G1V & TIC 164669854 & KIC 9389245 \\
Kepler-400 & G2V & TIC 122707140 & KIC 5272233 \\
TYC 3131-2137-1 & G2V & TIC 164460243 & KIC 7871914 \\
TYC 3146-672-1 & G2V & TIC 159448893 & KIC 7523785 \\
TYC 3545-2661-1 & G2V & TIC 399827121 & KIC 10850420 \\
HD 183473 & G5 & TIC 63120335 & KIC 7201012 \\
HD 214261 & G5 & TIC 200501090 & - \\
KOI-644 & G5 & TIC 122138452 & KIC 5356593 \\
TYC 3550-241-1 & G5 & TIC 299088815 & KIC 12008308 \\
HD 23524 & G5V & TIC 428761512 & - \\
TYC 3562-2088-1 & G5V & TIC 273872314 & KIC 10093680 \\
V* AG Lep & G5V & TIC 92845906 & - \\
HD 222259A & G6V & TIC 410214986 & - \\
Kepler-605 & G7 & TIC 158423850 & KIC 7595157 \\
TYC 3128-2312-1 & G8V & TIC 120686876 & KIC 5944209 \\
HD 180445 & G8V(e) & TIC 97914505 & - \\
HD 220186 & G9Ve & TIC 49619607 & - \\
\end{longtable}
}
{
\centering
\tabcolsep=8pt
\label{apA:list_of_f_stars}
\begin{longtable}{llll}
\caption{Table containing all stars used in this study of spectral type 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}, 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.} \\
\hline\hline
\multicolumn{1}{c}{Main Identifier} & \multicolumn{1}{c}{Spectral Type} & \multicolumn{1}{c}{TIC} & \multicolumn{1}{c}{KIC} \\
\hline
\endfirsthead
\hline\hline
\multicolumn{1}{c}{Main Identifier} & \multicolumn{1}{c}{Spectral Type} & \multicolumn{1}{c}{TIC} & \multicolumn{1}{c}{KIC} \\
\hline
\endhead
\hline
\endfoot
\hline\hline
\endlastfoot
2MASS J18491671+4410445 & F & TIC 123449867 & KIC 8212826 \\
KOI-4698 & F & TIC 159643077 & KIC 10663738 \\
Kepler-1271 & F & TIC 120825510 & KIC 1996180 \\
Kepler-1443 & F & TIC 164525743 & KIC 10057494 \\
Kepler-380 & F & TIC 48132154 & KIC 11121752 \\
Kepler-494 & F & TIC 169176556 & KIC 6305192 \\
TYC 3134-301-1 & F & TIC 137483286 & KIC 3852772 \\
KOI-19 & F3/F5V & TIC 123201406 & KIC 7255336 \\
TYC 3557-727-1 & F3/F5V & TIC 273684688 & KIC 9788113 \\
TYC 3140-1658-1 & F5 & TIC 138967825 & KIC 5802601 \\
TYC 3557-1501-1 & F6IV & TIC 273043859 & KIC 9724820 \\
KOI-44 & F7IV & TIC 239276046 & KIC 8845026 \\
Kepler-1084 & F8V & TIC 267749737 & KIC 10857519 \\
\end{longtable}
}
Physics_Thesis_Template/content/appendixB.tex
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@@ -18,6 +18,7 @@ The top panel reports the standard python packages, contained in the standard py
(Modified table based on Table A.1 from Rafael Goldgruber's Bachelor thesis).
\begin{table}[h!]
%{\centering
\vspace{3mm}
Physics_Thesis_Template/content/chapter-data.tex
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\chapter{Data and Methods}
\label{sec:data}
In this chapter the selection criteria for the data is explained is section \ref{sec:data:data_selection}. Furthermore a detailed description of the algorithm is given in section \ref{sec:data:data_reduction}.
In this chapter the selection criteria for the data is explained in section \ref{sec:data:data_selection}. Furthermore a detailed description of the algorithm is given in section \ref{sec:data:data_reduction}.
\section{Data selection}
\label{sec:data:data_selection}
@@ -14,6 +14,9 @@ In this chapter the selection criteria for the data is explained is section \ref
\label{sec:data:data_reduction}
\section{Spectral type identification}
\label{sec:data:sptype_identification}
\begin{table}[tp!]
\caption{Training sample of false-positive planet candidates for the clustering algorithm.}
\tabcolsep=6.5pt %use this macro to add some regular space between lines (or squeeze it)
Physics_Thesis_Template/content/chapter-results.tex
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\chapter{Results \label{sec:results}}
This chapter includes the main results of this study. The data for the plots were generated using the "New FC" Button from the main GUI described in section \ref{sec:gui:data_processing}.
The results are first split into the overall results for the different spectral types M, K, G, and F as well as combined results over all analyzed spectral types. Furthermore there is a selection of individual star results.
The results also only contain the data of folded lightcurves which could be fitted with a sine function and less than 30 iterations of the fold optimization. The data which uses polynomial fits or both sine and polynomial fits is available at \href{https://drive.google.com/drive/folders/1L_F21W3WwZicVZg9052B12B2hJNuJBwK?usp=drive_link}{google drive}.
The results contain plots for the different spectral types M, K, G, and F as well as combined results of every possible combination. Additionally for all these possible combinations, plots with data limits, e.g. only stars with a rotational period of less than 2 days or minimal/maximal normalized flare peak limits, were also generated. Additionally plots for stars with a more detailed spectral type like M0 or G5 were created. Furthermore there is a selection of individual star results. For every plot group a CSV file is generated, which contains information about every star and flare used to generate the plot.
The results also only contain the data of folded lightcurves which could be fitted with a sine function and less than 30 iterations of the fold optimization. The data which uses polynomial fits or both sine and polynomial fits as well as all plots and the accompanying CSV files are available at \href{https://drive.google.com/drive/folders/1L_F21W3WwZicVZg9052B12B2hJNuJBwK?usp=drive_link}{google drive}.
\section{M dwarfs \label{sec:results:m_dwarfs}}
This section shows the results for all M dwarfs in this study.\\
Figures \ref{fig:M-Flarecount-10_Bins} and \ref{fig:M-Flarecount-30_Bins} show histograms, with 10 and 30 bins respectively, of the amount of flares during the normalized phase. Looking at figure \ref{fig:M-Flarecount-10_Bins} there is a rather even distribution across the whole phase, except at $0.5 \pi$. There is a clear dip in the amount of flares happening visible.\\
Looking at the same data, just with 30 bins (figure \ref{fig:M-Flarecount-30_Bins}), the same dip is visible. Additionally there also seem to be a dip at phase $1.5 \pi$.
This section shows the results for all 144 M dwarfs in this study. The list of stars can be found in table \ref{apA:list_of_m_stars}.\\
Figures \ref{fig:M-Flarecount-10_Bins} and \ref{fig:M-Flarecount-30_Bins} show histograms, with 10 and 30 bins respectively, of the amount of flares during the normalized phase.\\
Looking at figure \ref{fig:M-Flarecount-10_Bins} there is an even distribution within error of flares across the normalized phase, with the excepion of the bin at phase $0.5 \pi$. The bin at phase $0.5 \pi$ shows a significant dip of roughly twice the error bar below the surrounding bins.\\
Looking at the same data, just with 30 instead of 10 bins (figure \ref{fig:M-Flarecount-30_Bins}), the same dip is visible. In this figure the dip spans 3 bins. Additionally there are additional dips at around phase $0.7 \pi$, $1.3 \pi$ and $1.4 \pi$. Including the error, the major dip (which was already visible in figure \ref{fig:M-Flarecount-10_Bins}) is still below the average. Similar for the dips at phases $0.7 \pi$ and $1.3 \pi$. The dip at phase $1.4 \pi$ on the other hand overlaps with its error with the error the average flare amount.
The error bars in this figure appear larger because the individual values per bin is lower. Additionally there also seem to be a dip at phase $1.5 \pi$.
\begin{figure}[pt!]
\includegraphics[width=\linewidth]{plots/sine/M/M-Flarecount-10_Bins.png}
\caption{Histogram of all M dwarfs with 10 bins across the phase showing the number of flares in each bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase, with the minimum at phase $1 \pi$.}
\caption{Histogram showing the amount of flares 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 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-10_Bins}
\end{figure}
\begin{figure}[pt!]
\includegraphics[width=\linewidth]{plots/sine/M/M-Flarecount-30_Bins.png}
\caption{Histogram of all M dwarfs with 30 bins across the phase showing the number of flares in each bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase, with the minimum at phase $1 \pi$.}
\caption{Histogram showing the amount of flares per phase for all 144 M dwarfs used in this study. The x-axis represents the normalized phase of the folded lightcurves. There are 30 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-30_Bins}
\end{figure}
@@ -26,25 +28,25 @@ Filtering the data by the minimal flare peak (see figures \ref{fig:M-Flarecount-
\begin{figure}[pt!]
\includegraphics[width=\linewidth]{plots/sine/M/M_minFlarePeak_1.25-Flarecount-10_Bins.png}
\caption{Histogram of all M dwarfs with 10 bins across the phase showing the number of flares with normalized peak above 1.25 in each bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase, with the minimum at phase $1 \pi$.}
\caption{Histogram 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 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-10_Bins_1.25_peak}
\end{figure}
\begin{figure}[pt!]
\includegraphics[width=\linewidth]{plots/sine/M/M_minFlarePeak_1.25-Flarecount-30_Bins.png}
\caption{Histogram of all M dwarfs with 30 bins across the phase showing the number of flares with normalized peak above 1.25 in each bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase, with the minimum at phase $1 \pi$.}
\caption{Histogram 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 30 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-30_Bins_1.25_peak}
\end{figure}
\begin{figure}[pt!]
\includegraphics[width=\linewidth]{plots/sine/M/M_minFlarePeak_1.5-Flarecount-10_Bins.png}
\caption{Histogram of all M dwarfs with 10 bins across the phase showing the number of flares with normalized peak above 1.5 in each bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase, with the minimum at phase $1 \pi$.}
\caption{Histogram 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 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-10_Bins_1.5_peak}
\end{figure}
\begin{figure}[pt!]
\includegraphics[width=\linewidth]{plots/sine/M/M_minFlarePeak_1.5-Flarecount-30_Bins.png}
\caption{Histogram of all M dwarfs with 30 bins across the phase showing the number of flares with normalized peak above 1.5 in each bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase, with the minimum at phase $1 \pi$.}
\caption{Histogram 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 30 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-30_Bins_1.5_peak}
\end{figure}
@@ -57,13 +59,13 @@ Looking at the same dataset with 30 bins for the histogram (figure \ref{fig:K-Fl
\begin{figure}[pt!]
\includegraphics[width=\linewidth]{plots/sine/K/K-Flarecount-10_Bins.png}
\caption{Histogram of all K dwarfs with 10 bins across the phase showing the number of flares in each bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase, with the minimum at phase $1 \pi$.}
\caption{Histogram showing the amount of flares 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 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-10_Bins}
\end{figure}
\begin{figure}[pt!]
\includegraphics[width=\linewidth]{plots/sine/K/K-Flarecount-30_Bins.png}
\caption{Histogram of all K dwarfs with 30 bins across the phase showing the number of flares in each bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase, with the minimum at phase $1 \pi$.}
\caption{Histogram showing the amount of flares per phase for all 37 K dwarfs used in this study. The x-axis represents the normalized phase of the folded lightcurves. There are 30 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-30_Bins}
\end{figure}
@@ -76,13 +78,13 @@ Due to the lower number of detected flares on G type stars, the error bars in fi
\begin{figure}[pt!]
\includegraphics[width=\linewidth]{plots/sine/G/G-Flarecount-10_Bins.png}
\caption{Histogram of all G dwarfs with 10 bins across the phase showing the number of flares in each bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase, with the minimum at phase $1 \pi$.}
\caption{Histogram showing the amount of flares 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 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-10_Bins}
\end{figure}
\begin{figure}[pt!]
\includegraphics[width=\linewidth]{plots/sine/G/G-Flarecount-30_Bins.png}
\caption{Histogram of all G dwarfs with 30 bins across the phase showing the number of flares in each bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase, with the minimum at phase $1 \pi$.}
\caption{Histogram showing the amount of flares per phase for all 71 G dwarfs used in this study. The x-axis represents the normalized phase of the folded lightcurves. There are 30 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-30_Bins}
\end{figure}
@@ -94,13 +96,13 @@ Due to the low number of F type stars in this study, and the difficulty to detec
\begin{figure}[pt!]
\includegraphics[width=\linewidth]{plots/sine/F/F-Flarecount-10_Bins.png}
\caption{Histogram of all F dwarfs with 10 bins across the phase showing the number of flares in each bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase, with the minimum at phase $1 \pi$.}
\caption{Histogram showing the amount of flares per phase for all 13 F dwarfs used in this study. The x-axis represents the normalized phase of the folded lightcurves. There are 10 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:F-Flarecount-10_Bins}
\end{figure}
\begin{figure}[pt!]
\includegraphics[width=\linewidth]{plots/sine/F/F-Flarecount-30_Bins.png}
\caption{Histogram of all F dwarfs with 30 bins across the phase showing the number of flares in each bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase, with the minimum at phase $1 \pi$.}
\caption{Histogram showing the amount of flares per phase for all 13 F dwarfs used in this study. The x-axis represents the normalized phase of the folded lightcurves. There are 10 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:F-Flarecount-30_Bins}
\end{figure}
@@ -112,13 +114,13 @@ Looking at the same data with 30 bins over the phase in figure \ref{fig:MKGF-Fla
\begin{figure}[pt!]
\includegraphics[width=\linewidth]{plots/sine/MKGF-Flarecount-10_Bins.png}
\caption{Histogram of all dwarfs (spectral types M, K, G and F) with 10 bins across the phase showing the number of flares in each bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase, with the minimum at phase $1 \pi$.}
\caption{Histogram showing the amount of flares per phase for all 265 dwarfs used in this study. The x-axis represents the normalized phase of the folded lightcurves. There are 10 bins of the phase, showing the number of flares per bin. The colors show the individual amount for each spectral type with the amount being stacked ontop of each other. 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:MKGF-Flarecount-10_Bins}
\end{figure}
\begin{figure}[pt!]
\includegraphics[width=\linewidth]{plots/sine/MKGF-Flarecount-30_Bins.png}
\caption{Histogram of all dwarfs (spectral types M, K, G and F) with 30 bins across the phase showing the number of flares in each bin. The error bar shows the standard deviation for the histogram. The blue line indicates an idialized phase, with the minimum at phase $1 \pi$.}
\caption{Histogram showing the amount of flares per phase for all 265 dwarfs used in this study. The x-axis represents the normalized phase of the folded lightcurves. There are 30 bins of the phase, showing the number of flares per bin. The colors show the individual amount for each spectral type with the amount being stacked ontop of each other. 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:MKGF-Flarecount-30_Bins}
\end{figure}
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