add nawi astrophysics template
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% !TEX root = ../thesis-example.tex
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%
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\pdfbookmark[0]{Abstract}{Abstract}
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\addcontentsline{toc}{chapter}{Abstract}
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\chapter*{Abstract}
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\label{sec:abstract}
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\vspace*{-10mm}
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%\noindent
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\physbf{Context.~}%\lipsum[1]
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\\[0.75em]
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%\noindent
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\physbf{Aims.~}%\lipsum[1]
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\\[0.75em]
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\noindent
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\physbf{Methods.~}%\lipsum[1]
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\\[0.75em]
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\noindent
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\physbf{Results.~}%\lipsum[1]
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\\[0.75em]
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\noindent
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\physbf{Conclusions.~}%\lipsum[1]
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%\vspace*{10mm}
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%\noindent
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%\physit{Keywords:~}
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%select up to six keywords from the list in Appendix A in the A&A editorial guidelines (page 11, https://www.aanda.org/doc_journal/instructions/aadoc.pdf)
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% !TEX root = ../thesis-example.tex
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%
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\pdfbookmark[0]{Acknowledgement}{Acknowledgement}
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\addcontentsline{toc}{chapter}{Acknowledgements}
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\chapter*{Acknowledgement}
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\label{sec:acknowledgement}
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\vspace*{-10mm}
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% Acknowledge infrastructure and people that supported you in your thesis. This can also cover family, friends, etc.
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I gratefully acknowledge my supervisor xxx for guiding me ... the technical team xxx, yyy, for the continuous support...
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I thank my family and friends...
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This thesis made use of the experimental setups, laboratory and technical infrastructure, general resources and observational facilities of the Institute of Physics of the University of Graz. This thesis also made use of infrastructure, which was supported by NAWI Graz.
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% you may also list missions, telescopes, data bases or code packages you have used. Copy here the predefined sentence you are requested on the project webpage to cite. Also make sure that you cite the requested papers, as mentioned in the text below.
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%
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\par
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\textit{Software:} \texttt{Python} \citep{10.5555/1593511},
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\texttt{numpy} \citep{numpy,Harris_2020},
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\texttt{matplotlib} \citep{4160265},
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\texttt{scipy} \citep{2020SciPy-NMeth},
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\texttt{pandas} \citep{reback2020pandas, mckinney-proc-scipy-2010}.
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This research made use of \texttt{astropy} \citep{astropy:2013, astropy:2018}., a community-developed core Python package for Astronomy.
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% acknowledge FUNDING that you have received as financial support
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%acknowledge sources of funding like a travel grant or a Erasmus fellowship, e.g.:
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I gratefully acknowledge the Austrian Science Fund (FWF): P30949-N36 (PI: xxx) for supporting this project.
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This work was supported with funding of the Dr. Heinrich-Jörg Foundation at the Faculty of Natural Sciences at the Karl-Franzens University of Graz.
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The authors acknowledge the support from ERASMUS+ grant number 2017-1-CZ01-KA203-035562.
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\chapter{Literature values for \Kepler systems \label{chap:appendixExtensiveTables}}
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\label{sec:appendix}
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%\section*{Authors' Note}
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%\lipsum[4]
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%\section{Literature values for \Kepler-systems}\label{sec:appendixA}
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\physit{[This appendix has been published as Appendix\,C of \cite{Beck2018}].}
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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.
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\section{Compilation of literature values}
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We refer to the cited literature for details on the applied methodology.
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\Table{tab:longTable} contains the following parameters,
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\begin{itemize}
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\item \textit{KIC} specifies the target identification number in the \Kepler Input Catalog.
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\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.
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\item P$_{\mathrm{orbit}}$ is the measured orbital period.
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\item $e$ is the orbital eccentricity.
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\item $\nu_{\mathrm{max}}$ is the peak frequency of the excess of oscillation power.
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\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.
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\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.
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\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.
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\item $T_{\mathrm{eff}}$ is the effective temperature.
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\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.
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\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 $q=0.5$.
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\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.
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\end{itemize}
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\begin{landscape}
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%\begin{able}
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\label{tab:longTable}
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\centering
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\tabcolsep=2pt
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\begin{longtable}{rrrrrrrrrrrl}
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\caption{Literature Parameters of red-giant binaries in the \Kepler sample. } \\
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\hline\hline
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\multicolumn{1}{c}{KIC} &
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\multicolumn{1}{c}{Type} &
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\multicolumn{1}{c}{P$_{\mathrm{orb}}$} &
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\multicolumn{1}{c}{$e$} &
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\multicolumn{1}{c}{$\nu_{\mathrm{max}}$} &
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\multicolumn{1}{c}{R/R$_\odot$} &
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\multicolumn{1}{c}{M/M$_\odot$} &
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\multicolumn{1}{c}{$q$} &
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\multicolumn{1}{c}{T} &
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\multicolumn{1}{c}{P$_{\mathrm{rot}}$} &
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\multicolumn{1}{c}{$\varepsilon_{\mathrm{R}}$} &
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REF \\
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& &
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\multicolumn{1}{c}{[days]} &
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\multicolumn{1}{c}{[]} &
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\multicolumn{1}{c}{[$\mu$Hz]} &
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\multicolumn{1}{c}{[]} &
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\multicolumn{1}{c}{[]} &
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\multicolumn{1}{c}{[]}&
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\multicolumn{1}{c}{[K]} &
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\multicolumn{1}{c}{[days]} &
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\multicolumn{1}{c}{[]} & \\
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\endfirsthead
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\caption{Literature Parameters of red-giant binaries in the \Kepler sample. (continued) }\\
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\hline\hline
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\multicolumn{1}{c}{KIC} &
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\multicolumn{1}{c}{Type} &
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\multicolumn{1}{c}{P$_{\mathrm{orb}}$} &
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\multicolumn{1}{c}{$e$} &
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\multicolumn{1}{c}{\numax} &
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\multicolumn{1}{c}{R/R$_\odot$} &
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\multicolumn{1}{c}{M/M$_\odot$} &
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\multicolumn{1}{c}{$q$} &
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\multicolumn{1}{c}{T} &
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\multicolumn{1}{c}{P$_{\mathrm{rot}}$} &
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\multicolumn{1}{c}{\varR} &
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REF \\
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& &
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\multicolumn{1}{c}{[days]} &
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\multicolumn{1}{c}{[]} &
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\multicolumn{1}{c}{[$\mu$Hz]} &
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\multicolumn{1}{c}{[]} &
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\multicolumn{1}{c}{[]} &
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\multicolumn{1}{c}{[]}&
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\multicolumn{1}{c}{[K]} &
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\multicolumn{1}{c}{[days]} &
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\multicolumn{1}{c}{[]} & \\
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\endhead
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\hline
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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% 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
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% 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
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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
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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
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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
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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
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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
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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
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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
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\hline
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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
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% 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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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% 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
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\hline
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\end{longtable}
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%\end{table}%
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\end{landscape}
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\section{Tidal properties of selected systems}
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Table\,\ref{tab:10th} lists the following parameters for the systems' red-giant primary with known $P_{\mathrm{rot}}$,
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\begin{itemize}
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\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)$.
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\item $\tau_{\mathrm{conv,10}}$ is the corresponding convective turnover timescale computed in the middle of the convective zone.
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\item $P_{\mathrm{tide}}$ > $\tau_{\mathrm{conv,10}}$ indicates if the tidal period is longer than the convective turnover timescale (Yes / No).
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\end{itemize}
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\vspace {5mm}
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\begin{table}[h!]
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\caption{Evolution of $\delta_{\mathrm{10}}$ for the systems with know rotation period.}
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\label{tab:10th}
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%\centering
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\tabcolsep=10pt
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\hfill\begin{tabular}{rrccc}
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\hline\hline
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\multicolumn{1}{c}{KIC} &
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\multicolumn{1}{c}{$P_{\mathrm{tide}}$} & $\tau_{\mathrm{conv,10}}$ & $P_{\mathrm{tide}}$ > $\tau_{\mathrm{conv,10}}$ & $\delta_{\mathrm{10}}$\\
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& \multicolumn{1}{c}{[days]} & [days] & & \\
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\hline
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7943602 & 357 & 20 & Y & 2.3-3.4 \\
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7377422 & 56 & 20 & Y & 3.7-4.8\\
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3955867 & 845 & 20-23 & Y & 2.6-3.7\\
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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 \\
|
||||
\hline
|
||||
\end{tabular}\hfill~
|
||||
\end{table}
|
||||
|
||||
|
||||
|
||||
@@ -0,0 +1,253 @@
|
||||
\chapter{Example for the presentation of programming code \label{chap:appendixCode}}
|
||||
|
||||
%In this section the code developed for this work is presented. Mention here the general dependencies you used in your development environment.
|
||||
%\systemDependencies{}
|
||||
|
||||
\section{System dependencies \label{sec:SystemDependencies}}
|
||||
The presented code is written for Python 3.7.
|
||||
\Table{tab:PyModules} details the used standard and specialized python packages and modules and is structured as follows.
|
||||
\begin{itemize}
|
||||
\item The package and module names are listed in the first column. Specialized modules are preceded with the abbreviation of the parent package, whose abbreviated package name is indicated in brackets.
|
||||
|
||||
\item The version number of the used library is indicate in the second column.
|
||||
|
||||
\item A brief module description is provided in the third column.
|
||||
%
|
||||
\end{itemize}
|
||||
The top panel reports the standard python packages, contained in the standard python distribution. The bottom panel lists specialized packages, which require individual download.
|
||||
(Modified table based on Table A.1 from Rafael Goldgruber's Bachelor thesis).
|
||||
|
||||
|
||||
\begin{table}[h!]
|
||||
%{\centering
|
||||
\vspace{3mm}
|
||||
\tabcolsep=8pt
|
||||
\caption{Required Python modules for the presented code.}
|
||||
\begin{tabular}{p{0.2\textwidth}
|
||||
p{0.1\textwidth}
|
||||
p{0.6\textwidth}}
|
||||
\hline\hline
|
||||
Package / Module & Version & Modul Description\\
|
||||
\hline
|
||||
math & $-$ & Access mathematical functions; \\
|
||||
os & $-$ & Miscellaneous
|
||||
operating system interfaces \\
|
||||
glob & $-$ & Creates iterable lists from folder content \\
|
||||
|
||||
matplotlib & 3.3.1 & Core package for scientific computation \& plotting \\
|
||||
numpy & 1.19.1 & Core package for numerical computing \\
|
||||
|
||||
\hline
|
||||
astropy (ap) & 4.0.1 & Community Python Library for Astronomy \\
|
||||
\textit{~~ap}.astroquery & 0.4 & Querying astronomical web databases \\
|
||||
\textit{~~ap}.vizier & 0.4 & Importing online data and catalogues, published along with papers \\
|
||||
\textit{~~ap}.io.pyfits & & Reading and operating with FITS files \\
|
||||
mesareader & $-$ & Reading MESA history and profile output files\\
|
||||
%datetime & $-$ & supplies classes for manipulating dates and times \\
|
||||
%jdcal & 1.4.1 & functions for converting between Julian dates and calendar dates \\
|
||||
%PIL & $-$ & Python Imaging Library \\
|
||||
%unicodedata & $-$ & access to the Unicode CharacterDatabase\\
|
||||
\hline
|
||||
\end{tabular}
|
||||
\label{tab:PyModules}
|
||||
|
||||
%\tablefoot{ }
|
||||
\end{table}
|
||||
|
||||
\section{Program to name new Planets \label{cod:HellowWorld}}
|
||||
|
||||
Provide a short description of the following script and give a brief description of the key settings or input format. The example below shows how to insert the code of a whole program from its source file.
|
||||
|
||||
\lstinputlisting[label=code:sampleCode,
|
||||
frame=Tb,
|
||||
caption= HelloPlanet.py: Sophisticated code to name new worlds.,
|
||||
language=python]{code/helloWorld.py}
|
||||
|
||||
|
||||
\vspace{5mm}
|
||||
\begin{table}[h!]
|
||||
\caption{Option menu for helloWorld.py (\Listing{code:sampleCode}), \label{cod:helloWorld}}
|
||||
|
||||
%\centering
|
||||
\hfill\begin{tabular}{p{0.15\textwidth}p{0.15\textwidth}p{0.6\textwidth}}
|
||||
\hline\hline
|
||||
Type & Argument & Functionality \\ \hline
|
||||
InCode & if \hbox{xY==True} & Description of what will happen if this option is used. \\
|
||||
CmdL & -n & Description of what will happen if this option is used. \\
|
||||
ReqIn & parameter name & Description of what will happen if this option is used. \\
|
||||
\hline
|
||||
\end{tabular}\hfill~
|
||||
|
||||
\tablefoot{Usage options:
|
||||
\textit{InCode} curial options to be set inside the code before excecution of the program,
|
||||
\textit{CmdL} options set in the command line,
|
||||
\textit{ReqIn} requested user input during the execution of the program;
|
||||
}
|
||||
\label{tab:functionalityTable}
|
||||
\end{table}
|
||||
|
||||
\section{Example for long code listing \label{chap:appendixMesaInlists}}
|
||||
|
||||
This section presents styles to present longer code snippets. To save printing space and cost, these are typset in a two-column format.
|
||||
|
||||
The combined presentation of \Listing{code:inlist1} and \Listing{code:inlist2} show how two snippets can be shown. \Listing{code:longListing} depicts how long code snippets or full programs can be included as multi-column and multi-page element.
|
||||
|
||||
Also for these listings a preamble stating the system requirements is needed.
|
||||
|
||||
|
||||
\begin{landscape}
|
||||
\begin{multicols}{2}
|
||||
\begin{lstlisting}[caption=inlist1 \label{code:inlist1}]
|
||||
&star_job
|
||||
show_log_description_at_start = .true.
|
||||
pgstar_flag = .true.
|
||||
/ ! end of star_job namelist
|
||||
|
||||
&controls
|
||||
extra_terminal_output_file = 'log1'
|
||||
log_directory = 'LOGS1'
|
||||
/ ! end of controls namelist
|
||||
|
||||
&pgstar
|
||||
History_Panels1_win_flag = .true.
|
||||
History_Panels1_win_width = 5
|
||||
History_Panels1_win_aspect_ratio = 1.0
|
||||
|
||||
History_Panels1_title = 'Orbital evolution'
|
||||
History_Panels1_num_panels = 2
|
||||
|
||||
History_Panels1_yaxis_name(1) = 'period_days'
|
||||
History_Panels1_other_yaxis_name(1) =
|
||||
'lg_mstar_dot_1'
|
||||
History_Panels1_yaxis_name(2) = 'Jdot'
|
||||
History_Panels1_other_yaxis_name(2) =
|
||||
'binary_separation'
|
||||
/ ! end of pgstar namelist
|
||||
|
||||
\end{lstlisting}
|
||||
%##########################################################################
|
||||
\begin{lstlisting}[caption=inlist2 \label{code:inlist2}]
|
||||
&star_job
|
||||
show_log_description_at_start = .false.
|
||||
|
||||
/ ! end of star_job namelist
|
||||
|
||||
&controls
|
||||
extra_terminal_output_file = 'log2'
|
||||
log_directory = 'LOGS2'
|
||||
/ ! end of controls namelist
|
||||
|
||||
&pgstar
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
/ ! end of pgstar namelist
|
||||
\end{lstlisting}
|
||||
\end{multicols}
|
||||
%\tablefoot{}
|
||||
% \end{table*}
|
||||
\end{landscape}
|
||||
|
||||
|
||||
\begin{landscape}
|
||||
|
||||
\begin{lstlisting}[language=Fortran,
|
||||
caption = Example for a multi-column and multi-page code listing.
|
||||
\label{code:longListing},frame=T]
|
||||
\end{lstlisting}
|
||||
\begin{lstlisting}[language=Fortran,multicols=2,frame=none]
|
||||
! inlist to evolve a 15 solar mass star
|
||||
|
||||
! For the sake of future readers of this file,
|
||||
! ONLY include the controls you are actually using.
|
||||
! DO NOT include all of the other controls that
|
||||
! simply have their default values.
|
||||
|
||||
&star_job
|
||||
|
||||
! begin with a pre-main sequence model
|
||||
create_pre_main_sequence_model = .true.
|
||||
|
||||
! save a model at the end of the run
|
||||
save_model_when_terminate = .false.
|
||||
save_model_filename = '15M_at_TAMS.mod'
|
||||
|
||||
! display on-screen plots
|
||||
pgstar_flag = .true.
|
||||
|
||||
/ !end of star_job namelist
|
||||
|
||||
|
||||
&controls
|
||||
|
||||
! starting specifications
|
||||
initial_mass = 15 ! in Msun units
|
||||
|
||||
! options for energy conservation
|
||||
use_dedt_form_of_energy_eqn = .true.
|
||||
use_gold_tolerances = .true.
|
||||
|
||||
! stop when the star nears ZAMS (Lnuc/L > 0.99)
|
||||
Lnuc_div_L_zams_limit = 0.99d0
|
||||
stop_near_zams = .true.
|
||||
|
||||
! stop when the center mass fraction
|
||||
of h1 drops below this limit
|
||||
xa_central_lower_limit_species(1) = 'h1'
|
||||
xa_central_lower_limit(1) = 1d-3
|
||||
|
||||
/ ! end of controls namelist
|
||||
|
||||
&pgstar
|
||||
|
||||
! MESA uses PGPLOT for live plotting and
|
||||
! gives the user a tremendous amount of control
|
||||
! of the presentation of the information.
|
||||
|
||||
! show HR diagram
|
||||
! this plots the history of L,Teff over many
|
||||
! timesteps
|
||||
HR_win_flag = .true.
|
||||
|
||||
! set static plot bounds
|
||||
HR_logT_min = 3.5
|
||||
HR_logT_max = 4.6
|
||||
HR_logL_min = 2.0
|
||||
HR_logL_max = 6.0
|
||||
|
||||
! set window size (aspect_ratio = height/width)
|
||||
HR_win_width = 6
|
||||
HR_win_aspect_ratio = 1.0
|
||||
|
||||
|
||||
! show temperature/density profile
|
||||
! this plots the internal structure at single
|
||||
! timestep
|
||||
TRho_Profile_win_flag = .true.
|
||||
|
||||
! add legend explaining colors
|
||||
show_TRho_Profile_legend = .true.
|
||||
|
||||
! display numerical info about the star
|
||||
show_TRho_Profile_text_info = .true.
|
||||
|
||||
! set window size (aspect_ratio = height/width)
|
||||
TRho_Profile_win_width = 8
|
||||
TRho_Profile_win_aspect_ratio = 0.75
|
||||
|
||||
/ ! end of pgstar namelist
|
||||
\end{lstlisting}
|
||||
\vspace{-\baselineskip}
|
||||
\noindent\rule{\linewidth}{0.4pt}
|
||||
|
||||
\end{landscape}
|
||||
@@ -0,0 +1,39 @@
|
||||
\chapter{Glossar Englisch-Deutsch
|
||||
\label{sec:glossar}}
|
||||
|
||||
Zur Besseren Übersicht ist hier ein Glossar der deutschsprachigen Übersetzungen der Fachbegriffe aus der Literatur gegeben.
|
||||
Ebenso sind die hierbei verwendeten und in der Literatur gebräuchlichen Abkürzungen der Fachbegriffe in der Literatur angeführt.
|
||||
|
||||
\vspace{5mm}
|
||||
|
||||
{\centering
|
||||
% \begin{landscape}
|
||||
\begin{table}[h!]
|
||||
\caption{Glossar der häufig verwendeten Begriffe auf Englisch mit ihrer deutschen Übersetzung und ihrer verwendeten Abkürzung.}
|
||||
\label{tab:glossar}
|
||||
\tabcolsep=10pt
|
||||
\hfill
|
||||
|
||||
\begin{tabular}{lll}
|
||||
|
||||
\hline\hline
|
||||
\multicolumn{1}{c}{Abkürzung} &
|
||||
\multicolumn{1}{c}{Englisch} &
|
||||
\multicolumn{1}{c}{Deutsch} \\
|
||||
|
||||
|
||||
|
||||
\hline
|
||||
EOS & equation of state & Zustandsgleichung \\
|
||||
FDU & first dredge up & maximales Durchmischungsereignis \\
|
||||
HRD & Hertzsprung-Russell diagram & Hertzsprung-Russell-Diagramm \\
|
||||
MS & main sequence & Hauptreihe \\
|
||||
PMS & pre-main sequence & vor der Hauptreihe \\
|
||||
RGB & red-giant branch & Roterriesenast\\
|
||||
TRGB & tip of the red-giant branch & Spitze des Rotenriesenastes\\
|
||||
\hline
|
||||
\end{tabular} \hfill~
|
||||
\end{table}
|
||||
% \end{landscape}
|
||||
|
||||
\par}
|
||||
@@ -0,0 +1,5 @@
|
||||
|
||||
\chapter{Modeling with MESA}
|
||||
\label{sec:MESA}
|
||||
|
||||
|
||||
@@ -0,0 +1,3 @@
|
||||
\chapter{Conclusion and Outlook}
|
||||
\label{sec:conclusion}
|
||||
\lipsum[1-3]
|
||||
@@ -0,0 +1,150 @@
|
||||
% !TEX root = ../thesis-example.tex
|
||||
%
|
||||
\chapter{Methodology}
|
||||
\label{sec:data}
|
||||
\lipsum[1]
|
||||
|
||||
\section{This is a section}
|
||||
\lipsum[2-4]
|
||||
|
||||
\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)
|
||||
\hfill\begin{tabular}{l r r r l}
|
||||
\hline
|
||||
\hline
|
||||
Star's identifier&
|
||||
\multicolumn{1}{c}{$T_{\mathrm{eff}}$} &
|
||||
\multicolumn{1}{c}{Lum} &
|
||||
\multicolumn{1}{l}{Luminosity} &
|
||||
Reference \\
|
||||
|
||||
&
|
||||
\multicolumn{1}{c}{[K]} &
|
||||
\multicolumn{1}{c}{[L/L$_\odot$]} &
|
||||
\multicolumn{1}{c}{cluster}& \\[0.5ex]
|
||||
\hline
|
||||
$\pi$\,Her & 4170 & 1320 & High & \cite{Hatzes1999} \\
|
||||
$\mu$\,UMa & 3899 & 1150 & High & \cite{Lee2016} \\
|
||||
HD\,18438 & 3871 & 830 & High & \cite{Delgado2018} \\
|
||||
$\gamma$\,Dra (Eltanin) & 3990 & 510 & High & \cite{Hatzes2018} \\
|
||||
$\alpha$\,Tau (Aldebaran) & 4055 & 440 & High & \cite{Hatzes2015} \\
|
||||
\hline
|
||||
$\theta^1$\,Tau & 5000 & 70 & Low & \cite{Beck2015} \\
|
||||
NGC2423\,No.3 & 4592 & 65 & Low &\cite{Delgado2018} \\
|
||||
$\gamma$\,Psc & 4909 & 60 & Low & \cite{Beck2015} \\
|
||||
$\beta$\,Gem (Pollux) & 4865 & 40 & Low & \cite{Delgado2018} \\
|
||||
IC4651\,No.9122 & 4720 & 35 & Low & \cite{Delgado2018} \\
|
||||
$\gamma$ Cep A & 4900 & 10 & Low & \cite{Hatzes1999} \\
|
||||
\hline
|
||||
\end{tabular} \hfill~
|
||||
\label{tab:false_positives}
|
||||
% an empty line should be left between the tabular body and the table foot to avoid formating problems.
|
||||
|
||||
\tablefoot{The star's identifier is given. For the most prominent stars, the name of the star is amended in brackets. The next columns report on the effective temperature and the luminosity of the star in units of the solar luminosity L$_\odot$. The typical uncertainty of the reported temperature and luminosity are 150K and $\sim$10\%, respectively. The top and bottom panel report classification of the clustering. The cluster name refers to the position in the red-giant phase. The literature references are provided in the last column. (Table taken from Elisabeth Höldrich bachelor thesis, 2020)}
|
||||
\end{table}
|
||||
|
||||
\lipsum[4]
|
||||
|
||||
\subsection{This is a subsection}
|
||||
\lipsum[4]
|
||||
|
||||
\section{Example of a code snippet \label{sec:MESA:Inlists}}
|
||||
\lipsum[1]
|
||||
|
||||
|
||||
\begin{table}[tp]
|
||||
\begin{lstlisting}[language=Fortran,frame=Tb,
|
||||
caption= Example for setting the tidal mechanisms in the \textit{star\_star} inlist.
|
||||
\label{code:tidalSettings}]{Name}
|
||||
&binary_controls
|
||||
do_tidal_circ = .true.
|
||||
circ_type_1 = 'Hut_conv'
|
||||
circ_type_2 = 'Hut_conv'
|
||||
|
||||
do_tidal_sync = .false.
|
||||
sync_type_1 = 'Hut_conv'
|
||||
sync_type_2 = 'Hut_conv'
|
||||
\end{lstlisting}
|
||||
\tablefoot{A part of \textit{\&binary\_controls} environment in the \textit{star\_inlist} is shown.
|
||||
The true/false-statements in line 2 and 6 determine if the models defined below takes into account the defined mechanism.
|
||||
The keywords for defining the formalistic description for circularization and synchronization mechanism are defined in lines 2-4 and 6-8, respectively. The number at the end of the keyword indicates which formalism is set for the primary (1) and secondary (2) stellar component.}
|
||||
\end{table}
|
||||
|
||||
|
||||
\lipsum[2-3]
|
||||
|
||||
|
||||
\begin{figure}[pt!]
|
||||
\includegraphics[width=\linewidth]{gfx/spectralSegmentDisentanlging.pdf}
|
||||
\caption{Disentangled spectra of KIC 9163796. The spectra of the primary in blue and secondary in red are shown in the left and right spectrum,
|
||||
respectively. Top panel: the region around the H\textbeta line, while bottom panel: magnesium triplet at 518 nm, normalised to the continuum flux of the
|
||||
composite spectrum. The synthetic model of the best fit of the determination of fundamental parameters and metallicity is shown as dashed grey
|
||||
line is shown depicted in the region of the Mg triplet. \citep[Graphic taken from][]{Beck2018}}
|
||||
\label{fig:multiPanelPlot}
|
||||
\end{figure}
|
||||
|
||||
\lipsum[3]
|
||||
|
||||
|
||||
\begin{landscape}
|
||||
\begin{table}[tp!]
|
||||
\caption{
|
||||
Seismic and fundamental parameters for 14 oscillating red giant heartbeat stars, ordered by descending orbital period.}
|
||||
\tabcolsep=5pt
|
||||
\hfill\begin{tabular}{c|rrrrrrrrrrrrrrrrrrr}
|
||||
\hline \hline
|
||||
\multicolumn{1}{c}{Star} & \multicolumn{1}{c}{$\nu_{\mathrm{max}}$} &
|
||||
\multicolumn{1}{c}{$\Delta\nu$} & \multicolumn{1}{c}{$\Delta\Pi_1$} &
|
||||
\multicolumn{1}{c}{$\delta f_{\mathrm{max}}$} & \multicolumn{1}{c}{Evol.} &
|
||||
\multicolumn{1}{c}{R} &
|
||||
\multicolumn{1}{c}{M} &
|
||||
\multicolumn{1}{c}{$\log g$} &
|
||||
\multicolumn{1}{c}{L} &
|
||||
\multicolumn{1}{c}{T$_{\mathrm{eff}}$} &
|
||||
\multicolumn{1}{c}{$P_{\mathrm{orbit}}$} &
|
||||
\multicolumn{1}{c}{A} &
|
||||
\multicolumn{1}{c}{$| \Delta $RV$|$} \\
|
||||
\multicolumn{1}{c}{KIC} &
|
||||
\multicolumn{1}{c}{ [$\mu$Hz]} &
|
||||
\multicolumn{1}{c}{ [$\mu$Hz]} &
|
||||
\multicolumn{1}{c}{ [sec]} &
|
||||
\multicolumn{1}{c}{ [nHz]} &
|
||||
\multicolumn{1}{c}{Phase} &
|
||||
\multicolumn{1}{c}{ [$R_\odot$]} &
|
||||
\multicolumn{1}{c}{ [$M_\odot$]} &
|
||||
\multicolumn{1}{c}{ [dex]} &
|
||||
\multicolumn{1}{c}{ [L$_\odot$]} &
|
||||
\multicolumn{1}{c}{ [K]} &
|
||||
\multicolumn{1}{c}{ [d]} &
|
||||
\multicolumn{1}{c}{ [ppt]} &
|
||||
\multicolumn{1}{c}{ [km\,s$^{-1}$]}
|
||||
\\\hline
|
||||
|
||||
\hline
|
||||
{9151763} & 13.8$\pm$0.2 & 1.98$\pm$0.01 & $-$ & $-$ & RGB? & 17.6$\pm$0.4 & 1.19$\pm$0.08 & 2.01 & 96$\pm$16 & 4290 & 437.5 & +7.1 & 32.2\\
|
||||
{7431665} &54.0$\pm$0.7 & 5.46$\pm$0.02& $\sim$67 & $-$ & RGB & 9.4$\pm$0.1 & 1.39$\pm$0.05 & 2.62 & 35$\pm$2 & 4580 & 281.4&-3.0 &[37.8]\\
|
||||
{5039392} & 6.2$\pm$0.1 & 1.13$\pm$0.01 & $-$ & $-$ & RGB & 24.0$\pm$0.7 & 0.98$\pm$0.07 & 1.67 & 157$\pm$24 & 4110& 236.7 & -6.0 &42.3\\
|
||||
{9540226}$^\star$ & 27.4$\pm$0.4 & 3.18$\pm$0.01 & $-$ & $-$ & RGB & 14.1$\pm$0.3 & 1.6$\pm$0.1 & 2.37 & 81$\pm$13 & 4600 & 175.4 & -7 & 45.3\\
|
||||
{8210370} &44.1$\pm$0.8 & 4.69$\pm$0.02 & $-$ & $-$ & RGB? & 10.5$\pm$0.2 & 1.40$\pm$0.08 & 2.54 & 44$\pm$4 & 4585 & 153.5 & -5.3 & 22.1\\
|
||||
{11044668}&50.2$\pm$0.2 & 5.65$\pm$0.01 & $\sim$60 & 83(?) & RGB & 8.18$\pm$0.09 & 0.99$\pm$0.03 & 2.59 & 26$\pm$3 & 4565 & 139.5 & -3.8& [43.0]\\
|
||||
{10614012$^\star$}&70.2$\pm$0.9 & 6.54$\pm$0.02 & $-$ & $-$& RGB & 8.6$\pm$0.2& 1.49$\pm$0.08 & 2.74 & 33$\pm$4 & 4715 & 132.1 & -4.7 & 49.3\\
|
||||
{9163796} &153.2$\pm$0.7& 13.53$\pm$0.04 & $-$ & $-$& RGB & 4.46$\pm$0.03 & 0.89$\pm$0.01 & 3.09 & 12$\pm$1 & 4820 & 121.3 &$\pm$0.5& 70.1 \\
|
||||
{2444348} & 30.5$\pm$0.3& 3.26$\pm$0.01 & $-$ & $-$ & RGB & 14.9$\pm$0.3 &1.94$\pm$0.11 & 2.38 & 86$\pm$14 & 4565 & 103.5 & -1.7 & 7.7\\
|
||||
\textbf{5006817}& 145.9$\pm$0.5 & 11.64$\pm$0.01 & 78 & 450 & RGB & 5.84$\pm$0.09 & 1.49$\pm$0.06 & 3.08 & 19$\pm$3 & 5000 & 94.8 & -1.7& 23.5\\
|
||||
8803882 & 347$\pm$3& 22.6$\pm$0.4& $-$ & 500(?) & RGB & 3.68$\pm$0.1 & 1.4$\pm$0.1 & 3.45& 8$\pm$1& 5043 & 89.7 & +0.5 & [1.9]\\
|
||||
{8144355} & 179$\pm$2& 13.95$\pm$0.04 & $\sim$78 & 210(?)& RGB & 4.90$\pm$0.09 & 1.26$\pm$0.08 &3.16 & 12$\pm$2 & 4875& 80.6 & +2.1 & 18.9\\
|
||||
{9408183} & 164.8$\pm$0.2& 13.29$\pm$0.02 & $\sim$93 & 450 & RGB & 5.02$\pm$0.07 & 1.23$\pm$0.05 & 3.12 & 13$\pm$1 & 4900 & 49.7 & +1.5& 64.4\\
|
||||
{2720096} & 110.1$\pm$0.7& 9.17$\pm$0.01 & $-$ & $-$ & RGB & 6.98$\pm$0.08 & 1.54$\pm$0.06 & 2.95 & 23$\pm$2 & 4812 & 26.7 & +1.0& 4.0 \\
|
||||
{8095275} & 69.3$\pm$0.3 & 6.81$\pm$0.01 & $-$ & $-$ & RGB & 7.78$\pm$0.08 & 1.21$\pm$0.05 & 2.74 & 25$\pm$3 & 4622 & 23.0 & -6.0 & 20.6 \\
|
||||
\hline
|
||||
\end{tabular}\hfill~
|
||||
|
||||
\label{tab:asteroseismicValues}
|
||||
|
||||
\tablefoot{The star's identifier in the \textit{Kepler} Input Catalogue (KIC) is given. Eclipsing systems are marked with an asterisk. The columns $\nu_{\mathrm{max}}$ and $\Delta\nu$ report the frequency of the oscillation power excess and the large frequency separation between radial modes for a given star. $\Delta\Pi_1$ quantifies the true period spacing of dipole modes. The maximum value of the detected rotational splitting $\delta f$ is listed. The evolutionary phase RGB describes H-shell burning red giant. Ambiguous values are marked with '?'. The columns $R$,\,$M$,\,$L$, and $\log g$ report the stellar radius, mass, luminosity, effective temperature and surface gravity from scaling relations, respectively. $T_{\mathrm{eff}}$ was adopted from the KIC. The uncertainties of $\log g$ are on the order of 0.01\,dex and for the temperature typically smaller than 150\,K. $P_{\mathrm{orbit}}$ gives the orbital period from photometry. The column $A$ lists the maximum amplitude of the heartbeat in a rebinned phase diagram. The error estimate for $P_{\mathrm{orbit}}$ and $A$ from the PDM is not reliable due to the remaining contamination of the solar-like oscillations and therefore not given. $|\Delta $RV$|$ reports the maximum difference in radial velocity. Squared brackets mark systems for which the orbital parameters could not yet be determined from radial velocities. \citep[Table taken from][]{Beck2014}}
|
||||
|
||||
\end{table}%
|
||||
\end{landscape}
|
||||
|
||||
|
||||
@@ -0,0 +1,5 @@
|
||||
\chapter{Discussion}
|
||||
\label{sec:discussion}
|
||||
|
||||
\lipsum[1-7]
|
||||
|
||||
@@ -0,0 +1,32 @@
|
||||
% !TEX root = ../thesis-example.tex
|
||||
%Example chapter on Asteroseismology
|
||||
\chapter{Introduction \label{sec:intro}}
|
||||
%\cleanchapterquote{Shoot for the moon. Even if you miss, you'll land among the stars.}{Les Brown} %optional, if you want to place something here.
|
||||
|
||||
Binary stars play a major role in astrophysics since their analysis by different means enables astronomers to deduce various stellar properties. In this thesis the binary system KIC 10614012 is analysed by combining asteroseismic techniques with radial velocity measurements and light curve analysis. This star system, also referred to as TYC 3561-1138-1, is part of the Kepler Input Catalog (KIC), a catalogue for potential target stars of the \textit{Kepler} mission. KIC 10614012 is an eclipsing binary (EB), i.e. an eclipse is visible in its light curve \citep[as written in][]{Kirk2016}. Furthermore, \cite{Beck2014} has shown that this star exhibits tidally induced flux modulations during periastron passage, on its eccentric ($e = 0.71$) orbit. Such binary stars, theorized by \citet{Kumar:1995}, are colloquially referred to as \textit{Heartbeat stars}, a term coined by \citet{Thompson2012}.
|
||||
|
||||
\begin{figure}[t!]
|
||||
\includegraphics[width=\linewidth]{gfx/rghbHRD.pdf}
|
||||
\caption{Position of the 18 red giant heartbeat stars from Tables 1 and 2 in
|
||||
the HR diagram, where the colour shows the mass of the red giant, derived from seismology. The size of the dots represents the orbital period,
|
||||
ranging between 20 and 438 d. The contour surfaces reflect the density
|
||||
distribution of 1000 pulsating red giants. The darkest areas mark the
|
||||
position of the densely populated red clump. Numbers in red indicate
|
||||
the star count per bin, for which the contour surfaces have been drawn.
|
||||
Lines of equal radii in the HR diagram have been drawn for selected
|
||||
stellar radii between 5 and 30 R. \citep[Figure taken from][]{Beck2014}}
|
||||
\label{fig:singelPanelPlot}
|
||||
\end{figure}
|
||||
|
||||
This case study is divided into 7 sections. The first section (Sec.\,\ref{sec:intro}) gives a brief introduction into some of the underlying astrophysics of this analysis. Sec.\,\ref{sec:data} presents the three datasets used for this case study (light curves, asteroseismic power spectra and radial velocity measurements) and the instruments which obtained them (\textit{Kepler} and HERMES). The analysis of KIC 10614012 by means of asteroseismology is described in Sec.\,\ref{sec:data}, while the next chapter (Sec.\,\ref{sec:results}) deals with the system's analysis regarding its binary features. The fifth section (Sec.\,\ref{sec:results}) combines results from the previous two sections and estimates stellar properties of both, the primary and the secondary. A discussion of those results and a comparison to other studies are given in Sec.\,\ref{sec:discussion}. Eventually, in Sec.\,\ref{sec:conclusion} some conclusions are drawn, suggestions for further analysis of KIC 10614012 are given and a brief outlook on future prospects in asteroseismology is provided.
|
||||
|
||||
|
||||
Calculating the hypotenuse follows the sentence of Pythagoras,
|
||||
\begin{eqnarray}
|
||||
c^2 &=& a^2 + b^2, \label{eq:pyth1}\\
|
||||
c &=& \sqrt{a^2 + b^2} \label{eq:pyth2},
|
||||
\end{eqnarray}
|
||||
whereby $a$ and $b$ are the cathetus and $c$ the hypotenuse of a right-angled triangle. Please note that $a$ and $b$ are typically in the range of 10$^{-9}$\,$\lesssim$\,R/R$_\odot$\,$\lesssim$\,10$^6$.
|
||||
|
||||
|
||||
\lipsum[1]
|
||||
@@ -0,0 +1,4 @@
|
||||
\chapter{Results \label{sec:results}}
|
||||
|
||||
\lipsum[1-8]
|
||||
|
||||
@@ -0,0 +1,16 @@
|
||||
% !TEX root = ../thesis-example.tex
|
||||
%
|
||||
|
||||
\pagestyle{empty}
|
||||
\hfill
|
||||
\vfill
|
||||
\pdfbookmark[0]{Colophon}{Colophon}
|
||||
\section*{Colophon}
|
||||
% The text of the colophon should be included in the thesis as such and not be altered.
|
||||
|
||||
This thesis was typeset with \LaTeXe.
|
||||
It uses the \textit{Clean Thesis} style developed by Ricardo Langner, available at \href{http://cleanthesis.der-ric.de/}{http://cleanthesis.der-ric.de/}. The design of the \textit{Clean Thesis} style is inspired by user guide documents from Apple Inc.
|
||||
|
||||
|
||||
The template is provided in this adapted version by {Desmond Grossmann,\,BSc, Stefan Janisch,\,BSc, Lea Schimak and Paul Beck,\,PhD} to implement the editorial guidelines of \textit{Astronomy \& Astrophysics} and the cooperate-identity guidelines of the University of Graz for the Institute for Physics. Version: March, 2024.
|
||||
|
||||
@@ -0,0 +1,177 @@
|
||||
% --- LaTeX CV Template - S. Venkatraman ---
|
||||
\pdfbookmark[0]{Curriculum vitae}{Curriculum Vitae}
|
||||
\addcontentsline{toc}{chapter}{Curriculum Vitae}
|
||||
\chapter*{Curriculum Vitae\\Mag. Nikolaus Copernicus, PhD}
|
||||
\chaptermark{}
|
||||
|
||||
\label{sec:cv}
|
||||
%\subsection*{Bibliographic information and overview}
|
||||
\begin{table}[h!]
|
||||
%\hline\hline
|
||||
\begin{tabular}{p{0.25\textwidth}p{0.75\textwidth}}
|
||||
\physnormal{Born} &
|
||||
February 19, 1473 \\%[0.5em]
|
||||
\physnormal{Citizenship} &
|
||||
Poland \\
|
||||
\end{tabular}\hfill~
|
||||
|
||||
\end{table}
|
||||
|
||||
|
||||
\section*{Research positions and academic education}
|
||||
%\physRules
|
||||
|
||||
\subsection*{Current academic position}
|
||||
\begin{table}[h!]
|
||||
\begin{tabular}{p{0.25\textwidth}p{0.74\textwidth}}
|
||||
\physnormal{Affilitation \& \newline academic address} &
|
||||
Institute for Physics, Karl Franzens University Graz, \newline Universitätsplatz 5/II, NAWI Graz, 8010 Graz, Austria \\
|
||||
|
||||
\smallskip \physnormal{Contact} &
|
||||
\smallskip nicolaus.copernicus@uni-graz.at \\
|
||||
|
||||
%\smallskip {Academic repository identifiers} &
|
||||
%\smallskip ORCID: xxx, \newline GitHub: xxx \\
|
||||
\end{tabular}\hfill~
|
||||
|
||||
\end{table}
|
||||
|
||||
\subsection*{Research Positions}
|
||||
\begin{longtable}{p{0.25\textwidth}p{0.74\textwidth}}
|
||||
{since March 2020} &
|
||||
Doctoral researcher at the
|
||||
Department for Astronomy, Inst. of Physics, NAWI Graz, University of Graz, Austria \\[0.5em]
|
||||
|
||||
{2019, March \newline $-$ 2020, March } &
|
||||
Pre-doctoral researcher at the
|
||||
Department for Astronomy, Inst. of Physics, NAWI Graz, University of Graz, Austria \\[0.5em]
|
||||
|
||||
|
||||
\end{longtable}
|
||||
|
||||
|
||||
\subsection*{Academic Education}
|
||||
\begin{longtable}{p{0.25\textwidth}p{0.74\textwidth}}
|
||||
|
||||
{2017, February \newline $-$ 2019, March} & University of Graz, Austria: Master of Natural Sciences in Physics (Graduation: March 32, 2019), Title of Thesis\\[0.5em]
|
||||
|
||||
{2014, October \newline $-$ 2017, February} & University of Vienna, Austria : Bachelor of Natural Sciences in Astronomy (Graduation: February, 30, 2017)\\[0.5em]
|
||||
|
||||
\end{longtable}
|
||||
\clearpage
|
||||
|
||||
\section*{Academic Recognition}
|
||||
%\physRules
|
||||
|
||||
\subsection*{Invited talks at conferences and seminars}
|
||||
\begin{itemize}
|
||||
|
||||
\item \textbf{Title of invited contribution}, title of conference or occasion, length of contribution, (date, hosting institution)
|
||||
|
||||
%\item \textbf{Title of invited contribution}, title of conference or occasion, length, (date, hosting institution)
|
||||
|
||||
%\item \textbf{Title of invited contribution}, title of conference or occasion, length, (date, hosting institution)
|
||||
|
||||
\end{itemize}
|
||||
|
||||
|
||||
\subsection*{Grants \& Awards}
|
||||
\begin{itemize}
|
||||
|
||||
\item \textbf{Name of achievement}, awarding entity or agency, (awarded amount, duration)
|
||||
|
||||
%\item \textbf{Name of achievement}, awarding agency, (awarded amount, duration)
|
||||
|
||||
%\item \textbf{Name of achievement}, awarding agency, (awarded amount, duration)
|
||||
|
||||
\end{itemize}
|
||||
|
||||
|
||||
|
||||
\subsection*{Service to the community \& memberships in academic organization}
|
||||
\begin{itemize}
|
||||
|
||||
\item \textbf{Refereeing activity for scientific journals}, give concise details
|
||||
|
||||
\item \textbf{Membership in relevant professional societies, consortia or collaborations}, give concise details
|
||||
|
||||
\item \textbf{Function in associations}, give concise details
|
||||
|
||||
\end{itemize}
|
||||
|
||||
\subsection*{Extended scientific or exchange stays}
|
||||
\begin{itemize}
|
||||
|
||||
\item Institution, program / purpose, give concise details
|
||||
|
||||
|
||||
\end{itemize}
|
||||
|
||||
\newpage
|
||||
\section*{Teaching Portfolio}%\physRules
|
||||
List here the courses you have assisted in or taught until now.
|
||||
\begin{itemize}
|
||||
|
||||
\item \textbf{Name of Course},
|
||||
(type of course: e.g. lecture, exercises, practicum, ...)
|
||||
Semester 202X,
|
||||
ECTS of the course,
|
||||
Bachelor's / Master's Curriculum,
|
||||
list your co- or lead-lecturer,
|
||||
description of your responsibilities in this course.
|
||||
|
||||
\item \textbf{Name of Course},
|
||||
(type of course: e.g. lecture, exercises, practicum, ...)
|
||||
Semester 202X,
|
||||
ECTS of the course,
|
||||
Bachelor's / Master's Curriculum,
|
||||
list your co- or lead-lecturer,
|
||||
description of your responsibilities in this course.
|
||||
|
||||
\end{itemize}
|
||||
|
||||
\physbf{Nota bene:} If you use this template for your Habilitationsschrift, replace this section by the structure and content of the teaching portfolio, as recommended\footnote{\href{https://lehrkompetenz.uni-graz.at/de/service/lehrportfolios/}{https://lehrkompetenz.uni-graz.at/de/service/lehrportfolios/}} by the \physit{Zentrum für Lehrkompetentz (ZLK) of Graz University.}
|
||||
|
||||
|
||||
\section*{Observing Portfolio}%\physRules
|
||||
|
||||
The candidate has obtained XXX nights of accumulated observing experience of at international facilities:
|
||||
\begin{itemize}
|
||||
\item Observatory name and location, telescope, technique, number of nights
|
||||
%\item Observatory name and location, telescope, technique, number of nights
|
||||
%\item Observatory name and location, telescope, technique, number of nights
|
||||
\end{itemize}
|
||||
|
||||
|
||||
|
||||
\subsection*{Proposals lead as Principle investigator}
|
||||
\begin{itemize}
|
||||
\item \textbf{Title of successful proposal},
|
||||
awarded observing time (observing semester),
|
||||
observatory, telescope \& instrument specification
|
||||
|
||||
%\item \textbf{Title of successful proposal},
|
||||
%awarded observing time (observing semester),
|
||||
%observatory, telescope \& instrument specification
|
||||
|
||||
%\item \textbf{Title of successful proposal},
|
||||
%awarded observing time (observing semester),
|
||||
%telescope \& instrument specification,
|
||||
|
||||
\end{itemize}
|
||||
|
||||
|
||||
\subsection*{Proposals contributed to as Co-investigator}
|
||||
\begin{itemize}
|
||||
|
||||
\item \textbf{Title of successful proposal},
|
||||
awarded observing time (observing semester),
|
||||
name of PI,
|
||||
observatory, telescope \& instrument specification
|
||||
|
||||
%\item \textbf{Title of successful proposal},
|
||||
%awarded observing time (observing semester),
|
||||
%name of PI,
|
||||
%observatory, telescope \& instrument specification
|
||||
|
||||
\end{itemize}
|
||||
@@ -0,0 +1,31 @@
|
||||
% !TEX root = ../thesis-example.tex
|
||||
%
|
||||
%************************************************
|
||||
% Declaration
|
||||
%************************************************
|
||||
\pdfbookmark[0]{Declaration}{Declaration}
|
||||
\chapter*{Declaration}
|
||||
\label{sec:declaration}
|
||||
\thispagestyle{empty}
|
||||
|
||||
% Hereby I declare that I have completed this work on my own, where not explicitly mentioned otherwise, and only used the mentioned references.
|
||||
|
||||
% TU nennt diesen Abschnitt Affidavit
|
||||
|
||||
I declare that I have authored this thesis independently, that I have not used other than the declared sources/resources, and that I have explicitly indicated all material which has been quoted either literally or by content from the sources used. The text document uploaded to UNIGRAZonline or TUGRAZonline is identical to the present master's thesis.
|
||||
|
||||
\bigskip
|
||||
|
||||
\noindent\textit{\thesisUniversityCity, \thesisDate}
|
||||
|
||||
\smallskip
|
||||
|
||||
\begin{flushright}
|
||||
\begin{minipage}{5cm}
|
||||
\rule{\textwidth}{1pt}
|
||||
\centering\thesisName
|
||||
\end{minipage}
|
||||
\end{flushright}
|
||||
|
||||
%*****************************************
|
||||
%*****************************************
|
||||
@@ -0,0 +1,53 @@
|
||||
|
||||
\pdfbookmark[0]{List of publications}{List of publications}
|
||||
\addcontentsline{toc}{chapter}{List of publications}
|
||||
\chapter*{List of Publications}
|
||||
\chaptermark{}
|
||||
|
||||
|
||||
\subsection*{Bibliographic information and overview}
|
||||
\begin{table}[h!]
|
||||
\begin{tabular}{p{0.25\textwidth}p{0.74\textwidth}}
|
||||
\physnormal{Repository \newline identifiers} &
|
||||
ORCID: xxx, \newline GitHub: xxx \\[1em]
|
||||
|
||||
\physnormal{Bibliometric \newline indicators}
|
||||
& H-index: xxx, \newline m-index: xxx \\[1em]
|
||||
|
||||
\physnormal{Publication record \newline in NASA ADS}
|
||||
& URL of your private NASA ADS library \\[2em]
|
||||
|
||||
\end{tabular}\hfill~
|
||||
|
||||
\end{table}
|
||||
|
||||
|
||||
\subsection*{Refereed journal publications}
|
||||
Published work that is available as open access through the ArXiv.org preprint server or journal policies is indicated through the abbreviation [AO].
|
||||
|
||||
|
||||
\begin{enumerate}
|
||||
|
||||
\item \physbf{Your, N.}, Author, A., Author, B., Author, C., ... ,
|
||||
\textbf{Title of the paper}, Journal, Volume, pages, DOI, (Year) [AO]
|
||||
|
||||
\item Author, A., Author, B., \physbf{Your, N.}, Author, C., ... ,
|
||||
\textbf{Title of the paper}, Journal, Volume, pages, DOI, (Year) [AO]
|
||||
|
||||
\end{enumerate}
|
||||
|
||||
\subsection*{Conference proceedings and other publications}
|
||||
|
||||
\begin{enumerate}
|
||||
|
||||
\item \physbf{Your, N.}, Author, A., Author, B., Author, C., ... ,
|
||||
\textbf{Title of the conference proceedings paper}, Conference Series, pages, DOI, (Year) [AO]
|
||||
|
||||
\item Author, A., Author, B., \physbf{Your, N.}, Author, C., ... , \textbf{Title of the popular paper}, Popular Journal, Volume, pages, DOI, (Year) [AO]
|
||||
|
||||
%\item \physbf{Your N.}, Author C. ... et al.,
|
||||
%\physbf{Title of the press release}, occasion, link
|
||||
|
||||
\end{enumerate}
|
||||
|
||||
%\subsection*{Published code segments}
|
||||
@@ -0,0 +1,37 @@
|
||||
%\afterpage{\newpage~} % ------------------------------------ --> main title page
|
||||
\begin{titlepage}
|
||||
\pdfbookmark[0]{Titlepage}{Titlepage}
|
||||
\tgherosfont
|
||||
|
||||
\flushright
|
||||
%\includegraphics[height=21mm]{KFU_generalLogo.png} \\[2mm]
|
||||
|
||||
\includegraphics[height=21mm]{KFU_Physics.png} \\[2mm]
|
||||
|
||||
%\includegraphics[height=21mm]{KFU_Phys_IGAM.jpg} \\[2mm]
|
||||
|
||||
|
||||
\centering
|
||||
\vfill
|
||||
{\large {\thesisSubject}} \\[5mm]
|
||||
{\LARGE \color{ctcolortitle}\textbf{\thesisTitle} \\[2mm]}
|
||||
{\Large \color{ctcolorgray}%\color{ctcolorgray}
|
||||
\textbf{\thesisSubtitle}\\[15mm]}
|
||||
{\Large \thesisName} \\ [5mm]
|
||||
|
||||
{in partial fulfillment of the requirements for the degree of} \\
|
||||
{\large {{\thesisDegree}}}
|
||||
|
||||
\vfill
|
||||
\begin{minipage}[t]{.27\textwidth}
|
||||
\raggedleft
|
||||
\physit{Supervisors}
|
||||
\end{minipage}
|
||||
\hspace*{15pt}
|
||||
\begin{minipage}[t]{.65\textwidth}
|
||||
\thesisFirstSupervisor\ \\ \thesisSecondSupervisor
|
||||
\end{minipage} \\[10mm]
|
||||
|
||||
\thesisDate \\
|
||||
|
||||
\end{titlepage}
|
||||
@@ -0,0 +1 @@
|
||||
\printthesistitle
|
||||
@@ -0,0 +1,44 @@
|
||||
% !TEX root = ../thesis-example.tex
|
||||
%
|
||||
|
||||
% ------------------------------------ --> cover title page
|
||||
\begin{titlepage}
|
||||
\pdfbookmark[0]{Cover}{Cover}
|
||||
\flushright
|
||||
\hfill
|
||||
\vfill
|
||||
{\color{ctgreenblue}\LARGE\thesisTitle \par}
|
||||
{\color{ctcolorgray}\large\thesisSubtitle}
|
||||
\color{ctgreenblue}\rule[5pt]{\textwidth}{1.25pt} \par
|
||||
{\color{ctgreenblue}\Large\thesisName}
|
||||
\vfill
|
||||
\textit{\large\thesisDate}
|
||||
\end{titlepage}
|
||||
% ------------------------------------ --> page 2 left empty on purpose
|
||||
|
||||
\input{content/titlepageKFU} % uncomment for KFU style
|
||||
%\input{content/titlepageTU} % uncomment for TU style
|
||||
|
||||
% ------------------------------------ --> lower title back for single page layout
|
||||
|
||||
|
||||
\hfill
|
||||
\vfill
|
||||
{
|
||||
\small\noindent
|
||||
\physbf{\thesisName} \\
|
||||
\physit{\thesisTitle~$-$~\thesisSubtitle} \\[0.5em]
|
||||
Thesis in partial fulfillment of the \hbox{requirements for the degree of \thesisDegree}; \\
|
||||
%Thesis submitted on \red{Month DD, 202X}. %and defended on \red{Month DD, 2020}. %e.g. 2020, November 15, 2020. Before submission, uncomment this line, fill out the date, remove the red color of the data and delete the following line, containing 'Unsubmitted Thesis Manuscript'.
|
||||
\red{\bfseries Unsubmitted Thesis Manuscript: compiled on \thesisDate}
|
||||
\\[0.5em]
|
||||
Institute of Physics, NAWI Graz, University of Graz.\\[1.5em]
|
||||
\physit{Supervisors}: \thesisFirstSupervisor $^1$ and
|
||||
\thesisSecondSupervisor $^{1,2}$\\
|
||||
%\physit{Jury panel}:
|
||||
\physit{External Readers}:
|
||||
Dr. Hypatia$^{1}$, Doz.\,Dr. Galileo Galilei$^{2}$, and Prof.\,Dr. Carl Sagan$^{1,2}$
|
||||
\\[1.5em]
|
||||
$^1$~Institut für Physik, \hbox{NAWI\,Graz, University of Graz, Universitätsplatz 5/II, 8010 Graz, Austria.}\\
|
||||
$^2$~Instituto de F\'{\i}sica de Canarias, E-38200 La Laguna, Tenerife, Spain.\\
|
||||
}
|
||||
@@ -0,0 +1,383 @@
|
||||
\pdfbookmark[0]{Writing and formatting guide for your thesis}{Writing and formatting guide for your thesis}
|
||||
\setcounter{chapter}{-1}
|
||||
\chapter{Writing and formatting guide for your thesis}
|
||||
%\pagestyle{plain}
|
||||
|
||||
|
||||
\vspace{-3mm}
|
||||
Dear colleague,
|
||||
|
||||
\textit{Scientific writing} is the number one skill of a successful scientist. Mastering this proficiency requires extensive practice, iteration, and feedback. To support you in the first steps to master this essential skill, we provide you with a summary of the essential style rule and some writing style guidelines. We are happy that you are taking those first steps on this demanding but exciting journey with us.
|
||||
|
||||
|
||||
\vspace{-3mm}
|
||||
%\noindent
|
||||
\begin{flushright}
|
||||
Success in writing your thesis, \\
|
||||
Your thesis advisers at the Institute of Physics\\
|
||||
\end{flushright}
|
||||
|
||||
\noindent \physit{The following notes were written by Paul Beck,\,PhD in Astrophysics, with addenda by the teachers and advisers at the Institute of Physics (Version: April 2021). These notes should be a rough guideline. We advice to consult with your supervisor to get feedback for your writing style and how to correctly put references, since these might differ between different scientific communities (Experimental Physics, Theoretical Physics, Geophysics, Astrophysics).}
|
||||
|
||||
|
||||
\vspace{-5mm}
|
||||
\section*{Writing}
|
||||
\noindent
|
||||
The language has to be clear and objective. Science requires quantifying things and putting results into context. The following items will give you a first impression of where to be on your toes.
|
||||
\begin{itemize}
|
||||
\item Avoid qualitative adjectives (e.g., very, a lot, little, many) and refrain from expressing personal beliefs or using sarcasm. Following the maxim of \textit{'show, don't tell'} a sentence like \textit{'Sample A is much better than sample B'} should be rewritten into something like \textit{'The statistical uncertainty of the measurements of parameter X in sample A is three times smaller than in sample B.'}
|
||||
|
||||
\item Consider your \textit{'Why?'}. A sentence like \textit{'Studying stars is important'}, is a general statement which says everything and nothing at once. Following the principle, \textit{Show, don't tell} you can implicitly show \textit{why} something has significance, rather than saying so, \textit{'Stars are the building blocks of the galaxy. Studying these objects allows for a better understanding of how our milky way evolved'.}
|
||||
|
||||
\item Avoid wordy sentences. A typical sentence should be less than two full lines. A good trick is to mark each sentence longer than that with a text marker on a printout. Then split such sentences into two or three shorter sentences.
|
||||
|
||||
\item Write in an active form. For example, write \textit{`Galileo has found 4 Jovian satellites'} instead of \textit{`The four Jovian satellites have been found by Galileo'}. The active form will help you write more precise and shorter sentences. Remember that your text may need to be read and understood by people with lower language skills than yours. Make the reader's life easier.
|
||||
|
||||
\item Use abbreviations sparsely and only for your most important phrases or key terms. At first use in the text body, they need to be defined. The use of abbreviations or acronyms is highly de-appreciated by editors in a paper's title and abstract. Consequently, colloquially used acronyms, such as HRD, RV, ZAMS, or TAMS, need to be spelled out in the title and abstract.
|
||||
|
||||
\item Similar applies for each mathematical symbol used in the text and equation must be defined at first use $-$ an occasional reminder of the meaning throughout the paper doesn't hurt.
|
||||
|
||||
\item Only use footnotes to indicate webpage links, e.g., for MESA, \textsc{Phoebe}, AstroPy, data catalogs portals, or as demonstrated above for a specific document of high relevance to your work.
|
||||
|
||||
\item References to papers are fundamental for your work's scientific integrity and placing your work into the broader context of timely and relevant research. The examples below and in the next section and Chapter\,\ref{sec:intro} demonstrate the use of the implemented BibTex-package.
|
||||
|
||||
\item Short notes on grammar. Always put a ``,'' before the word ``which'', but never before ``that''. Remember the ``s'' at the end of the verbs in the third singular person. If possible, try to keep the tenses of the verbs always the same throughout the text. Write all numbers between zero and ten as a word while keeping the others in number.
|
||||
|
||||
\item Plagiarism and doctoring the data are the cardinal sins of a scientist. Such behavior is not tolerated. Be aware of the automated plagiarism check during the submission process. If detected, we would consider this a major abuse of our trust in you and reserve the right to take academic action.
|
||||
|
||||
%\item In a continued thought, refrain from starting follow-up sentences with 'This'.
|
||||
\end{itemize}
|
||||
|
||||
%\vspace{5mm}
|
||||
\subsection*{Additional self-study resources on scientific writing}
|
||||
\begin{itemize}
|
||||
|
||||
\item The best way to improve your writing is to read much scientific literature. Different authors write differently, though, so you have to find your own style. You can do this by exercising your writing and reading and identifying authors who write in a way you like. Keep notes on the content of the papers you read. We also recommend reading the article on reading \hbox{papers by \cite{PaperOnRreadingPapers}.}
|
||||
|
||||
\item Concise collections of lecture notes on the topic are available in the books by Prof. Arnold Hanslmeier\footnote{The PDF of the book (in German) is available at \hbox{\href{https://bookboon.com/de/wissenschaftliches-arbeiten-ebook}{https://bookboon.com/de/wissenschaftliches-arbeiten-ebook}}} and \cite{Mack2018Book}\footnote{The PDF of the book (in English) is available at \href{https://spie.org/samples/9781510619142.pdf}{https://spie.org/samples/9781510619142.pdf}}.
|
||||
|
||||
\item You may use modern software, such as \href{http://www.Grammerly.com}{Grammerly.com}, to check your thesis's grammar and spelling. Doing so allows us to focus on discussing science and content and streamline the iteration process.
|
||||
|
||||
\item Play around with \LaTeX. Writing in this scripting language will become second nature to you. You are encouraged to search \LaTeX-documentation and advance your thesis beyond this template, e.g., defining your own frequently used symbol-groups. A good source of documentation about working with \LaTeX\ is provided by Overleaf: \href{https://www.overleaf.com/learn}{https://www.overleaf.com/learn}.
|
||||
|
||||
Commented text, using '\%' allows you to keep hidden notes. This is particular helpful to keep notes or an earlier version of a sentences or paragraph, you wanted to reword.
|
||||
% While they are not shown in the text of the PDF, they are still part of the file and can be read out. There are twitter accounts, which echo the funniest or most embarrasing hidden coments from papers on the preprint server ArXiv: e.g. @LeaksPh is eavesdropping on tex-source comments in papers posted to astro-ph.
|
||||
Use colors to mark action items or text during the iteration phase. Some examples are shown at the end of this chapter.
|
||||
\end{itemize}
|
||||
|
||||
A very common mistake beginners make is to write meaningless sentences. This happens because you know well what you want to say, write it down in a sentence in a meaningless way due to lack of practice. Yet, because you know what you want to say, the sentence you have just written looks useful to you. There is a straightforward strategy that you should apply to avoid this. Write a piece of text, then read it aloud or (even better) record it, and finally listen to it, trying to understand what you want to say from listening to what you read. If you cannot understand the meaning of what you said, then there is something wrong with that text.
|
||||
|
||||
A final piece of advice. Write something, then leave it aside without reading it for a few days and then returning to it. The more times you do this process, the better the text will become.
|
||||
|
||||
|
||||
|
||||
%\newpage
|
||||
\section*{Elements of a scientific work}
|
||||
\noindent
|
||||
In general, the style in this thesis template follows the formatting guidelines\footnote{The PDF version of the editorial guidelines: \href{https://www.aanda.org/doc_journal/instructions/aadoc.pdf}{https://www.aanda.org/doc\_journal/instructions/aadoc.pdf} \label{fn:AAstyleGuide}} of \physit{Astronomy \& Astrophysics {\rmfamily (A\&A)}}, the European workhorse journal for astrophysics. The only divergence from these guidelines is the more extensive bibliographic information of cited papers and how you can \hbox{present your programming code in the appendix.}
|
||||
|
||||
Below, we summarize the essential guidelines to follow in your writing.
|
||||
Examples for typical elements, such as including citations, cross references, and the inclusion of figures and tables are shown in Chapter\,\ref{sec:intro} and Chapter\,\ref{sec:data}. Each content element (e.g. abstract, table of contents, chapter, bibliography) starts on the right page (recto). This means that in some cases the left side (verso) will be left blank. \LaTeX\ will take care of this.
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
\subsection*{Structure of your thesis}
|
||||
\begin{itemize}
|
||||
\item \physbf{Abstract:} It follows the structured abstract of A\&A. Write a few sentences for each of the indicated blocks. The length of the abstract should be about half a page. Do not use abbreviations, acronyms, or formulae in this block. Typically this section is written as last.
|
||||
|
||||
\item \physbf{Acknowledgements:} This section allows you to give explicit credit to people, institutions, programs, or projects. This template shows typical examples. Many telescopes, space missions or software projects provide predefined sentences for the acknowledgements which you simply should copy. Make sure that you \hbox{cite the requested instrumental-reference papers in the text body.}
|
||||
|
||||
\item \physbf{Text body:} consists of the main content of the paper. It starts with the first chapter, the \physit{Introduction}, where you explain, how your research question connects to the bigger picture of the field. Do not write a review on the whole field. Rather follow the recipe depicted in \Fig{fig:logicalFlow}. Ideally, you pick up the argumentative thread again in the the final section on \physit{Discussions \& Conclusions} and demonstrate how your work has advanced on the addressed topics.
|
||||
|
||||
\item Name and content of the following chapters are not defined. However, it should loosely follow the logic: \physit{Methodology}, \physit{Observing techniques} (or simply) \physit{Data $-$ Analysis $-$ Results $-$ Discussions \& Conclusions.} Optimally, you have a \LaTeX\ file per chapter, as demonstrated in this template.
|
||||
|
||||
\item Sections or subsections will follow the logic of your work. Use lower case for all words in chapter and section title headings, except for the first character. Do not introduce subsubsections.
|
||||
|
||||
|
||||
|
||||
\item \physbf{Bibliography:} This section provides all information to find and retrieve your cited literature unambiguously. If you are using the recommended BibTex package to manage your references, this part will be taken care of for you by \LaTeX. How to work with BibTex is demonstrated below.
|
||||
|
||||
\item \physbf{Appendix} is used to place extensive content, which would otherwise interrupt the reader. It can have several sections, labeled with capital letters. You typically would place code, additional figures, or large tables. Content in the appendix, such as figures, tables, or supplementary method descriptions in sections, needs to be referenced at least once in the main text body.
|
||||
|
||||
\item For a master or PhD thesis, include the \physbf{Curriculum Vitae}. Complete the predefined sections. List what is relevant to your studies and research activity.
|
||||
|
||||
\item List your scientific publications in the \physbf{List of publications}.
|
||||
|
||||
\end{itemize}
|
||||
|
||||
\begin{figure}
|
||||
\centering
|
||||
\includegraphics[width=\textwidth]{gfx/constructionMap.png}
|
||||
\caption{Schematic structure of the elements of a thesis or research paper. The cones depict the ideal logical flow of the chapters of the \textit{Introduction} and \textit{Conclusions \& Outlook}. }
|
||||
\label{fig:logicalFlow}
|
||||
\end{figure}
|
||||
|
||||
%The logical flow of a thesis is illustrated in \Fig{fig:logicalFlow}.
|
||||
As the first step in your writing process, we recommend that you lay out the anticipated structure and approximate content by crafting chapter and perhaps the main section titles. This first structure can already be implemented in the template and be discussed with your adviser early on. Doing this will allow you to have a more straightforward path to assess the thesis's content and expected workload.
|
||||
|
||||
|
||||
\subsection*{Literature references \& managing your bibliography}
|
||||
\begin{itemize}
|
||||
\item A citation is needed whenever a bibliographic reference to published content is required. The leading astronomical journals use the style of inter-textual citations. In this format, you see the first author's name in the text, most likely to be followed by \textit{et al.} to indicate that more than two authors have signed the paper and the publication year of the paper. The \textit{Bibliography} section in the rear provides all the information on how to retrieve the cited article. Each item listed in the bibliography needs to \hbox{be referenced at least once in the paper.}
|
||||
|
||||
\item BibTex is a powerful software package that will help you to easily manage your bibliographic references and the respective bibliography. By using the citation commands
|
||||
$\backslash$cite\{\},
|
||||
$\backslash$citep\{\},
|
||||
$\backslash$citep[]$\{\}$, and
|
||||
$\backslash$citep[][]\{\} you create inter-textual references. The following examples show how the above mentioned macros can be used in the syntax of a sentence:
|
||||
|
||||
|
||||
|
||||
$-$ \textit{It was shown by \cite{Beck2015} that the long-periodic variations of the radial-velocity signal of $\theta^1$\,Tau originates from stellar activity.} \\
|
||||
$-$ \textit{Combining remote-sensing image data with in-situ measurements have lead to an improved flare-CME characterization
|
||||
\citep{Temmer2017}.}\\
|
||||
$-$ \textit{The extreme-ultraviolet Radiation from A-stars has significant implications for the formation of \citep[and references therein]{Fossati2018}.}\\
|
||||
$-$ \textit{This topic has been discussed in the recent literature
|
||||
\citep[e.g. see][and references therein]{Hanslmeier2018phsabook,Veronig2020}.}
|
||||
|
||||
\item To cite from a monography use the $\backslash$citep[]\{\} command to reference the book you are citing. If of relevance you can note to which chapter or page you are referring to in the squared brackets of the makro.
|
||||
|
||||
\item Those macros access the content of the file \textit{bib-refs.bib}. To add references, copy the content from \textit{'export citation'} on the NASA ADS webpage of a paper into the bib-file. Experience has shown that it will improve the readability of your \LaTeX\ code if you change the predefined bibcode (e.g., 2017SoPh..292...93T) into a more user-friendly keyword (e.g., Temmer2017), which is then used in the macros mentioned above to cite the paper.
|
||||
|
||||
\end{itemize}
|
||||
|
||||
\subsection*{Cross references to elements inside your thesis}
|
||||
\begin{itemize}
|
||||
\item Each Figure, Table, and Equation presented in the paper needs to be referenced at least once in the text body. The objects of each group (figures, tables, equations) must be introduced in the paper in consecutive order: Reference Fig.\,1 in the text before you mention Fig.\,2.
|
||||
|
||||
\item Abbreviate the following expressions unless they appear at the beginning of a sentence: \textit{Sect., Sects., Fig., Figs., Col., Cols.}. \textit{Table} and \textit{Listing} are never abbreviated in a paper. Write the object abbreviation in the upper case if used as a numbered reference. Otherwise, object names should not be abbreviated and written in lower case.
|
||||
|
||||
$-$ \textit{\Figure{fig:singelPanelPlot} shows the position of 18 eccentric binary in the HR diagram.}\\
|
||||
$-$ \textit{As shown in \Fig{fig:singelPanelPlot}, the 18 eccentric binary are found on the low-luminosity red-giant branch (RGB).} \\
|
||||
$-$ \textit{The 18 eccentric binary are found on the low-luminosity RGB (see \Fig{fig:singelPanelPlot}).}
|
||||
|
||||
\item To generate an automated numbering, you need to create a reference-able label, using \textit{$\backslash$label$\{$keyword$\}$}. Calling the keyword through the reference macro, \textit{$\backslash$ref$\{$keyword$\}$} will create the reference in the text. You can freely choose the keyword. Experience has shown that it is good practice to encode what kind of object you are referencing into the keyword, e.g.
|
||||
\textit{$\backslash$label$\{$fig:HRD$\}$},
|
||||
\textit{$\backslash$label$\{$tab:redGiantCatalogue$\}$},
|
||||
\textit{$\backslash$label$\{$eq:pythagoras$\}$}, or
|
||||
\textit{$\backslash$label$\{$sec:introduction$\}$}.
|
||||
|
||||
Note that the template contains customized macros in the \textit{main.tex} for all full and abbreviate element names. This way, you only need to type, e.g. \textit{$\backslash$Fig\{fig:HRD\}}, instead of \textit{Fig.$\backslash$,$\backslash$ref\{fig:HRD\}}
|
||||
|
||||
|
||||
\end{itemize}
|
||||
|
||||
|
||||
%\newpage
|
||||
\subsection*{Figures}
|
||||
\noindent
|
||||
Example of single and multi-panel figures and their caption format are given in Fig.\,\ref{fig:singelPanelPlot} and Fig.\,\ref{fig:multiPanelPlot}, respectively.
|
||||
\begin{itemize}
|
||||
|
||||
\item \physbf{Position:} to be placed on top of the page, using the figure attribute~\textit{[t!]}. Do not place a figure on the first page of a chapter.
|
||||
|
||||
\item \physbf{Message:} be clear to yourself, what take away message is, which you want to give to the reader of your paper by showing this figure. Now optimize your figure to maximize the storytelling: use different symbols, line styles, and colors. A good test for a colored figure is if it is still readable on a black-and-white printout.
|
||||
|
||||
\item \physbf{Caption}: The first sentence of the figure's caption should be a sentence describing the figure. This sentence should start without 'The' / 'This', 'A / An', or similar.
|
||||
Describe all symbols and line styles used in the figure. Express no physical or scientific interpretation of the depicted context.
|
||||
|
||||
\item Refer to the figure's axes as the \textit{'horizontal'} and the \textit{'vertical axes'}, instead of the x- and y-axis, respectively.
|
||||
|
||||
\item For multi-panel figures, you should refer to the individual panels by using \textit{'top left panel'}, \textit{'middle bottom panel}, or \textit{'bottom right panel'}.
|
||||
|
||||
\item In case you show additional figures depicting different data but using the identical symbol and color scheme, you can refer to the first figure explaining the meaning. State something like \textit{'Meaning of the colors and symbols is similar to Fig.\,XY'}.
|
||||
|
||||
\item If you show a figure previously published in another article, you need to indicate the source, such as \textit{(Figure taken from REFERENCE)}. In case somebody provided you an unpublished figure, you would state \textit{(Figure provided by PERSON).}
|
||||
|
||||
\item \physbf{Axis labels}: produce plots with readable axes, labels, and ticks. Unreadable labels are the easiest way of getting into \hbox{trouble with the referee (or adviser).}
|
||||
|
||||
|
||||
\item Format: preferably use PNG to avoid excessive file sizes for figures depicting many datapoints.
|
||||
|
||||
|
||||
|
||||
\end{itemize}
|
||||
|
||||
%\newpage
|
||||
\subsection*{Tables}
|
||||
\noindent
|
||||
An example of a simple, complex and a multi-page table are given in Tab.\,\ref{tab:false_positives}, Tab.\,\ref{tab:asteroseismicValues}, and Tab.\,\ref{tab:longTable} respectively.
|
||||
|
||||
\begin{itemize}
|
||||
\item \physbf{Position:} to be placed on top of the page, using the table attribute~\textit{[t!]}. Do not place a table on the first page of a chapter.%(The only exception are tables depicting a code's functions, as shown in Appendix\,\ref{chap:appendixCode}.)
|
||||
|
||||
\item \physbf{Caption:} (on top of the table): The table caption should be a one-line sentence, describing the table and placing it into the work or paper context. This sentence should start without 'The' / 'This', 'A / An', or similar.
|
||||
|
||||
\item \physbf{Layout:} Tables start from above with a double vertical line, followed by the table header, followed by a single line, followed by the table's content. A final horizontal line is closing the table.
|
||||
|
||||
If appropriate, you can use horizontal lines in the table body to mark separations. In this case, the A\&A guidelines refer to the separated blocks as panels. An example is given in Table\,\ref{tab:false_positives}.
|
||||
|
||||
\item The content of the table is typically formatted to the left or right of the column. If you wish to do the extra work for a nice looking table, you can center the header, as shown in Tab.\,\ref{tab:asteroseismicValues}.
|
||||
|
||||
\item \physbf{Tablefoot:} (text block below the actual table starting with \physbf{Notes.}) should contain all relevant information for each column should be provided in the table foot. If you use abbreviated references, you should give the connection to the inter-textual references here. Express no physical or scientific interpretation here. The tablefoot-macro requires an empty line between the text and the table to avoid layout issues.
|
||||
|
||||
\item \physbf{Extensive tables} can be presented in the landscape format and / or be split over several pages (longtable). Consider placing it in the Appendix. In this case, you could place the tablefoot-block into the text body of the Appendix as demonstrated in Appendix\,\ref{chap:appendixExtensiveTables}
|
||||
|
||||
\item Tables are usually not used in the Introduction or Conclusions chapter.
|
||||
\end{itemize}
|
||||
|
||||
%\newpage
|
||||
\subsection*{Equations}
|
||||
\begin{itemize}
|
||||
\item Treat equations as part of the sentence and place them like a subordinate clause. See Eq.\,\ref{eq:pyth1}\,and\,\ref{eq:pyth2} for an example.
|
||||
|
||||
\item All mathematical symbols used in the equation need to be defined near the equation, if not defined before in the text. Mention the physical units of the parameter used in the equation.
|
||||
|
||||
\item Text in equations or math mode is written in italics per default. In case you want to place a subscript text, which is not an index, you need to force it to be non-italic, e.g., P$_{\mathrm{orb}}$.
|
||||
|
||||
%\item multiple equations (if \&=\&, alingement of equations)
|
||||
|
||||
%\item \ref{eq:pyth1}, \ref{eq:pyth2}
|
||||
\end{itemize}
|
||||
|
||||
|
||||
\subsection*{Presentation of code and code snippets}
|
||||
|
||||
One of the bricks of the fundament of science is the replicability of disseminated results. Therefore, the modern standard of research journals that any elaborated code that is used for the data analysis presented in the paper should be made available to the reader. Such code is typically distributed on pages such as GitHub.com.
|
||||
For your thesis, we simulate such public distribution of code by presenting your code in the appendix. Discuss with your adviser if or what part of your code should be part of the thesis work. \Listing{code:tidalSettings} and Appendix\,\ref{chap:appendixCode} demonstrate how code (snippet) or pseudo-code is to be presented in the textbody and appendix your thesis, respectively.
|
||||
|
||||
\noindent
|
||||
\physbf{\bfseries\sffamily Presentation in the text body}
|
||||
\begin{itemize}
|
||||
\item Only essential code parts or concepts (via snippets or pseudo code, respectively) should be presented in the main body of your thesis.
|
||||
|
||||
\item The \texttt{verbatim} command is a very severe command, which cannot be used within the iteration tools. Instead of \texttt{verb} or \texttt{verbatim}, please use \textit{$\backslash$texttt$\{\}$}.
|
||||
|
||||
\item Treat the code listing like a table. The \physbf{caption} should be a one-line sentence, describing the table and placing it into the work or paper context. This sentence should start without 'The' / 'This', 'A / An', or similar. Explain the environment and variables in the \physbf{tablefoot}. See \Listing{code:tidalSettings} for an example.
|
||||
\end{itemize}
|
||||
|
||||
\noindent
|
||||
\physbf{\bfseries\sffamily Presentation in the Appendix}
|
||||
\begin{itemize}
|
||||
|
||||
\item Before listing the code, provide a preamble outlining your system dependencies of your code (scripting language, version, etc.) Any necessary information should be given in the preceding preamble.
|
||||
An expamle is shown in Appendix\,\ref{sec:SystemDependencies} and \Table{tab:PyModules}.
|
||||
|
||||
\item Provide a caption as described above, to create a referencable object.
|
||||
|
||||
\item Each program should be listed in a separate section of the Appendix. Before listing the source code, provide an abstract of the tasks and functions of the program. Also, give a brief characterization (name, version, download information) of any non-standard package that you have used imported and~used.
|
||||
|
||||
\item \Listing{cod:helloWorld} provides an example. For the reader's benefit, provide in-code comments and documentation.% to make your code to make it more accessible.
|
||||
|
||||
\item If you have built-in options, provide a table explaining the options' functionality and how they are called. \Table{tab:functionalityTable} provides an example for the necessary documentation. For those tables, use the positioning argument [h!].
|
||||
|
||||
\item To see how to include MESA inlists, activate Appendix\,C. For those use 'language= Fortran'.
|
||||
\end{itemize}
|
||||
|
||||
|
||||
\subsection*{Abfassen einer Arbeit auf Deutsch}
|
||||
\begin{itemize}
|
||||
\item Sollten Sie diese Arbeit auf Deutsch verfassen, so sind auch die Elemente auf Titelseite, Elementnamen (Abstract, Acknowledgements, Table, Figure) sowie der Colophon zu übersetzen. Die Endung 'et al.' verbleibt als solches.
|
||||
|
||||
\item Fachbegriffe müssen in ihrer deutschen Übersetzung ausgeschrieben werden, da eine Mischung zwischen Deutsch und English nicht zulässig ist.
|
||||
|
||||
\item Die Erfahrung hat jedoch gezeigt dass es dem Verständnis des Textes zuträglich ist, wenn in Klammer nach der ersten Verwendung eines Begriffes die englische Originalbezeichnung so wie die in der Literatur übliche Abkürzung angegeben wird.
|
||||
Geben Sie im Appendix ein Glossar der englischen Fachbegriffe sowie der in der Arbeit verwendeten Übersetzung wieder (siehe das auskommentierte Bsp.\,\textit{ appendix$\_$DeutschesGlossar.tex}). Im Text können die Abkürzungen Verwendung finden, wobei bei der ersten Abkürzung im Text eine Fußnote zu setzten ist um auf die Tabelle im Appendix zu verwesien, z.B:
|
||||
|
||||
|
||||
\textit{Der rote Riesensternast (in der englischsprachigen Fachliteratur auch als \textit{red giant branch} oder abgekürzt RGB\footnote{In diesem Text werden der Fachliteratur entsprechend die Abkürzungen des englischsprachigen Fachbegriffes verwendet. Siehe ebenfalls \Table{tab:glossar} im Anhang.} bezeichnet) ist das Stadium des Wasserstoffschalenbrennens. Dieses RGB-Sterne besitzen einen degenerierten Heliumkern.}
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
\end{itemize}
|
||||
|
||||
|
||||
|
||||
\begin{center}
|
||||
\vspace{+5mm}
|
||||
\color{ctgreenblue}\rule[10pt]{0.3\textwidth}{1pt}
|
||||
\vspace{-10mm}
|
||||
\end{center}
|
||||
|
||||
\newpage
|
||||
\section*{Submitting your thesis at the University of Graz}
|
||||
|
||||
Please consult BEFORE start writing your thesis the following webpage
|
||||
\href{https://nawi.uni-graz.at/de/studienservice/alles-zu-abschlussarbeiten/}{Abschlussarbeiten} covering all information starting from the announcement of your thesis topic (needs to be done before actually working on it), until submission of the thesis. In case of questions, always contact your supervisor.
|
||||
|
||||
\newpage
|
||||
\section*{Color scheme and implemented tools for iteration}
|
||||
\noindent The implemented blue-green color in section headings and text markup agrees with the corporate-design manual$^{\ref{fn:KFUcorporateDesignManual}}$ of the University of Graz and the assigned scheme for the Institute for Physics. You can use these comments to highlight important text. This is the only color to be used for text as \hbox{markup in the submitted version.}
|
||||
\begin{table}[h!]
|
||||
%\centering
|
||||
\hfill\begin{tabular}{p{0.25\textwidth}p{0.70\textwidth}}
|
||||
\hline\hline
|
||||
Macro name & Example \& Explanation \\[0.5em] \hline
|
||||
|
||||
%-----------------------------------------------------
|
||||
%Corporate Identity
|
||||
|
||||
\smallskip
|
||||
\textit{$\backslash$physbf$\{\}$} &
|
||||
\smallskip \physbf{bold text with CI color.} \\[0.5em]
|
||||
|
||||
\textit{$\backslash$physit$\{\}$} &
|
||||
\physit{italic text with CI color.}\\[0.5em]
|
||||
\hline
|
||||
\end{tabular}
|
||||
\hfill~
|
||||
|
||||
\end{table}
|
||||
|
||||
\vspace{-5mm}
|
||||
You will find the following macros useful to mark text or place action items and comments in the iteration phase. This approach adopts typical elements of a paper's revision phase, indicating changes requested by the referee.
|
||||
\begin{table}[h!]
|
||||
|
||||
%\centering
|
||||
\hfill\begin{tabular}{p{0.25\textwidth}p{0.70\textwidth}}
|
||||
%\hline\hline Macro name & Example \& Explanation \\[0.5em]
|
||||
\hline
|
||||
|
||||
%-----------------------------------------------------
|
||||
|
||||
\smallskip \textit{$\backslash$myComment$\{\}$} &
|
||||
\smallskip \myComment{Macro marking a comment with your initial.}\\[0.5em]
|
||||
\textit{$\backslash$myRevision$\{\}$} &
|
||||
\myRevision{This macro is to mark text, revised according to your adviser comment.}\\[0.5em]
|
||||
\textit{$\backslash$myToDo$\{\}$} &
|
||||
\myToDo{describe your identified action item.} \\[0.5em] \hline
|
||||
\end{tabular}
|
||||
|
||||
\hfill~
|
||||
|
||||
\end{table}
|
||||
|
||||
\vspace{-5mm}
|
||||
If you and your adviser choose to communicate via a shared project on overleaf, then your adviser has the following defined tools at their disposal to mark and comment. Typically, you can expect an explanation next to \textit{Markover} or \textit{Cossout} why this text requires further attention or should be deleted.
|
||||
\begin{table}[h!]
|
||||
%\centering
|
||||
\hfill\begin{tabular}{p{0.25\textwidth}p{0.70\textwidth}}
|
||||
%\hline\hline Macro name & Example \& Explanation \\[0.5em]
|
||||
\hline
|
||||
|
||||
%-----------------------------------------------------
|
||||
|
||||
\smallskip \textit{$\backslash$adviserComment$\{\}$} &\smallskip\adviserComment{Macro marking a comment of your adviser}\\[0.5em]
|
||||
|
||||
\textit{$\backslash$adviserAddition$\{\}$} &\adviserAddition{Macro marking an textual addition to your thesis.} \\[0.5em]
|
||||
|
||||
\textit{$\backslash$adviserHighlighted$\{\}$} &\colorbox{yellow}{\parbox{0.7\textwidth}{Macro highlighting a text in yellow.}} \\[0.5em]
|
||||
\textit{$\backslash$longSentence$\{\}$} &\colorbox{yellow}{\parbox{0.7\textwidth}{Same as above, printing \textit{'long sentence'} to the right.}} \\[0.5em]
|
||||
|
||||
\textit{$\backslash$adviserMarkover$\{\}$} &
|
||||
\adviserMarkover{Macro marking a text that requires a makeover.}\\[0.5em]
|
||||
|
||||
\textit{$\backslash$adviserMarkoverComment$\{\}\{\}$} &
|
||||
~~~~~~~~~~~~~~\adviserMarkoverComment{Marking text.}{Placing a comment}\\[0.5em]
|
||||
|
||||
\textit{$\backslash$adviserDelete$\{\}$} &\adviserDelete{Text to be deleted.}\\[0.5em]
|
||||
\hline
|
||||
\end{tabular}
|
||||
\hfill~
|
||||
|
||||
\end{table}
|
||||
|
||||
\vspace{-5mm}
|
||||
You are free to change the iterative tools' color settings if you do not like the chosen colors. If so, please make sure that your and your adviser's macros remain well distinguishable in color.
|
||||
|
||||
%Note on writing in German: Sofern in Deutsch geschrieben wird wäre es hilfreich wenn dennoch die Abkürzungen aus der englischen Fachliteratur verwedent würden. Um konsistent zu bleiben, bietet sich folgende erklärenden Fußnote bei dem ersten Fachbegriff an, z.B.
|
||||
%"Die Leuchtkraft eines Sternes an der Spitze des roten Riesenastes (in der englischsprachigen Fachliteratur auch als \textit{red-giant branch} oder abgekürzt\footnote{In diesem Text werden der Fachliterature entsprechend die Abkürzungen des englischsprachigen Fachbegriffes verwendet} als RGB bezeichnet.) von bestimmten Parametern abhängt und beeinflusst wird.
|
||||
Reference in New Issue
Block a user