update templates

This commit is contained in:
2025-11-12 17:13:43 +01:00
parent 63f66fbf02
commit 3202ab8096
114 changed files with 1178 additions and 2034 deletions

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55
Beamer/Parts/Apercu.tex Normal file
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\section{Aper\c{c}u global}
\begin{frame}{Aper\c{c}u global}
Texte normal \alert{Texte Alert} \exemple{Texte exemple} \emph{Texte emphase}
\begin{columns}
\begin{column}{0.5\textwidth}
\begin{block}{Bloc simple}
\begin{itemize}
\item Premier point
\end{itemize}
\end{block}
\begin{exampleblock}{Bloc exemple}
\begin{itemize}
\item Premier point
\end{itemize}
\end{exampleblock}
\begin{alertblock}{Bloc alert}
\begin{itemize}
\item Premier point
\end{itemize}
\end{alertblock}
\end{column}
\begin{column}{0.5\textwidth}
\boiteviolette{
Une boite violette
}
\boiteorange{
Une boite orange
}
\boitegrise{
Une boite grise
}
\begin{tcolorbox}[tabvert,tabularx={X||Y|Y|Y|Y||Y}, boxrule=0.5pt, title=Mon tableau des prix]
Couleur & Prix 1 & Prix 2 & Prix 3 \\\hline\hline
Rouge & 10.00 & 20.00 & 30.00 \\\hline
Vert & 20.00 & 30.00 & 40.00 \\\hline
Bleu & 30.00 & 40.00 & 50.00 \\\hline\hline
Orange & 60.00 & 90.00 & 120.00
\end{tcolorbox}
\end{column}
\end{columns}
\end{frame}

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Beamer/Parts/Blocs.tex Normal file
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\section{Les blocs}
\begin{frame}{Les blocs}
\begin{block}{Bloc simple}
\begin{itemize}
\item Premier point
\item Second point
\item Troisième point
\end{itemize}
\end{block}
\begin{exampleblock}{Bloc exemple}
\begin{itemize}
\item Premier point
\item Second point
\item Troisième point
\end{itemize}
\end{exampleblock}
\begin{alertblock}{Bloc alert}
\begin{itemize}
\item Premier point
\item Second point
\item Troisième point
\end{itemize}
\end{alertblock}
\end{frame}

44
Beamer/Parts/Boites.tex Normal file
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\section{Les bo\^ites}
\begin{frame}{Les boites}
\begin{columns}
\begin{column}{0.5\textwidth}
\boitejaune{
Ceci est \\
une boite jaune
}
\boiteorange{
Ceci est \\
une boite orange
}
\boitemarron{
Ceci est \\
une boite marron
}
\end{column}
\begin{column}{0.5\textwidth}
\boiteviolette{
Ceci est \\
une boite violette
}
\boitebleue{
Ceci est \\
une boite bleue
}
\boitegrise{
Ceci est \\
une boite grise
}
\end{column}
\end{columns}
\end{frame}

11
Beamer/Parts/Figures.tex Normal file
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\section{Les Figures/logos}
\begin{frame}{Titre de la frame}
\begin{figure}
\centering
\includegraphics[scale=0.5]{example-image-a}
\caption{Une bonne description de la figure}
\end{figure}
\end{frame}

31
Beamer/Parts/Listes.tex Normal file
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\section{Les listes}
\subsection{Liste à item}
\begin{frame}{Titre de la frame}
\begin{itemize}
\item premier élément de liste,
\item deuxième élément de liste,
\item troisième élément de liste.
\end{itemize}
\end{frame}
\subsection{Liste énumérative}
\begin{frame}{Titre de la frame}
\begin{enumerate}
\item élément de liste numéro 1,
\item élément de liste numéro 2,
\item élément de liste numéro 3.
\end{enumerate}
\end{frame}
\subsection{Liste descriptive}
\begin{frame}{Titre de la frame}
\begin{description}
\item [Thème de présentation : ] ces thèmes sont en fait...
\item [Thème de couleur : ] gère tout ce qui est couleur...
\item [Thème de police : ] s'occupe de tout ce qui est police, gras...
\item [Thème interne : ] s'occupe de l'apparence des éléments...
\end{description}
\end{frame}

46
Beamer/Parts/Tableaux.tex Normal file
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\section{Les tableaux}
\begin{frame}{Tableaux}
% merci: http://tex.stackexchange.com/questions/112343/beautiful-table-samples
\begin{tcolorbox}[tabjaune,tabularx={X||Y|Y|Y|Y||Y}, boxrule=0.5pt]
Couleur & Prix 1 & Prix 2 & Prix 3 & Prix 4 & Prix 5 \\\hline\hline
Rouge & 10.00 & 20.00 & 30.00 & 40.00 & 100.00 \\\hline
Vert & 20.00 & 30.00 & 40.00 & 50.00 & 140.00 \\\hline
Bleu & 30.00 & 40.00 & 50.00 & 60.00 & 180.00 \\\hline\hline
Orange & 60.00 & 90.00 & 120.00 & 150.00 & 420.00
\end{tcolorbox}
\begin{tcolorbox}[tabvert,tabularx={X||Y|Y|Y|Y||Y}, boxrule=0.5pt, title=Mon tableau des prix]
Couleur & Prix 1 & Prix 2 & Prix 3 & Prix 4 & Prix 5 \\\hline\hline
Rouge & 10.00 & 20.00 & 30.00 & 40.00 & 100.00 \\\hline
Vert & 20.00 & 30.00 & 40.00 & 50.00 & 140.00 \\\hline
Bleu & 30.00 & 40.00 & 50.00 & 60.00 & 180.00 \\\hline\hline
Orange & 60.00 & 90.00 & 120.00 & 150.00 & 420.00
\end{tcolorbox}
\end{frame}
\begin{frame}{Tableaux}
% merci: http://tex.stackexchange.com/questions/112343/beautiful-table-samples
\begin{tcolorbox}[tabgris,tabularx={X||Y|Y|Y|Y||Y}, boxrule=0.5pt]
Couleur & Prix 1 & Prix 2 & Prix 3 & Prix 4 & Prix 5 \\\hline\hline
Rouge & 10.00 & 20.00 & 30.00 & 40.00 & 100.00 \\\hline
Vert & 20.00 & 30.00 & 40.00 & 50.00 & 140.00 \\\hline
Bleu & 30.00 & 40.00 & 50.00 & 60.00 & 180.00 \\\hline\hline
Orange & 60.00 & 90.00 & 120.00 & 150.00 & 420.00
\end{tcolorbox}
\begin{tcolorbox}[taborange,tabularx={X||Y|Y|Y|Y||Y}, boxrule=0.5pt, title=Mon tableau des prix]
Couleur & Prix 1 & Prix 2 & Prix 3 & Prix 4 & Prix 5 \\\hline\hline
Rouge & 10.00 & 20.00 & 30.00 & 40.00 & 100.00 \\\hline
Vert & 20.00 & 30.00 & 40.00 & 50.00 & 140.00 \\\hline
Bleu & 30.00 & 40.00 & 50.00 & 60.00 & 180.00 \\\hline\hline
Orange & 60.00 & 90.00 & 120.00 & 150.00 & 420.00
\end{tcolorbox}
\end{frame}

13
Beamer/Parts/Texte.tex Normal file
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\section{Le texte}
\begin{frame}{Titre de la frame}
Voici du texte normal
\alert{Voici du texte \texttt{alert}}
\exemple{Voici du texte \texttt{exemple}}
\emph{Voici du texte \texttt{emphase}}
\end{frame}

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Beamer/beamer.tex Normal file
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%! TeX Program = pdflatex
%! TeX Root = ./beamer.tex
\documentclass{bredelebeamer}
%\pdfpcsetup{duration=45,lastminutes=5,enduserslide=\getrefnumber{lastslide}}
\selectlanguage{french}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\title[Titre version courte]{Placez votre titre ici dans sa version longue}
% Titre du diaporama
\subtitle{Vous pouvez ajouter un sous-titre}
% Sous-titre optionnel
\author[P. Nom]{Prénom Nom\inst{1}}
% La commande \inst{...} Permet d'afficher l' affiliation de l'intervenant.
% Si il y a plusieurs intervenants: Marcel Dupont\inst{1}, Roger Durand\inst{2}
% Il suffit alors d'ajouter un autre institut sur le modèle ci-dessous.
\institute[(ObAS)]
{
\inst{1}%
Observatoire Astronomique de Strasbourg, CNRS
}
\date{\today}
% Optionnel. La date, généralement celle du jour de la conférence
\subject{Sujet de votre diaporama}
% C'est utilisé dans les métadonnes du PDF
\titlegraphic{
\includegraphics[height=0.10\textheight]{Figures/logos/logo_ObAS.pdf}
\hspace{1.5cm}
\includegraphics[height=0.10\textheight]{Figures/logos/logo_Unistra.pdf}
}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\begin{document}
\begin{frame}[plain]
\titlepage
\end{frame}
\begin{frame}{Sommaire}
\tableofcontents
% possibilité d'ajouter l'option [pausesections]
\end{frame}
\input{Parts/Apercu}
\input{Parts/Blocs}
\input{Parts/Boites}
\input{Parts/Listes}
\input{Parts/Texte}
\input{Parts/Tableaux}
\input{Parts/Figures}
\part*{}
\begin{frame}[plain,label=lastslide]
Pour finir, je dois citer \citet{FavoriteAuthor}, voilà ! Je peux également choisir de le citer en pied de page\footcite{FavoriteAuthor}
\end{frame}
\appendix
\begin{frame}[plain]{Bibliographie}
\renewcommand*{\bibfont}{\footnotesize}
\printbibliography
\end{frame}
\end{document}

10
Beamer/biblio.bib Normal file
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@article{FavoriteAuthor,
author = {{Another-Name}, I. and {Another-Name}, J. and {Another-Name}, K.
and {Another-Name}, L.},
title = "{Some really interesting article I didn't even write}",
journal = {Nature},
year = 2005,
month = oct,
adsurl = {https://ui.adsabs.harvard.edu/abs/},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}

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@@ -9,9 +9,12 @@
\ProvidesClass{bredelebeamer}[17/02/2015, v1.0]
\PassOptionsToPackage{svgnames}{xcolor}
\LoadClass[compress,8pt]{beamer}
\LoadClass[aspectratio=1610,compress,8pt]{beamer}
\setbeamersize{text margin left=5mm, text margin right=5mm}
\usepackage[french]{babel}
% \usepackage[french]{babel}
\usepackage[export]{adjustbox}
\usepackage[english,french]{babel}
\usepackage[utf8]{inputenc}
\usepackage[T1]{fontenc}
\usepackage{helvet}
@@ -19,7 +22,21 @@
\usepackage{graphicx}% http://ctan.org/pkg/graphicx
\usepackage[footnotesize,hang]{caption} % réduire la taille des légendes des images
\usepackage{hyperref}
\usepackage{refcount}
\usepackage{tikz}
\usepackage{qrcode}
\usepackage[overridenote]{pdfpc}
%% Setup for bibliography
\usepackage{csquotes}
\usepackage{microtype}
\usepackage[backend=biber,natbib=true,style=authoryear,uniquelist=false,uniquename=false,giveninits=false,isbn=false,url=false,doi=false,maxcitenames=3,maxbibnames=6,sorting=nyvt]{biblatex}
\addbibresource[glob]{biblio.bib}
\BiblatexSplitbibDefernumbersWarningOff
\DeclareFieldFormat{labelnumberwidth}{}
\setbeamertemplate{bibliography item}{}
\emergencystretch=1em
\renewcommand{\footcite}[2][]{\footnote[#1]{\citet{#2}}}
\usepackage{appendixnumberbeamer}% ne compte pas les slides backups dans le nombre total
\long\def\beamer@@ssection*#1{\beamer@section[]{}}% retire les sections invisibles de la barre de navigation
@@ -47,6 +64,7 @@
\usepackage{tcolorbox}
\usepackage{tabularx}
\usepackage{array}
\usepackage{booktabs}
\usepackage{colortbl}
\tcbuselibrary{skins}
@@ -152,38 +170,39 @@ coltitle=white,center title}}
\beamer@compresstrue
\defbeamertemplate*{headline}{smoothbars theme}
{%
\begin{beamercolorbox}[ht=2.125ex,dp=3.150ex]{section in head/foot}
\insertnavigation{\paperwidth}
\end{beamercolorbox}%
% Commenter les 4 lignes suivantes si vous ne voulez pas la barre des sous-sections.
\begin{beamercolorbox}[ht=2.125ex,dp=1.125ex,%
leftskip=.3cm,rightskip=.3cm plus1fil]{subsection in head/foot}
\usebeamerfont{subsection in head/foot}\insertsubsectionhead
\end{beamercolorbox}%
\begin{beamercolorbox}[ht=2.125ex,dp=3.150ex]{section in head/foot}
\insertnavigation{\paperwidth}
\end{beamercolorbox}%
% Comment next block to hide subsection bar
\ifnum\c@subsection>0{%
\begin{beamercolorbox}[ht=2.125ex,dp=1.125ex,%
leftskip=.3cm,rightskip=.3cm plus1fil]{subsection in head/foot}%
\usebeamerfont{subsection in head/foot}\insertsubsectionhead%
\ifnum\c@subsubsection>0{\;-\;\insertsubsubsectionhead}\fi%
\end{beamercolorbox}%
}\fi%
}
\setbeamercolor{author in head/foot}{bg=leftFootlineColor, fg=authorColor}
\setbeamercolor{title in head/foot}{bg=middleFootlineColor, fg=footlineTitleColor}
\setbeamercolor{institute in head/foot}{fg=instituteColor}
\setbeamercolor{date in head/foot}{bg=rightFootlineColor, fg=dateColor}
\defbeamertemplate*{footline}{infolines theme}
{
\leavevmode%
\hbox{%
\begin{beamercolorbox}[wd=.333333\paperwidth,ht=2.25ex,dp=1ex,center]{author in head/foot}%
\usebeamerfont{author in head/foot}\insertshortauthor~~
\insertshortinstitute
\end{beamercolorbox}%
\begin{beamercolorbox}[wd=.333333\paperwidth,ht=2.25ex,dp=1ex,center]{title in head/foot}%
\usebeamerfont{title in head/foot}\insertshorttitle
\end{beamercolorbox}%
\begin{beamercolorbox}[wd=.333333\paperwidth,ht=2.25ex,dp=1ex,right]{date in head/foot}%
\usebeamerfont{date in head/foot}\insertshortdate{}\hspace*{2em}
\insertframenumber{} / \inserttotalframenumber\hspace*{2ex}
\end{beamercolorbox}
\defbeamertemplate*{footline}{infolines theme}{%
\leavevmode%
\hbox{%
\begin{beamercolorbox}[wd=.333333\paperwidth,ht=2.25ex,dp=1ex,center]{author in head/foot}%
\usebeamerfont{author in head/foot}\insertshortauthor~~%
\insertshortinstitute%
\end{beamercolorbox}%
\begin{beamercolorbox}[wd=.333333\paperwidth,ht=2.25ex,dp=1ex,center]{title in head/foot}%
\usebeamerfont{title in head/foot}\insertshorttitle%
\end{beamercolorbox}%
\begin{beamercolorbox}[wd=.333333\paperwidth,ht=2.25ex,dp=1ex,right]{date in head/foot}%
\usebeamerfont{date in head/foot}\insertshortdate{}\hspace*{2em}%
\insertframenumber{} / \inserttotalframenumber\hspace*{2ex}%
\end{beamercolorbox}%
}%
\vskip0pt%
}%
\vskip0pt%
}
\mode
<all>
@@ -196,76 +215,125 @@ leftskip=.3cm,rightskip=.3cm plus1fil]{subsection in head/foot}
\usepackage{etoolbox}
\AtBeginEnvironment{exampleblock}{%
\setbeamercolor{itemize item}{fg=exampleTitleBlockColor!70}
\setbeamercolor{itemize item}{fg=exampleTitleBlockColor!70}
}
\AtBeginEnvironment{alertblock}{%
\setbeamercolor{itemize item}{fg=alertTitleBlockColor!70}
\setbeamercolor{itemize item}{fg=alertTitleBlockColor!70}
}
\AtBeginEnvironment{block}{%
\setbeamercolor{itemize item}{fg=normalTitleBlockColor!70}
\setbeamercolor{itemize item}{fg=normalTitleBlockColor!70}
}
\newcommand{\boitejaune}[1]{
\begin{center}
\fcolorbox{Framajaune}{Framajaunelight}{
\begin{minipage}{0.5\textwidth}
#1
\end{minipage}
}
\end{center}
\begin{center}
\fcolorbox{Framajaune}{Framajaunelight}{
\begin{minipage}{0.5\textwidth}
#1
\end{minipage}
}
\end{center}
}
\newcommand{\boiteviolette}[1]{
\begin{center}
\fcolorbox{Framaviolet}{Framavioletlight}{
\begin{minipage}{0.5\textwidth}
#1
\end{minipage}
}
\end{center}
\begin{center}
\fcolorbox{Framaviolet}{Framavioletlight}{
\begin{minipage}{0.5\textwidth}
#1
\end{minipage}
}
\end{center}
}
\newcommand{\boiteorange}[1]{
\begin{center}
\fcolorbox{Framaorange}{Framaorangelight}{
\begin{minipage}{0.5\textwidth}
#1
\end{minipage}
}
\end{center}
\begin{center}
\fcolorbox{Framaorange}{Framaorangelight}{
\begin{minipage}{0.5\textwidth}
#1
\end{minipage}
}
\end{center}
}
\newcommand{\boitemarron}[1]{
\begin{center}
\fcolorbox{Framamarron}{Framamarronlight}{
\begin{minipage}{0.5\textwidth}
#1
\end{minipage}
}
\end{center}
\begin{center}
\fcolorbox{Framamarron}{Framamarronlight}{
\begin{minipage}{0.5\textwidth}
#1
\end{minipage}
}
\end{center}
}
\newcommand{\boitegrise}[1]{
\begin{center}
\fcolorbox{Framagris}{Framagrislight}{
\begin{minipage}{0.5\textwidth}
#1
\end{minipage}
}
\end{center}
\begin{center}
\fcolorbox{Framagris}{Framagrislight}{
\begin{minipage}{0.5\textwidth}
#1
\end{minipage}
}
\end{center}
}
\newcommand{\boitebleue}[1]{
\begin{center}
\fcolorbox{Framableu}{Framableulight}{
\begin{minipage}{0.5\textwidth}
#1
\end{minipage}
\begin{center}
\fcolorbox{Framableu}{Framableulight}{
\begin{minipage}{0.5\textwidth}
#1
\end{minipage}
}
\end{center}
}
\end{center}
%%%%%%%%%%%%%%%%%%%%%%%%%%%% Code Listings
% Default fixed font does not support bold face
\DeclareFixedFont{\ttb}{T1}{txtt}{bx}{n}{9} % for bold
\DeclareFixedFont{\ttm}{T1}{txtt}{m}{n}{9} % for normal
% Custom colors
\usepackage{color}
\definecolor{deepblue}{rgb}{0,0,0.5}
\definecolor{deepred}{rgb}{0.6,0,0}
\definecolor{deepgreen}{rgb}{0,0.5,0}
\definecolor{orange}{rgb}{1.0,0.49,0.0}
\definecolor{codegreen}{rgb}{0,0.6,0}
\definecolor{codegray}{rgb}{0.5,0.5,0.5}
\definecolor{codepurple}{HTML}{C42043}
\definecolor{backcolour}{HTML}{F2F2F2}
\definecolor{bookColor}{cmyk}{0,0,0,0.90}
\color{bookColor}
\usepackage{listings}
% Python style for highlighting
\newcommand\pythonstyle{\lstset{
language=Python,
basicstyle=\scriptsize\ttfamily,
morekeywords={self}, % Add keywords here
keywordstyle=\bf\color{deepblue},
emph={MyClass,__init__}, % Custom highlighting
emphstyle=\bf\color{deepred}, % Custom highlighting style
stringstyle=\color{deepgreen},
commentstyle=\bf\color{codegray},
frame=single, % Any extra options here
showstringspaces=false,
breaklines=true,
}}
% Python environment
\lstnewenvironment{python}[1][]
{
\pythonstyle
\lstset{#1}
}
{}
% Python for external files
\newcommand\pythonexternal[2][]{{
\pythonstyle
\lstinputlisting[#1]{#2}
}}

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@@ -1,300 +0,0 @@
\documentclass{bredelebeamer}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\title[Titre version courte]{Placez votre titre ici dans sa version longue}
% Titre du diaporama
\subtitle{Vous pouvez ajouter un sous-titre}
% Sous-titre optionnel
\author{Thibault Barnouin\inst{1}}
% La commande \inst{...} Permet d'afficher l' affiliation de l'intervenant.
% Si il y a plusieurs intervenants: Marcel Dupont\inst{1}, Roger Durand\inst{2}
% Il suffit alors d'ajouter un autre institut sur le modèle ci-dessous.
\institute[(ObAS)]
{
\inst{1}%
Observatoire Astronomique de Strasbourg, CNRS
}
\date{September 30$^\text{th}$ 2025}
% Optionnel. La date, généralement celle du jour de la conférence
\subject{Sujet de votre diaporama}
% C'est utilisé dans les métadonnes du PDF
\titlegraphic{
\includegraphics[height=0.10\textheight]{images/logo_ObAS.pdf}
\hspace{1.5cm}
\includegraphics[height=0.10\textheight]{images/logo_Unistra.pdf}
}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\begin{document}
\begin{frame}
\titlepage
\end{frame}
\begin{frame}{Sommaire}
\tableofcontents
% possibilité d'ajouter l'option [pausesections]
\end{frame}
\section{Aperçu global}
\begin{frame}{Aperçu global}
Texte normal \alert{Texte Alert} \exemple{Texte exemple} \emph{Texte emphase}
\begin{columns}
\begin{column}{0.5\textwidth}
\begin{block}{Bloc simple}
\begin{itemize}
\item Premier point
\end{itemize}
\end{block}
\begin{exampleblock}{Bloc exemple}
\begin{itemize}
\item Premier point
\end{itemize}
\end{exampleblock}
\begin{alertblock}{Bloc alert}
\begin{itemize}
\item Premier point
\end{itemize}
\end{alertblock}
\end{column}
\begin{column}{0.5\textwidth}
\boiteviolette{
Une boite violette
}
\boiteorange{
Une boite orange
}
\boitegrise{
Une boite grise
}
\begin{tcolorbox}[tabvert,tabularx={X||Y|Y|Y|Y||Y}, boxrule=0.5pt, title=Mon tableau des prix]
Couleur & Prix 1 & Prix 2 & Prix 3 \\\hline\hline
Rouge & 10.00 & 20.00 & 30.00 \\\hline
Vert & 20.00 & 30.00 & 40.00 \\\hline
Bleu & 30.00 & 40.00 & 50.00 \\\hline\hline
Orange & 60.00 & 90.00 & 120.00
\end{tcolorbox}
\end{column}
\end{columns}
\end{frame}
\section{Les blocs}
\begin{frame}{Les blocs}
\begin{block}{Bloc simple}
\begin{itemize}
\item Premier point
\item Second point
\item Troisième point
\end{itemize}
\end{block}
\begin{exampleblock}{Bloc exemple}
\begin{itemize}
\item Premier point
\item Second point
\item Troisième point
\end{itemize}
\end{exampleblock}
\begin{alertblock}{Bloc alert}
\begin{itemize}
\item Premier point
\item Second point
\item Troisième point
\end{itemize}
\end{alertblock}
\end{frame}
\section{Les bo\^ites}
\begin{frame}{Les boites}
\begin{columns}
\begin{column}{0.5\textwidth}
\boitejaune{
Ceci est \\
une boite jaune
}
\boiteorange{
Ceci est \\
une boite orange
}
\boitemarron{
Ceci est \\
une boite marron
}
\end{column}
\begin{column}{0.5\textwidth}
\boiteviolette{
Ceci est \\
une boite violette
}
\boitebleue{
Ceci est \\
une boite bleue
}
\boitegrise{
Ceci est \\
une boite grise
}
\end{column}
\end{columns}
\end{frame}
\section{Les listes}
\subsection{Liste à item}
\begin{frame}{Titre de la frame}
\begin{itemize}
\item premier élément de liste,
\item deuxième élément de liste,
\item troisième élément de liste.
\end{itemize}
\end{frame}
\subsection{Liste énumérative}
\begin{frame}{Titre de la frame}
\begin{enumerate}
\item élément de liste numéro 1,
\item élément de liste numéro 2,
\item élément de liste numéro 3.
\end{enumerate}
\end{frame}
\subsection{Liste descriptive}
\begin{frame}{Titre de la frame}
\begin{description}
\item [Thème de présentation : ] ces thèmes sont en fait...
\item [Thème de couleur : ] gère tout ce qui est couleur...
\item [Thème de police : ] s'occupe de tout ce qui est police, gras...
\item [Thème interne : ] s'occupe de l'apparence des éléments...
\end{description}
\end{frame}
\section{Le texte}
\begin{frame}{Titre de la frame}
Voici du texte normal
\alert{Voici du texte \texttt{alert}}
\exemple{Voici du texte \texttt{exemple}}
\emph{Voici du texte \texttt{emphase}}
\end{frame}
\section{Les tableaux}
\begin{frame}{Tableaux}
% merci: http://tex.stackexchange.com/questions/112343/beautiful-table-samples
\begin{tcolorbox}[tabjaune,tabularx={X||Y|Y|Y|Y||Y}, boxrule=0.5pt]
Couleur & Prix 1 & Prix 2 & Prix 3 & Prix 4 & Prix 5 \\\hline\hline
Rouge & 10.00 & 20.00 & 30.00 & 40.00 & 100.00 \\\hline
Vert & 20.00 & 30.00 & 40.00 & 50.00 & 140.00 \\\hline
Bleu & 30.00 & 40.00 & 50.00 & 60.00 & 180.00 \\\hline\hline
Orange & 60.00 & 90.00 & 120.00 & 150.00 & 420.00
\end{tcolorbox}
\begin{tcolorbox}[tabvert,tabularx={X||Y|Y|Y|Y||Y}, boxrule=0.5pt, title=Mon tableau des prix]
Couleur & Prix 1 & Prix 2 & Prix 3 & Prix 4 & Prix 5 \\\hline\hline
Rouge & 10.00 & 20.00 & 30.00 & 40.00 & 100.00 \\\hline
Vert & 20.00 & 30.00 & 40.00 & 50.00 & 140.00 \\\hline
Bleu & 30.00 & 40.00 & 50.00 & 60.00 & 180.00 \\\hline\hline
Orange & 60.00 & 90.00 & 120.00 & 150.00 & 420.00
\end{tcolorbox}
\end{frame}
\begin{frame}{Tableaux}
% merci: http://tex.stackexchange.com/questions/112343/beautiful-table-samples
\begin{tcolorbox}[tabgris,tabularx={X||Y|Y|Y|Y||Y}, boxrule=0.5pt]
Couleur & Prix 1 & Prix 2 & Prix 3 & Prix 4 & Prix 5 \\\hline\hline
Rouge & 10.00 & 20.00 & 30.00 & 40.00 & 100.00 \\\hline
Vert & 20.00 & 30.00 & 40.00 & 50.00 & 140.00 \\\hline
Bleu & 30.00 & 40.00 & 50.00 & 60.00 & 180.00 \\\hline\hline
Orange & 60.00 & 90.00 & 120.00 & 150.00 & 420.00
\end{tcolorbox}
\begin{tcolorbox}[taborange,tabularx={X||Y|Y|Y|Y||Y}, boxrule=0.5pt, title=Mon tableau des prix]
Couleur & Prix 1 & Prix 2 & Prix 3 & Prix 4 & Prix 5 \\\hline\hline
Rouge & 10.00 & 20.00 & 30.00 & 40.00 & 100.00 \\\hline
Vert & 20.00 & 30.00 & 40.00 & 50.00 & 140.00 \\\hline
Bleu & 30.00 & 40.00 & 50.00 & 60.00 & 180.00 \\\hline\hline
Orange & 60.00 & 90.00 & 120.00 & 150.00 & 420.00
\end{tcolorbox}
\end{frame}
\section{Les images}
\begin{frame}{Titre de la frame}
\begin{figure}
\centering
\includegraphics[scale=0.5]{images/logo_ObAS.pdf}
\caption{Une bonne description de la figure}
\end{figure}
\end{frame}
\end{document}

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root = true
[*]
charset = utf-8
end_of_line = lf
indent_style = space
insert_final_newline = true
trim_trailing_whitespace = true
[Makefile]
indent_style = tab
indent_size = 8
[*.{tex,sty,bib}]
indent_size = 2

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$bibtex_use = 2;
$clean_ext = "nav snm";

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The MIT License (MIT)
=====================
**Copyright (c) Anish Athalye (me@anishathalye.com)**
Permission is hereby granted, free of charge, to any person obtaining a copy of
this software and associated documentation files (the "Software"), to deal in
the Software without restriction, including without limitation the rights to
use, copy, modify, merge, publish, distribute, sublicense, and/or sell copies
of the Software, and to permit persons to whom the Software is furnished to do
so, subject to the following conditions:
The above copyright notice and this permission notice shall be included in all
copies or substantial portions of the Software.
THE SOFTWARE IS PROVIDED "AS IS", WITHOUT WARRANTY OF ANY KIND, EXPRESS OR
IMPLIED, INCLUDING BUT NOT LIMITED TO THE WARRANTIES OF MERCHANTABILITY,
FITNESS FOR A PARTICULAR PURPOSE AND NONINFRINGEMENT. IN NO EVENT SHALL THE
AUTHORS OR COPYRIGHT HOLDERS BE LIABLE FOR ANY CLAIM, DAMAGES OR OTHER
LIABILITY, WHETHER IN AN ACTION OF CONTRACT, TORT OR OTHERWISE, ARISING FROM,
OUT OF OR IN CONNECTION WITH THE SOFTWARE OR THE USE OR OTHER DEALINGS IN THE
SOFTWARE.

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@@ -1,9 +0,0 @@
.PHONY: main clean FORCE
main: poster.pdf
poster.pdf: FORCE
latexmk -pdflatex='lualatex -interaction nonstopmode' -pdf poster.tex
clean:
latexmk -pdf -C

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@@ -1,91 +0,0 @@
# Gemini [![Build Status](https://github.com/anishathalye/gemini/actions/workflows/ci.yml/badge.svg)](https://github.com/anishathalye/gemini/actions/workflows/ci.yml)
Gemini is a modern LaTeX [beamerposter] theme.
<p align="center">
<a href="https://raw.githubusercontent.com/anishathalye/assets/master/gemini/poster-gemini.pdf">
<img src="https://raw.githubusercontent.com/anishathalye/assets/master/gemini/poster-gemini-small.png">
</a>
</p>
If you're looking for a beamer presentation theme, take a look at [Auriga].
## Dependencies
* A TeX installation that includes [LuaTeX]
* You also need `latexmk` if you want to use the provided `Makefile`
* LaTeX package dependencies including beamerposter (these usually come with
your TeX installation, but if not, you can get them from [CTAN])
* [Raleway] and [Lato], which are both available under Open Font License
## Usage
1. Copy the files in this repository (or clone the repository)
1. In `poster.tex`, set up your paper size, column layout, and scale the
content as necessary
1. Make a copy of `beamercolorthemegemini.sty`, update the `\usecolortheme`
line in `poster.tex`, and theme the poster to your liking (optional, but
highly recommended)
1. Run `make` to build your poster
## FAQ
See the [FAQ] in the Wiki for answers to frequently asked questions such as how
to add an institution logo to the poster.
## Themes
Gemini currently includes the following color themes:
* `gemini` (default)
* `mit`
* `umich`
* `labsix`
It's also easy to make your own!
### MIT theme
<p align="center">
<a href="https://raw.githubusercontent.com/anishathalye/assets/master/gemini/poster-mit.pdf">
<img src="https://raw.githubusercontent.com/anishathalye/assets/master/gemini/poster-mit-small.png">
</a>
</p>
### LabSix theme
<p align="center">
<a href="https://raw.githubusercontent.com/anishathalye/assets/master/gemini/poster-labsix.pdf">
<img src="https://raw.githubusercontent.com/anishathalye/assets/master/gemini/poster-labsix-small.png">
</a>
</p>
## Design goals
* **Minimal**: clean and easy to read, so that the emphasis is on the content
* **Batteries included**: works and looks good out of the box
* **Easy theming**: easy to create and use a new color theme
## Contributing
Contributions to Gemini such as bug reports, new themes, and new poster
components are greatly appreciated! Given the subjective nature of design,
you're encouraged to open an issue or pull request early to get feedback before
investing a lot of time in implementing a new feature.
## License
Copyright (c) Anish Athalye. Released under the MIT License. See
[LICENSE.md][license] for details.
[beamerposter]: https://github.com/deselaers/latex-beamerposter
[Auriga]: https://github.com/anishathalye/auriga
[LuaTeX]: http://www.luatex.org/
[CTAN]: https://ctan.org/
[Raleway]: https://www.fontsquirrel.com/fonts/raleway
[Lato]: https://www.fontsquirrel.com/fonts/lato
[license]: LICENSE.md
[FAQ]: https://github.com/anishathalye/gemini/wiki/FAQ

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@@ -1,58 +0,0 @@
% Gemini theme
% https://github.com/anishathalye/gemini
% ====================
% Definitions
% ====================
\definecolor{lightgray}{RGB}{245, 246, 250}
\definecolor{blue}{RGB}{64, 115, 158}
\definecolor{darkblue}{RGB}{39, 60, 117}
\definecolor{lightblue}{RGB}{232, 244, 255}
% ====================
% Theme
% ====================
% Basic colors
\setbeamercolor{palette primary}{fg=black,bg=white}
\setbeamercolor{palette secondary}{fg=black,bg=white}
\setbeamercolor{palette tertiary}{bg=black,fg=white}
\setbeamercolor{palette quaternary}{fg=black,bg=white}
\setbeamercolor{structure}{fg=darkblue}
% Headline
\setbeamercolor{headline}{fg=lightgray,bg=blue}
\setbeamercolor{headline rule}{bg=darkblue}
% Block
\setbeamercolor{block title}{fg=blue,bg=white}
\setbeamercolor{block separator}{bg=black}
\setbeamercolor{block body}{fg=black,bg=white}
% Alert Block
\setbeamercolor{block alerted title}{fg=blue,bg=lightblue}
\setbeamercolor{block alerted separator}{bg=black}
\setbeamercolor{block alerted body}{fg=black,bg=lightblue}
% Example Block
\setbeamercolor{block example title}{fg=blue,bg=lightgray}
\setbeamercolor{block example separator}{bg=black}
\setbeamercolor{block example body}{fg=black,bg=lightgray}
% Heading
\setbeamercolor{heading}{fg=black}
% Itemize
\setbeamercolor{item}{fg=darkblue}
% Bibliography
\setbeamercolor{bibliography item}{fg=black}
\setbeamercolor{bibliography entry author}{fg=black}
\setbeamercolor{bibliography entry title}{fg=black}
\setbeamercolor{bibliography entry location}{fg=black}
\setbeamercolor{bibliography entry note}{fg=black}
\setbeamertemplate{bibliography entry article}{}
\setbeamertemplate{bibliography entry title}{}
\setbeamertemplate{bibliography entry location}{}
\setbeamertemplate{bibliography entry note}{}

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% Gemini theme
% https://github.com/anishathalye/gemini
% ====================
% Definitions
% ====================
\definecolor{labsixorange}{RGB}{243, 111, 33}
% Extra colors
\definecolor{lightgray}{RGB}{240, 240, 240}
\definecolor{lightorange}{RGB}{255, 240, 230}
% ====================
% Theme
% ====================
% Basic colors
\setbeamercolor{palette primary}{fg=black,bg=white}
\setbeamercolor{palette secondary}{fg=black,bg=white}
\setbeamercolor{palette tertiary}{bg=black,fg=white}
\setbeamercolor{palette quaternary}{fg=black,bg=white}
\setbeamercolor{structure}{fg=labsixorange}
% Headline
\setbeamercolor{headline}{fg=white,bg=labsixorange}
\setbeamercolor{headline rule}{bg=black}
% Block
\setbeamercolor{block title}{fg=labsixorange,bg=white}
\setbeamercolor{block separator}{bg=black}
\setbeamercolor{block body}{fg=black,bg=white}
% Alert Block
\setbeamercolor{block alerted title}{fg=labsixorange,bg=lightorange}
\setbeamercolor{block alerted separator}{bg=black}
\setbeamercolor{block alerted body}{fg=black,bg=lightorange}
% Example Block
\setbeamercolor{block example title}{fg=labsixorange,bg=lightgray}
\setbeamercolor{block example separator}{bg=black}
\setbeamercolor{block example body}{fg=black,bg=lightgray}
% Heading
\setbeamercolor{heading}{fg=black}
% Itemize
\setbeamercolor{item}{fg=labsixorange}
% Bibliography
\setbeamercolor{bibliography item}{fg=black}
\setbeamercolor{bibliography entry author}{fg=black}
\setbeamercolor{bibliography entry title}{fg=black}
\setbeamercolor{bibliography entry location}{fg=black}
\setbeamercolor{bibliography entry note}{fg=black}

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@@ -1,57 +0,0 @@
% Gemini theme
% https://github.com/anishathalye/gemini
% ====================
% Definitions
% ====================
% Colors from http://web.mit.edu/graphicidentity/colors.html
\definecolor{mitred}{cmyk}{0.24, 1.0, 0.78, 0.17}
\definecolor{mitdarkgray}{cmyk}{0.48, 0.39, 0.39, 0.04}
\definecolor{mitlightgray}{cmyk}{0.24, 0.20, 0.20, 0.0}
% Extra colors
\definecolor{lightgray}{RGB}{240, 240, 240}
\definecolor{lightorange}{RGB}{255, 245, 242}
% ====================
% Theme
% ====================
% Basic colors
\setbeamercolor{palette primary}{fg=black,bg=white}
\setbeamercolor{palette secondary}{fg=black,bg=white}
\setbeamercolor{palette tertiary}{bg=black,fg=white}
\setbeamercolor{palette quaternary}{fg=black,bg=white}
\setbeamercolor{structure}{fg=mitred}
% Headline
\setbeamercolor{headline}{fg=black,bg=lightgray}
% Block
\setbeamercolor{block title}{fg=mitred,bg=white}
\setbeamercolor{block separator}{bg=black}
\setbeamercolor{block body}{fg=black,bg=white}
% Alert Block
\setbeamercolor{block alerted title}{fg=mitred,bg=lightorange}
\setbeamercolor{block alerted separator}{bg=black}
\setbeamercolor{block alerted body}{fg=black,bg=lightorange}
% Example Block
\setbeamercolor{block example title}{fg=mitred,bg=lightgray}
\setbeamercolor{block example separator}{bg=black}
\setbeamercolor{block example body}{fg=black,bg=lightgray}
% Heading
\setbeamercolor{heading}{fg=black}
% Itemize
\setbeamercolor{item}{fg=mitred}
% Bibliography
\setbeamercolor{bibliography item}{fg=black}
\setbeamercolor{bibliography entry author}{fg=black}
\setbeamercolor{bibliography entry title}{fg=black}
\setbeamercolor{bibliography entry location}{fg=black}
\setbeamercolor{bibliography entry note}{fg=black}

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@@ -1,55 +0,0 @@
% Gemini theme
% https://github.com/anishathalye/gemini
% ====================
% Definitions
% ====================
\definecolor{UMichBlue}{RGB}{0, 39, 76} % #00274C
\definecolor{UMichMaize}{RGB}{255, 203, 5} % #FFCB05
\definecolor{UMichWhite}{RGB}{255, 255, 255} % #FFFFFF
\definecolor{UMichGray}{RGB}{235, 235, 235}
\definecolor{UMichLightMaize}{RGB}{242, 237, 217}
% ====================
% Theme
% ====================
% Basic colors
\setbeamercolor{palette primary}{fg=UMichBlue,bg=UMichWhite}
\setbeamercolor{palette secondary}{fg=UMichBlue,bg=UMichWhite}
\setbeamercolor{palette tertiary}{bg=UMichBlue,fg=UMichWhite}
\setbeamercolor{palette quaternary}{fg=UMichBlue,bg=UMichWhite}
\setbeamercolor{structure}{fg=UMichBlue}
% Headline
\setbeamercolor{headline}{fg=UMichGray,bg=UMichBlue}
\setbeamercolor{headline rule}{bg=UMichMaize}
% Block
\setbeamercolor{block title}{fg=UMichBlue,bg=UMichWhite}
\setbeamercolor{block separator}{bg=UMichBlue}
\setbeamercolor{block body}{fg=UMichBlue,bg=UMichWhite}
% Alert Block
\setbeamercolor{block alerted title}{fg=UMichBlue,bg=UMichLightMaize}
\setbeamercolor{block alerted separator}{bg=UMichBlue}
\setbeamercolor{block alerted body}{fg=UMichBlue,bg=UMichLightMaize}
% Example Block
\setbeamercolor{block example title}{fg=UMichBlue,bg=UMichWhite}
\setbeamercolor{block example separator}{bg=UMichBlue}
\setbeamercolor{block example body}{fg=UMichBlue,bg=UMichWhite}
% Heading
\setbeamercolor{heading}{fg=UMichBlue}
% Itemize
\setbeamercolor{item}{fg=UMichBlue}
% Bibliography
\setbeamercolor{bibliography item}{fg=UMichBlue}
\setbeamercolor{bibliography entry author}{fg=UMichBlue}
\setbeamercolor{bibliography entry title}{fg=UMichBlue}
\setbeamercolor{bibliography entry location}{fg=UMichBlue}
\setbeamercolor{bibliography entry note}{fg=UMichBlue}

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@@ -1,257 +0,0 @@
% Gemini theme
% https://github.com/anishathalye/gemini
% ====================
% Dependencies
% ====================
\RequirePackage{exscale}
\RequirePackage{ragged2e}
\RequirePackage{changepage}
\RequirePackage{fontspec}
\RequirePackage{calc}
% ====================
% Fonts
% ====================
\newfontfamily\Raleway[Ligatures=TeX]{Raleway}
\newfontfamily\Lato[Ligatures=TeX]{Lato}
\usefonttheme{professionalfonts}
\setsansfont{Lato}[
UprightFont=*-Light,
ItalicFont=*-LightItalic,
BoldFont=*-Regular,
BoldItalicFont=*-Italic
]
\setbeamerfont{headline}{family=\Raleway}
\setbeamerfont{headline title}{size=\Huge,series=\bfseries}
\setbeamerfont{headline author}{size=\Large}
\setbeamerfont{headline institute}{size=\normalsize}
\setbeamerfont{block title}{family=\Raleway,size=\large,series=\bfseries}
\setbeamerfont{heading}{family=\Lato,series=\bfseries}
\setbeamerfont{caption}{size=\small}
\setbeamerfont{footline}{family=\Raleway,size=\normalsize}
% ====================
% Macros
% ====================
\newcommand{\samelineand}{\qquad}
% ====================
% Elements
% ====================
% List
\def\@listi{\leftmargin\leftmargini
\topsep 1ex % spacing before
\parsep 0\p@ \@plus\p@
\itemsep 0.5ex} % spacing between
% Itemize
\setbeamertemplate{itemize item}{\raise0.5ex \hbox{\vrule width 0.5ex height 0.5ex}}
\setbeamertemplate{itemize subitem}{\raise0.3ex \hbox{\vrule width 0.5ex height 0.5ex}}
\setbeamertemplate{itemize subsubitem}{\raise0.2ex \hbox{\vrule width 0.5ex height 0.5ex}}
% Enumerate
\setbeamertemplate{enumerate item}{\insertenumlabel.}
\setbeamertemplate{enumerate subitem}{\insertsubenumlabel.}
\setbeamertemplate{enumerate subsubitem}{\insertsubsubenumlabel.}
% Equation
\setlength\belowdisplayshortskip{2ex}
% Caption
\setbeamertemplate{caption}[numbered]
\setbeamertemplate{caption label separator}[period]
\setlength{\abovecaptionskip}{2ex}
\setlength{\belowcaptionskip}{1ex}
% Bibliography
\setbeamertemplate{bibliography item}[text]
% Navigation
\beamertemplatenavigationsymbolsempty
% ====================
% Components
% ====================
% Heading
\newcommand\heading[1]
{%
\par\bigskip
{\usebeamerfont{heading}\usebeamercolor[fg]{heading}#1}\par\smallskip
}
% logo
\newlength{\logoleftwidth}
\setlength{\logoleftwidth}{0cm}
\newlength{\logorightwidth}
\setlength{\logorightwidth}{0cm}
\newlength{\maxlogowidth} % space on both sides set to maxlogowidth to keep title centered
\setlength{\maxlogowidth}{0cm}
\newcommand{\logoright}[1]{
\newcommand{\insertlogoright}{#1}
\settowidth{\logorightwidth}{\insertlogoright}
\addtolength{\logorightwidth}{10ex}
\setlength{\maxlogowidth}{\maxof{\logoleftwidth}{\logorightwidth}}
}
\newcommand{\logoleft}[1]{
\newcommand{\insertlogoleft}{#1}
\settowidth{\logoleftwidth}{\insertlogoleft}
\addtolength{\logoleftwidth}{10ex}
\setlength{\maxlogowidth}{\maxof{\logoleftwidth}{\logorightwidth}}
}
% Headline
\setbeamertemplate{headline}
{
\begin{beamercolorbox}{headline}
\begin{columns}
\begin{column}{\maxlogowidth}
\vskip5ex
\ifdefined\insertlogoleft
\vspace*{\fill}
\hspace{10ex}
\raggedright
\insertlogoleft
\vspace*{\fill}
\else\fi
\end{column}
\begin{column}{\dimexpr\paperwidth-\maxlogowidth-\maxlogowidth}
\usebeamerfont{headline}
\vskip3ex
\centering
\ifx \inserttitle \empty \else
{\usebeamerfont{headline title}\usebeamercolor[fg]{headline title}\inserttitle\\[0.5ex]}
\fi
\ifx \beamer@shortauthor \empty \else
{\usebeamerfont{headline author}\usebeamercolor[fg]{headline author}\insertauthor\\[1ex]}
\fi
\ifx \insertinstitute \empty \else
{\usebeamerfont{headline institute}\usebeamercolor[fg]{headline institute}\insertinstitute\\[1ex]}
\fi
\end{column}
\begin{column}{\maxlogowidth}
\vskip5ex
\ifdefined\insertlogoright
\vspace*{\fill}
\raggedleft
\insertlogoright
\hspace{10ex}
\vspace*{\fill}
\else\fi
\end{column}
\end{columns}
\vspace{5ex}
\ifbeamercolorempty[bg]{headline rule}{}{
\begin{beamercolorbox}[wd=\paperwidth,colsep=0.5ex]{headline rule}\end{beamercolorbox}
}
\end{beamercolorbox}
}
% Block
\setbeamertemplate{block begin}
{
\begin{beamercolorbox}[colsep*=0ex,dp=2ex,center]{block title}
\vskip0pt
\usebeamerfont{block title}\insertblocktitle
\vskip-1.25ex
\begin{beamercolorbox}[colsep=0.025ex]{block separator}\end{beamercolorbox}
\end{beamercolorbox}
{\parskip0pt\par}
\usebeamerfont{block body}
\vskip-0.5ex
\begin{beamercolorbox}[colsep*=0ex]{block body}
\justifying
\setlength{\parskip}{1ex}
\vskip-2ex
}
\setbeamertemplate{block end}
{
\end{beamercolorbox}
\vskip0pt
\vspace*{2ex}
}
% Alert Block
\setbeamertemplate{block alerted begin}
{
\begin{beamercolorbox}[colsep*=0ex,dp=2ex,center]{block alerted title}
\vskip0pt
\usebeamerfont{block title}\insertblocktitle
\vskip-1.25ex
\begin{beamercolorbox}[colsep=0.025ex]{block alerted separator}\end{beamercolorbox}
\end{beamercolorbox}
{\parskip0pt\par}
\usebeamerfont{block body}
\vskip-0.5ex
\begin{beamercolorbox}[colsep*=0ex]{block alerted body}
\justifying
\begin{adjustwidth}{1ex}{1ex}
\setlength{\parskip}{1ex}
\vskip-2ex
}
\setbeamertemplate{block alerted end}
{
\end{adjustwidth}
\vskip1ex
\end{beamercolorbox}
\vskip0pt
\vspace*{2ex}
}
% Example Block
\setbeamertemplate{block example begin}
{
\begin{beamercolorbox}[colsep*=0ex,dp=2ex,center]{block example title}
\vskip0pt
\usebeamerfont{block title}\insertblocktitle
\vskip-1.25ex
\begin{beamercolorbox}[colsep=0.025ex]{block example separator}\end{beamercolorbox}
\end{beamercolorbox}
{\parskip0pt\par}
\usebeamerfont{block body}
\vskip-0.5ex
\begin{beamercolorbox}[colsep*=0ex]{block example body}
\justifying
\begin{adjustwidth}{1ex}{1ex}
\setlength{\parskip}{1ex}
\vskip-2ex
}
\setbeamertemplate{block example end}
{
\end{adjustwidth}
\vskip1ex
\end{beamercolorbox}
\vskip0pt
\vspace*{2ex}
}
% Footer
\newcommand{\footercontent}[1]{\newcommand{\insertfootercontent}{#1}}
\setbeamertemplate{footline}{
\ifdefined\insertfootercontent
\begin{beamercolorbox}[vmode]{headline}
\ifbeamercolorempty[bg]{headline rule}{}{
\begin{beamercolorbox}[wd=\paperwidth,colsep=0.25ex]{headline rule}\end{beamercolorbox}
}
\vspace{1.5ex}
\hspace{\sepwidth}
\usebeamerfont{footline}
\centering
\insertfootercontent
\hspace{\sepwidth}
\vspace{1.5ex}
\end{beamercolorbox}
\else\fi
}

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@@ -1,9 +0,0 @@
@article{shannon1948communication,
author = {Claude E. Shannon},
title = {A Mathematical Theory of Communication},
journal = {Bell System Technical Journal},
year = 1948,
volume = {27},
number = {3},
pages = {379-423},
}

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%! TeX Program = lualatex
% Gemini theme
% https://github.com/anishathalye/gemini
\documentclass[final]{beamer}
% ====================
% Packages
% ====================
\usepackage[T1]{fontenc}
\usepackage{lmodern}
\usepackage[size=custom,width=120,height=72,scale=1.0]{beamerposter}
\usetheme{gemini}
\usecolortheme{gemini}
\usepackage{graphicx}
\usepackage{booktabs}
\usepackage{tikz}
\usepackage{pgfplots}
\pgfplotsset{compat=1.14}
\usepackage{anyfontsize}
% ====================
% Lengths
% ====================
% If you have N columns, choose \sepwidth and \colwidth such that
% (N+1)*\sepwidth + N*\colwidth = \paperwidth
\newlength{\sepwidth}
\newlength{\colwidth}
\setlength{\sepwidth}{0.025\paperwidth}
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\title{Some fancy title: followed by some more text}
\author{Alyssa P. Hacker \inst{1} \and Ben Bitdiddle \inst{2} \and Lem E. Tweakit \inst{2}}
\institute[shortinst]{\inst{1} Some Institute \samelineand \inst{2} Another Institute}
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\chapter*{Acknowledgements}
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\section{Sagittarius \texorpdfstring{A$^*$}{A*} (\textit{IXPE})}
\hspace{\parindent}The very first hard X-ray (8.5 -- 22~keV) images of the extended emission situated around the Galactic Center's supermassive black hole Sgr~A$^*$ were taken using the International Astrophysical Observatory \textit{GRANAT}. They revealed elongated emission parallel to the Galactic plane\cite{Sunyaev1993}, whereas soft X-ray emission is known to be more circularly-shaped\cite{Watson1981}. Theoretically, this asymmetry could be due to Thomson scattering of high energy photons by dense molecular gas clouds, such as the Giant Molecular Clouds (GMCs). And, indeed, X-ray observations of the GMCs have revealed fluorescent X-ray emission from cold iron atoms, a steep spectrum and a reflection continuum\cite{Koyama1996,Murakami2000,Churazov2002}, indicating that the GMCs act like reflecting mirrors. Basic scattering physics tells us that the reflected (polarized) X-ray radiation should lead to a map of the three-dimensional position of the clouds with respect to the illuminating source, together with revealing the position and luminosity history of the original source\cite{Vainshtein1980}. However, there is currently no persistent source bright enough ($\text{L}_{X} \ge 10^{39} \; \text{erg} \cdot \text{s}^{-1}$) to be the progenitor of the reflected radiation. From spectroscopic, imaging and timing arguments, numerous authors have speculated that Sgr~A$^*$ could have been much brighter in the past despite being presently dim\cite{Sunyaev1993,Churazov2002,Koyama1996,Murakami2000}. What we observe are just echoes of long-gone bright phases. If true, it means that the Galactic Center was similar to a low-luminosity Active Galactic Nucleus\cite{Ptak2001,Halderson2001} (LLAGN) in the past, with an X-ray luminosity $\sim 10^{40} \; \text{erg} \cdot \text{s}^{-1}$. Determining the activity period(s) of the bright X-ray emission is crucial to understand the duty cycle of black hole mass accretion\cite{Narayan1994,Elitzur2006}, the formation of AGN winds and torus\cite{Konigl1994,Elitzur2006}, and the spin evolution of primordial black holes \cite{Berti2008}.
\subsection*{Observation and data reduction problems}
\hspace{\parindent}The Sgr~A region nearby the central SMBH in the Galactic Center was observed with \textit{IXPE} twice in 2022: both in February and March. The total integration time amounts for about $1$Ms on the clock. As this source is expected to be faint and extended, it required the best possible seeing conditions and longest integration time. However the observation period matched with an increased solar activity period, which led to increased atmospheric noise and spurious events of geomagnetic storm. To analyse the data, an additional filtering is then required to remove noise and background events from the actual target observation.\par
The \textit{IXPE} spacecraft is on a low orbit ($\sim 600$km) at $\sim 0^\circ$ inclination to minimize the time spent above the South Atlantic Anomaly (SAA). This region produces atmospheric noise at high energy and seems to be dependent on solar activity. When passing above this region, the detectors onboard \textit{IXPE} are then turned off and the observation is resumed upon exit. As can be seen in Fig. \ref{fig:SgrAnoisy}, the light curve of the observation is heavily dominated by noise. Assuming an enlargement of the SAA due to increased solar activity, it is possible that the detector off-time does not match the time spent in the SAA and could then explain the increased background flux right before and after SAA pass-related off-times (see appendix \ref{Afig:Filtcorr}). Using \textsc{ixpeobssim} to predict the intervals corresponding to a target occulted by the Earth and the satellite trajectory above the noisy SAA, I successfully determined revised Good Time Intervals (GTIs\footnote{The GTI file contains the start and stop times of all accepted time intervals over the observation. The "good times" are periods when observing conditions were good: acceptable aspect solution and low background.}). This allowed me to perform some first-order filtering. I also had to fit the offset between the simulated observation time and the actual observation time to account for the true orbital parameters of the spacecraft (see appendix \ref{Afig:SgrAfilt}) and filter out a few geomagnetic storm events that occurred during the acquisition. The result is given in Fig. \ref{fig:SgrAnoisy}, where we can see that our assumption that the SAA has been enlarged can account for the detected noise and that our filtering effectively re-define the GTIs. After this filtering, we are left with a corrected Total GTI of $930,566$sec, which represents $96.7$\% of the original Total GTI. This filtering has been compared to other methods tried by different collaborators and yielded similar results (see appendix \ref{Afig:SgrAmultiplefilt}). My properly reduced list of events was then used for the analysis of the observation.
\begin{figure}[!ht]
\centering
\includegraphics[width=\textwidth]{./parts/appendix/SgrA_LC_SAA_large.png}
\caption{Color-coded lightcurve of the observation of SgrA$^*$ by \textit{IXPE} with in \textbf{\textcolor{blue}{blue}} the corrected GTIs, in \textbf{\textcolor{green}{green}} the time in the Earth's shadow (target occulted), in \textbf{\textcolor{red}{red}} the time in the enlarged SAA and in \textbf{\textcolor{black}{black}} the events corresponding to a geomagnetic storm.}
\label{fig:SgrAnoisy}
\end{figure}
\subsection*{Analysis of the data}
\hspace{\parindent}The previously filtered observation allowed us to analyse the underlying real flux from the Galactic Center. The target of this observation was a series of GMCs named the "Sagittarius A complex". Any detected polarization in the X-ray band would hint to the scattering of a past, long-lived X-ray outburst from the close-by SMBH Sgr~A$^*$. For this scenario to be valid, the angle of polarization must be normal to the line connecting the emission source and the scattering cloud. Then the polarization degree will inform us on the scattering angle (according to the Malus law), giving us the missing $z$-axis information of the cloud(s), allowing us to access the true distance of the scattering medium from the emission source.\par
The analysis of the \textit{IXPE} data yielded both polarization angle and degree coherent with the scattering of a past outburst of the central SMBH (see Fig. \ref{fig:SgrAanalysis}). The polarization degree exceeds $1$\% and the polarization angle is $\approx 133^\circ$, which is perpendicular to the position angle of the SMBH ($\sim 45^\circ$). The detected reflection is the record of a past active phase of the now quiescent Sgr~A$^*$. The data still need refinement to better locate the position of each GMC in the Sgr~A region, but the projected distance tells us that Sgr~A$^*$ was active in the past, around 400 years ago. The estimated X-ray luminosity necessary to produce such detectable feature in the X-ray corresponds to the activity of a low-luminosity AGN. This promising result allow us to do achieve, for the first time, Galactic archaeology and we are on the verge of characterizing its accretion-evolution history.
\begin{figure}[!ht]
\centering
\begin{subfigure}{0.5\textwidth}
\centering
\includegraphics[width=0.9\textwidth]{./parts/appendix/SgrA_avg_pol.png}
\captionsetup{width=0.9\textwidth}
\caption{\footnotesize Polarization components as a function of the confidence level for the emission from the targeted molecular cloud averaged on the 3 detector units of \textit{IXPE}.}
\label{fig:SgrApol}
\end{subfigure}%
\begin{subfigure}{0.5\textwidth}
\centering
\includegraphics[width=0.9\textwidth]{./parts/appendix/SgrA_img_pol.png}
\captionsetup{width=0.9\textwidth}
\caption{\footnotesize Imaging of the Sagittarius A complex by \textit{IXPE} showing the detected polarization angle coherent with a reflected event.}
\label{fig:SgrAimg}
\end{subfigure}
\caption{First analysis of the observation of the Sagittarius A complex with (a) the determination of the polarization components and (b) the corresponding imaging. The detected polarization is coherent with the reflection of a past X-ray outburst from SgrA$^*$ reflected on a molecular cloud.}
\label{fig:SgrAanalysis}
\end{figure}
\section{Centaurus A (\textit{IXPE})}
\hspace{\parindent}Centaurus~A (Cen~A) is a nearby ($z = 0.00183$, $d \approx 3.84$~Mpc) radio-loud AGN that has been known for more than 175 years \cite{Herschel1847}. Its optical spectrum classifies it as a type-2 AGN, i.e. seen from the edge, where the nuclear light of the central SMBH and its accretion disk is obscured by a thick reservoir of dust and gas known as the ``torus'' \cite{Antonucci1993}. Due to its proximity, Cen~A has been observed at high spatial resolution despite its relatively low bolometric luminosity (a few $10^{43} \; \text{erg} \cdot \text{s}^{-1}$, \cite{Beckmann2011}) with respect to standard type-2 AGNs (a few $10^{44} \; \text{erg} \cdot \text{s}^{-1}$, \cite{Lusso2012}). In particular, the complex morphology of the jets and lobes detected from each side of the core has been explored in details. Only apparent in the radio and X-ray bands, those jets become sub-relativistic at a few parsec from the nucleus before expending into plumes at a projected distance of $5$kpc, ending their propagation in space in the form of huge radio lobes extending out to $250$kpc \cite{Israel1998}.\par
The core of Cen~A, however, is not only obscured by the spatially unresolved parsec-scale torus but also by a gigantic warped dust lane which effectively bisects the main body of the host galaxy, partially shrouding the nucleus and all optical structure in the inner $500$pc \cite{Schreier1996}. This dust lane is thought to be the remnant signature of a $10^7$ -- $10^8$ years old merger of Cen~A's host galaxy with a smaller spiral galaxy \cite{Baade1954,Malin1983,Israel1998} that could be responsible for the activity of the nucleus. The host galaxy of Cen~A is actually a giant, moderately triaxial, elliptical galaxy that contains large amounts of dust, atomic and molecular gas as well as luminous young stars \cite{Israel1998}. The excess of obscuring material is unfortunate as the nucleus is likely the place where the high energy photons detected by Cherenkov telescopes \cite{Grindlay1975}, EGRET \cite{Hartman1999}, HESS \cite{Aharonian2009} and Fermi \cite{Abdo2010a} are produced. Determining the mechanisms responsible for the acceleration of photons and particles to ultra high energies is fundamental for understanding the physics of cosmic $\gamma$-ray emitters and in particular the role of radio-galaxies as highly efficient relativistic electron accelerators. Because of their large number, these would collectively contribute, in a very significant way, to the redistribution of energy in the intergalactic medium \cite{Velzen2012}.
\subsection*{Observation preparation}
\hspace{\parindent} I seized the opportunity of \textit{IXPE}'s observation of Cen~A ($100$ks in February 2022) to investigate the true core polarization of this dust-enshrouded AGN. To do so, I not only used \textit{IXPE} results but also correlated the X-ray polarimetric data to other polarized information acquired in various wavelength bands. I searched the SAO/NASA Astrophysics Data System Abstract Service for all papers mentioning a past polarimetric measurement of the core of Cen~A. I discarded all radio polarization campaigns measuring the total (core plus jets plus lobes) polarization of Cen~A, since the lobes are known to strongly dominate the polarization from the core at most radio frequencies \cite{Burns1983,Goddi2021}. In total, there are only 13 papers reporting a polarization measurement from Cen~A's core, most of them in the near-infrared band. The data points cover almost the full electromagnetic spectrum, from the radio to the $\gamma$-ray band, the high energy emission coming from the base of the jets, see Fig.~\ref{fig:CenAmultiSED}.\par
\begin{figure}[!ht]
\centering
\includegraphics[width=\textwidth]{./parts/appendix/CenA_multi_SEDpol.png}
\caption{Spectral Energy Distribution of the core of Cen A, color-coded in aperture size, where the solid dots are the total flux and the hollow dots are the polarized flux, all taken from the literature, except for the \textit{IXPE} point at 5 keV.}
\label{fig:CenAmultiSED}
\end{figure}
The total flux and polarized Spectral Energy Distribution (SEDs) of Cen~A allowed me to determine the presence of the following processes:
\begin{itemize}
\item \textbf{Radio}: synchrotron emission dominates, with a low ($< 1$\%) polarization degree due to the optically thick nature of the emission region and the associated polarization position angle may be perpendicular to the jet axis.
\item \textbf{Millimeter}: starburst emission onsets and the coherent large-scale magnetic fields are dominated by randomly oriented fields, inducing a strong depolarization around the mm-break.
\item \textbf{Far-infrared}: dichroic emission from the dust lane and/or the AGN torus prevails over the core synchrotron polarization. The polarization angle is perpendicular to the jet axis.
\item \textbf{Mid-infrared}: dichroic absorption modifies the core synchrotron polarization and imposes a polarization angle parallel to the jet axis
\item \textbf{Near-infrared}: scattering of synchrotron seed core photons off the AGN polar outflows produces high polarization degrees associated with a polarization position angle perpendicular to the jet axis.
\item \textbf{Optical/near-ultraviolet}: the polarization of synchrotron seed core photons traveling through the dust lanes is altered by dichroic transmission from aligned dust grains. The polarization position angle rotates with decreasing wavelengths, marking the transition between synchrotron and inverse-Compton regimes.
\item \textbf{X-rays\footnote{Polarization observed by \textit{IXPE} and analysed in the next subsection.}}: inverse-Compton scattering dominates. The polarization angle is parallel to the jet axis but the polarization degree is yet to be measured (constrained by our \textit{IXPE} study at values lower than 6.5\%).
\item \textbf{$\gamma$-rays}: inverse-Compton scattering in the jets dominates. The polarization is yet to be measured.
\end{itemize}
\subsection*{Analysing the X-ray emission mechanism}
The upper limit to the degree of polarization measured by \textit{IXPE} (6.5\%, see Fig.~\ref{fig:CenAanalysis}) provides important information about the particle population responsible for generating the X-rays. Given the low polarization degrees measured for Cen~A in the radio and IR bands, however, it is not surprising that significant polarization was not measured in the \textit{IXPE} bandpass. The measured limits for the X-ray polarization degree remain consistent with expectations from synchrotron self-Compton emission, where the polarization degree of the Compton scattered X-rays is predicted to be $\sim 2-5$ times smaller than that of the synchrotron radiation acting as seed photons for Compton scattering. Thus with a significantly longer exposure with \textit{IXPE}, where MDP$_{99}$ could reach levels of $\sim 1\%$, the detection of polarization would be a strong argument in favor of synchrotron radiation as a source of seed photons for Compton scattering.
The observed limits on X-ray polarization are in tension with a physical scenario where the X-ray emission arises from hadronic jets. Processes involving hadrons in jets have been suggested as a possible source of the higher than expected emission of Cen~A at TeV energies \cite{Abdo2010}, and such models applied to blazars predict X-ray polarization degrees as high as $\sim 50-80\%$, much higher than the observed limits allow \cite{Zhang2013}.
\begin{figure}[!ht]
\centering
\begin{subfigure}{0.55\textwidth}
\centering
\includegraphics[width=0.9\textwidth]{./parts/appendix/CenA_Core_avg_pol.png}
\captionsetup{width=0.9\textwidth}
\caption{\footnotesize Analysis of the polarization components as a function of the confidence level for the emission from the core of Cen~A averaged on the 3 detector units of \textit{IXPE}.}
\label{fig:CenApol}
\end{subfigure}%
\begin{subfigure}{0.45\textwidth}
\centering
\includegraphics[width=\textwidth]{./parts/appendix/CenA_img_pol.png}
\captionsetup{width=0.9\textwidth}
\caption{\footnotesize Imaging of the AGN core of Cen~A by \textit{IXPE} showing the contribution of each feature to the total detected flux.}
\label{fig:CenAimg}
\end{subfigure}
\caption{Observed degree of polarization as a function of confidence level (left) and total flux map of Cen~A (right) as observed by IXPE.}
\label{fig:CenAanalysis}
\end{figure}
\section{IC~5063 (\textit{HST/FOC})}
\hspace{\parindent}IC~5063 is a nearby\footnote{From the NASA/IPAC Extragalactic Database.} ($z = 1.011358$, $d \approx 4.27$~Gpc) elliptical, type II \cite{Inglis1993} galaxy. It is one of the most radio-loud ($P_{1.4 \text{GHz}} = 6.3 \cdot 10^{23} \; \text{W} \cdot \text{Hz}^{-1}$ \cite{Morganti1998}) Seyfert 2 galaxies in the local universe. It shows an ionizing radiation field with an “X” morphology \cite{Colina1991} and a complex system of dust lanes, likely due to merger remnants \cite{Morganti1998,Oosterloo2017}. High-resolution radio data (ATCA at 8 GHz \cite{Morganti1998}) reveal a triple radio structure ($1.3$ kpc) along the position angle (PA) of $\sim 295^\circ$ with a total flux density of $230$ mJy, consisting of a nuclear blob and two hot spots, i.e., termination points where the jets collide with the gas. Most of the flux ($195$ mJy) is emitted from the North-West radio hot spot. IC~5063 is a perfect laboratory to explore AGN interaction with the medium of its host galaxy: it is a peculiar system because the radio jets lie in the same plane as the \emph{HI} galactic disk (PA $\sim 300^\circ$ \cite{Danziger1981,Morganti1998}), allowing a full interaction between the mechanical energy released by the AGN and the host galaxy.\par
This AGN is also strongly obscured by both a dust lane in front of the galaxy and the dusty torus around its core. The latter have recently been observed thanks to the fact that the AGN is highly inclined with its host galaxy \cite{Maksym2020}.
\subsection*{IC~5063 and Cen~A: twin AGN}
\hspace{\parindent}Among the observed but not analyzed datasets in the \textit{HST/FOC} archives, IC~5063 got our attention as it shows characteristics very similar to Cen~A. Indeed, both of them are radio-loud AGNs with strong jets that are interacting with their respective host galaxy, but most importantly they are both obscured by a foreground dust lane. Their core emission is completely obscured and no one knows if the central source is dominated by thermal accretion onto a SMBH or by synchrotron emission by the jet bases. Because Cen~A was never observed by the \textit{HST/FOC} it is impossible to investigate it in the UV band, but we took the opportunity to use its twin to test the synchrotron origin predicted by \textit{IXPE} for Cen~A.
\subsection*{Total and polarized fluxes in UV}
\hspace{\parindent}On February 25$^\text{th}$ 1998, the \textit{HST/FOC} observed IC~5063 for $5261.875$ seconds through each polarizer filter ($0^\circ$, $60^\circ$ and $120^\circ$). This dataset has only one associated paper that does not make use of the polarization information that can be deduced from it \cite{Dasyra2015}. Thus, the following results consist in the first UV polarimetric analysis of IC~5063.\par
We used our pipeline to reduce and analyse this dataset comprising 3 observations. The resulting polarization map with vectors displayed at full scale to better study the pattern they form is shown in Fig. \ref{fig:IC5063UV}. The polarization vectors are displayed on-top of the intensity map for a confidence level on the polarization degree $\text{SNR}_P = \frac{\sigma_P}{P} \geq 3$ and on the flux intensity $\text{SNR}_I = \frac{\sigma_I}{I} \geq 60$, which corresponds to highly significant polarization detection only.\par
The UV intensity map allows us to reveal the morphology of the AGN and compare it to what was presented in previous papers: on the South-East, a jet and its lobe are revealed thanks to high fluxes in the UV band; in the center, the core of the AGN might be located in a heavily obscured region right to the South of the brightest total flux spot (remember that the SMBH is hidden by a torus, so we don't know it's real location); finally on the North-West part, a less intense jet and its lobe seems to be diverging in the upper part of a "X" pattern (the lower part being on the South-East of the SE lobe). When analysing the flux from these different regions we get that the SE lobe is $2.5$ times brighter than the NW lobe. This can be due to both less extinction from dust and more scattering by the medium.\par
The integrated values of polarization degree and angle on the $7$x$7$ arcseconds$^2$ of the \textit{HST/FOC} aperture of respectively $1.6$\% and $162^\circ$ can be surprising at first as we expect integrated polarization degree of $10$--$20$\% around Type 2 AGNs (see for example Fig. \ref{fig:NGC1068CapettiUs} and Fig. \ref{Afig:NGC1068analysis} for NGC~1068). This can be explained by a highly depolarized region around the center of the AGN plus the contamination by dichroic transmission through interstellar dust, which is coherent with our detected polarization components (see Fig. \ref{fig:IC5063ISP}). However, on the North-West extremity of the NW lobe we can see a centro-symmetric polarization pattern that is typical of the emission from the central core that is scattered on ionized polar winds onto our line-of-sight. This particular region has a polarization degree of $5.7$\% and a polarization angle of $11.6^\circ$, almost perpendicular to the jets direction. By taking the normal to the vectors in this region we can locate the obscured core of the AGN with great precision, even if it is hidden by an optically thick dust reservoir.
\begin{figure}[!ht]
\centering
\includegraphics[width=\textwidth]{./parts/appendix/IC5063_FOC_combine_FWHM020_pol.png}
\caption{UV polarization map obtained with our new pipeline where we can see in intensity the location of both jets and lobes and the central core. The polarization vectors are all represented at full size to better study the patterns they form.}
\label{fig:IC5063UV}
\end{figure}
\begin{figure}[!ht]
\centering
\includegraphics[width=0.8\textwidth]{./parts/appendix/ISP.png}
\caption{Polarization degree and angle measurement as a function of the wavelength and color-coded by aperture size for the emission from IC~5063. The dotted line represent the expected polarization from scattering on interstellar dust.}
\label{fig:IC5063ISP}
\end{figure}
\subsection*{Relation to radio and infrared maps}
\hspace{\parindent}To better understand the rest of the polarization patterns that does not bear the usual signature of an AGN and seem chaotic to us at first glance, we correlated to our results information from other wavelength (see Fig. \ref{fig:IC5063multiwav}). We use polarized radio flux measurements from ATCA (Fig. \ref{fig:IC5063Radio}) and near-infrared map of the AGN surroundings from HST (Fig. \ref{fig:IC5063IR}) to identify structures associated with radio emission and/or dust absorption around the core, jets, lobes and the host galaxy.\par
The radio emission identifies the approaching jet to be the North-West one. Its lobe emission is $16$ times brighter than the South-East lobe associated with the counter-jet (see Fig. \ref{fig:IC5063Radio}). This hierarchy in radio intensity is the opposite to what we see in the UV intensity maps, and can be explained by the fact that the former results from isotropic emission in the shocks at the boundaries of the lobes, while the latter results from scattering of the emission from the core on turbulent medium (less absorbed in the counter-jet associated lobe).\par
The inverted scale for the display of the near-IR map highlights the position of the dust clouds in the field-of-view (see Fig. \ref{fig:IC5063IR}). We can see that the region that is directly North of the AGN core in the UV map (see Fig. \ref{fig:IC5063UV}), where almost no UV flux is detected, correlates in IR to a foreground dust lane that absorbs the UV emission. We thus pinpoint with precision the regions of the AGN that are heavily polluted by the galaxy merger.
\begin{figure}[!ht]
\centering
\begin{subfigure}{0.5\textwidth}
\centering
\includegraphics[width=\textwidth]{./parts/appendix/IC5063_18GHz_overplot_forced.png}
\captionsetup{width=0.9\textwidth}
\caption{\footnotesize Superposition of our UV polarization map with radio contours at 18GHz by Morganti et al. \cite{Morganti1998}. This highlights the jet propagation through the host galaxy medium.}
\label{fig:IC5063Radio}
\end{subfigure}%
\begin{subfigure}{0.5\textwidth}
\centering
\includegraphics[width=\textwidth]{./parts/appendix/IC5063_IR_overplot_forced.png}
\caption{\footnotesize Superposition of a near-infrared map taken with \textit{HST/WFPC} with the polarization vectors from our UV map. This highlights the alignment of the polarization pattern along the foreground dust lane.}
\label{fig:IC5063IR}
\end{subfigure}
\caption{Multiwavelength analysis of IC~5063 with (a) the UV polarization map overplotted with 18GHz radio contours, (b) a near-infrared map from the \textit{HST/WFPC} overplotted with our UV polarization vectors.}
\label{fig:IC5063multiwav}
\end{figure}
\subsection*{Dissecting the AGN}
\hspace{\parindent}Correlating the UV polarization map to radio and infrared spatial features allowed us to emit a certain number of hypothesis to explain the different polarization patterns visible in the UV band. Beginning in the innermost regions of the AGN we can see in infrared and UV that the thermal emission from the core seems to be obscured by the putative dusty torus from the AGN model. Radiation manages to escape a few milliarcseconds North of the core by perpendicular scattering. A bit further, the path of the jets is completely depolarized in UV and this might be due to the jets pushing the surrounding material around, creating turbulences and removing the scattering medium from the jets axis. The depolarization can also be due to superposition of the perpendicular polarization angle coming from the synchrotron emission from the jets and scattering of the core emission on turbulent medium at the same location. This can also explain the centro-symmetric pattern on the North-West of the approaching lobe, where scattering on ionized winds is still possible as they have not yet been perturbed by the jet.\par
We explain the UV extinction and the aligned polarization vectors on the Northern part of the AGN by the presence of a foreground dust lane, visible in infrared, that produces polarization through forward scattering on aligned dust grains. This extinction and emission by aligned grains in the dust lane produces polarization by dichroic transmission, allowing us to characterize the mineralogy and geometry of the dust cloud.\par
Comparing the different sources of polarization to the integrated polarization (see Fig. \ref{fig:IC5063UV}) on the \textit{HST/FOC} aperture, we can say that the dominant mechanism could indeed be dichroic transmission on interstellar dust, but not necessarily from the Milky Way. It is rather due to the foreground dust lane that is located near the IC~5063 host galaxy. Its precise distance from the AGN is yet to be determined. A way to guess the proximity to the AGN would be to study the mechanism that align the dust grains in the cloud. Their alignment seems indeed to be parallel to the jets axis and this mean that there could be a mechanical alignment of the grains by kinetic pressure from the matter pushed around by the relativistic jets. Another scenario would imply a large scale magnetic field, similar to what have been observed in the infrared in the foreground dust lane of Cen~A \cite{Lopez-Rodriguez2021}.

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% \documentstyle[11pt,aas_macros]{article}
%
% For more information on the AASTeX and A&A packages, please see:
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% ftp://ftp.edpsciences.org/pub/aa/readme.html
% For more information about ADS abstract server, please see:
% http://adsabs.harvard.edu/ads_abstracts.html
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\def\pasj{\ref@jnl{PASJ}} % Publications of the ASJ
\def\rmxaa{\ref@jnl{Rev. Mexicana Astron. Astrofis.}}%
% Revista Mexicana de Astronomia y Astrofisica
\def\qjras{\ref@jnl{QJRAS}} % Quarterly Journal of the RAS
\def\skytel{\ref@jnl{S\&T}} % Sky and Telescope
\def\solphys{\ref@jnl{Sol.~Phys.}} % Solar Physics
\def\sovast{\ref@jnl{Soviet~Ast.}} % Soviet Astronomy
\def\ssr{\ref@jnl{Space~Sci.~Rev.}} % Space Science Reviews
\def\zap{\ref@jnl{ZAp}} % Zeitschrift fuer Astrophysik
\def\nat{\ref@jnl{Nature}} % Nature
\def\iaucirc{\ref@jnl{IAU~Circ.}} % IAU Cirulars
\def\aplett{\ref@jnl{Astrophys.~Lett.}} % Astrophysics Letters
\def\apspr{\ref@jnl{Astrophys.~Space~Phys.~Res.}}
% Astrophysics Space Physics Research
\def\bain{\ref@jnl{Bull.~Astron.~Inst.~Netherlands}}
% Bulletin Astronomical Institute of the Netherlands
\def\fcp{\ref@jnl{Fund.~Cosmic~Phys.}} % Fundamental Cosmic Physics
\def\gca{\ref@jnl{Geochim.~Cosmochim.~Acta}} % Geochimica Cosmochimica Acta
\def\grl{\ref@jnl{Geophys.~Res.~Lett.}} % Geophysics Research Letters
\def\jcp{\ref@jnl{J.~Chem.~Phys.}} % Journal of Chemical Physics
\def\jgr{\ref@jnl{J.~Geophys.~Res.}} % Journal of Geophysics Research
\def\jqsrt{\ref@jnl{J.~Quant.~Spec.~Radiat.~Transf.}}
% Journal of Quantitiative Spectroscopy and Radiative Transfer
\def\memsai{\ref@jnl{Mem.~Soc.~Astron.~Italiana}}
% Mem. Societa Astronomica Italiana
\def\nphysa{\ref@jnl{Nucl.~Phys.~A}} % Nuclear Physics A
\def\physrep{\ref@jnl{Phys.~Rep.}} % Physics Reports
\def\physscr{\ref@jnl{Phys.~Scr}} % Physica Scripta
\def\planss{\ref@jnl{Planet.~Space~Sci.}} % Planetary Space Science
\def\procspie{\ref@jnl{Proc.~SPIE}} % Proceedings of the SPIE
\makeatother
\let\astap=\aap
\let\apjlett=\apjl
\let\apjsupp=\apjs
\let\applopt=\ao

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@@ -1,4 +0,0 @@
\chapter*{Glossary}
\chaptermark{Glossary}
\markboth{GLOSSARY}{PUBLICATIONS}
\addcontentsline{toc}{chapter}{Glossary}

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@@ -1,17 +1,17 @@
\chapter{Chapter 1 title}
\chaptermark{Chapter 1 title in header}
\label{ch:chapter1}
%\adjustmtc
\graphicspath{{Figures/Ch1/}}
\minitoc
\section{First Section of first chapter}
\subsection{Let's talk about A}
I must quote \citet{FavoriteAuthor} because they did a great job.
I must quote \citet{FavoriteAuthor} because they did a great job looking at this type of \gls{GAL}.
\subsection{And now B}
...
We can even reuse the acronym to plural: \glspl{GAL}
\section{But what about this}

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@@ -1,7 +1,7 @@
\chapter{Chapter 2 title}
\chaptermark{Chapter 2 title in header}
\label{ch:chapter2}
%\adjustmtc
\graphicspath{{Figures/Ch2/}}
\minitoc

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@@ -1,7 +1,7 @@
\chapter{Chapter 3 title}
\chaptermark{Chapter 3 title in header}
\label{ch:chapter3}
%\adjustmtc
\graphicspath{{Figures/Ch3/}}
\minitoc
\section{Look at this Table}

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@@ -1,6 +0,0 @@
\chapter*{Abstract}
\chaptermark{Abstract}
\markboth{ABSTRACT}{ABSTRACT}
\addcontentsline{toc}{chapter}{Abstract}
...

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@@ -1,6 +0,0 @@
\chapter*{R\'esum\'e}
\chaptermark{R\'esum\'e}
\markboth{R\'ESUM\'E}{R\'ESUM\'E}
\addcontentsline{toc}{chapter}{R\'esum\'e}
...

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@@ -5,26 +5,26 @@
\setlength\evensidemargin{\oddsidemargin}
\makeatletter
\begin{changemargin}{-15mm}{-5mm}
\begin{changemargin}{-25mm}{-15mm}
\noindent%
\vspace*{-20mm}%
\begin{center}%
\includegraphics[keepaspectratio, height=8mm, trim={0 8mm 0 0}]{\@UniversityLogo}%
\includegraphics[keepaspectratio, height=14mm, valign=c]{\@UniversityLogo}%
\hfill%
{\Large\bf \@Firstname\, \MakeUppercase{\@Lastname}}%
{\LARGE\bf \@Firstname\, \MakeUppercase{\@Lastname}}%
\hfill%
\includegraphics[keepaspectratio, height=8mm, trim={0 8mm 0 0}]{\ifdefempty{\@LaboLogo}{\@DoctoralSchoolLogo}{\@LaboLogo}}%
\includegraphics[keepaspectratio, height=12mm, valign=c]{\ifdefempty{\@LaboLogo}{\@DoctoralSchoolLogo}{\@LaboLogo}}%
\end{center}%
\end{changemargin}\vspace*{1cm}%
\begin{changemargin}{-10mm}{0mm}
\begin{changemargin}{-23mm}{-13mm}
\begin{center}
{\LARGE\bf \@TitreThese}%
\end{center}
\begin{mybox}
{\Large\textbf{Résumé}}\vspace*{5mm}
\@resume
\@resume\PhDThesis@checkResume
\vspace*{5mm}
\textbf{Mots-clés}: \@motscles
@@ -36,7 +36,7 @@
\begin{mybox}
{\Large\textbf{Abstract}}\vspace*{5mm}
\@abstract
\@abstract\PhDThesis@checkAbstract
\vspace*{5mm}
\textbf{Keywords}: \@keywords

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@@ -6,24 +6,24 @@
\setlength\evensidemargin{\oddsidemargin}
\makeatletter
\begin{changemargin}{-15mm}{-5mm}
\begin{changemargin}{-25mm}{-15mm}
\noindent
\vspace*{-25mm}%
\begin{center}%
\includegraphics[keepaspectratio, height=1.5cm]{\@UniversityLogo}%
\ifdefempty{\@LaboLogo}{}{\hfill\includegraphics[keepaspectratio, height=1.5cm]{\@LaboLogo}}%
\includegraphics[keepaspectratio, height=1.5cm,valign=c]{\@UniversityLogo}%
\ifdefempty{\@LaboLogo}{}{\hfill\includegraphics[keepaspectratio, height=1.5cm,valign=c]{\@LaboLogo}}%
\hfill%
\includegraphics[keepaspectratio, height=1.8cm, trim={0 3.0mm 0 0}]{\@DoctoralSchoolLogo}\\\vspace{5mm}
\includegraphics[keepaspectratio, height=1.75cm,valign=c]{\@DoctoralSchoolLogo}\\\vspace{5mm}
{\ifdefempty{\@LaboLogo}{\vspace{-15mm}}{}\Large\bf \MakeUppercase{\@UniversityName}}\\\vspace{10mm}
{\large\bf\textit{\MakeUppercase{\@DoctoralSchoolName}}}\\\vspace{5mm}
{\bf \@LaboName}
\end{center}
\end{changemargin}
\vfill%
\begin{changemargin}{-10mm}{0mm}
\begin{changemargin}{-15mm}{0mm}
\begin{center}
\huge \textbf{TH\`ESE} \large pr\'esent\'ee par\\\vspace{5mm}
{\LARGE\bf\@Firstname\, \MakeUppercase{\@Lastname}}\\\vspace{5mm}
{\LARGE\bf \@Firstname\, \MakeUppercase{\@Lastname}}\\\vspace{5mm}
{\large soutenue le: \bfseries \@ThesisDate}\vspace{5mm}
\begin{tabular}{rl}
@@ -40,7 +40,7 @@
\end{center}%
\end{changemargin}%
\vfill%
\begin{changemargin}{-15mm}{-5mm}
\begin{changemargin}{-25mm}{-15mm}
{\large\bfseries THÈSE dirigée par}:\vspace{2mm}
\begin{tabular}{p{7cm}p{10cm}}%

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Thesis/NAME_Thesis.pdf Normal file

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@@ -1,22 +1,21 @@
%\documentclass{PhDThesisED182}
\documentclass[showNotes, showLineNumbers]{PhDThesisED182}
%! TeX Program = pdflatex
%! TeX Root = ./NAME_Thesis.tex
%\documentclass{PhDThesis}
\documentclass[showNotes,showLineNumbers]{PhDThesis}
%\modulolinenumbers[5] % Change line numbering every N lines
%\renewcommand{\familydefault}{\sfdefault} % Uncomment to default to sans serif font
%%%%%%%%%%%%%%%% Fill in for Front and Back Covers %%%%%%%%%%%%%%%%
% Author
\Firstname{Firstname}
\Lastname{Lastname}
\author{Firstname}{Lastname}
% University
\UniversityName{Universit\'e de Strasbourg}
\UniversityLogo{Images/Covers/Logo\_StrasbourgUni.pdf}
\University{Universit\'e de Strasbourg}{Figures/Covers/Logo\_Unistra.pdf}
% Labo
\LaboName{Observatoire Astronomique de Strasbourg (UMR 7550)}
\LaboLogo{Images/Covers/Logo\_ObAS.pdf}
\Labo{Observatoire Astronomique de Strasbourg (UMR 7550)}{Figures/Covers/Logo\_ObAS.pdf}
% Doctoral school
\DoctoralSchoolName{\'Ecole Doctorale de physique et chimie-physique}
\DoctoralSchoolLogo{Images/Covers/logo\_ED182.pdf}
\DoctoralSchool{\'Ecole Doctorale de physique et chimie-physique}{Figures/Covers/logo\_ED182.pdf}
% Thesis
\ThesisDate{XX mois 20XX}
\TitreThese{Le titre de la thèse en français.}
@@ -50,61 +49,54 @@
\firstauth{Name}
\addboldnames{{Name, Firstname},{Name, I.}}
\makeglossaries
%%%%%%%%%%%%%%%% Document begin %%%%%%%%%%%%%%%%
\begin{document}
\include{Covers/FrontCover}
\cleardoublepage
\clearemptydoublepage
\pagenumbering{roman}
\dominitoc % use a mini table of contents for each chapter
\ifshowLineNumbers\linenumbers\fi % show line numbers if switched on
\adjustmtc % to avoid minitoc position issue in the following chapters
\include{Chapters/ch-Abstract}
\include{Chapters/ch-Résumé}
\adjustmtc
\include{Chapters/ch-Acknowledgements}
\include{Chapters/ch-Remerciements}
\adjustmtc % to avoid minitoc position issue in the following chapters
\include{Preamble/Acknowledgements}
\include{Preamble/Remerciements}
\tableofcontents
\adjustmtc
\include{Appendices/app-Glossary}
\adjustmtc
\include{Appendices/app-Publications}
\newpage
\listoffigures
\newpage
\listoffigures \mtcaddchapter % do not forget "\mtcaddchapter" (ohterwise, conflict with minitoc)
\listoftables
\newpage
\listoftables \mtcaddchapter
% Define Glossary terms
\include{Preamble/Glossary}
\printglossaries
\adjustmtc
\include{Preamble/Publications}
\cleardoublepage
\pagenumbering{arabic}
\adjustmtc
\include{Chapters/ch-Introduction}
\include{Preamble/Abstract}
\include{Preamble/Resume}
\include{Chapters/ch-Chapter1}
\include{Chapters/ch-Chapter2}
\include{Chapters/ch-Chapter3}
\newpage
\include{Chapters/Chapter1}
\include{Chapters/Chapter2}
\include{Chapters/Chapter3}
\adjustmtc
\include{Chapters/ch-Conclusion}
\begin{appendices}
\include{Appendices/app-AppendixA}
\end{appendices}
\resetboldnames % Remove bold font on \firstauth for global bibliography
\printbibliography
\addcontentsline{toc}{chapter}{Bibliography}
\cleardoublepage
\begin{appendices}
\include{Appendices/AppendixA}
\end{appendices}
\clearemptydoublepage
\include{Covers/BackCover}
\end{document}

282
Thesis/PhDThesis.cls Normal file
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@@ -0,0 +1,282 @@
%%% File: PhDThesis.cls
%%% Brief: Document class template for ED182 thesis manuscript
%%% Use: \documentclass[showNotes, showLineNumbers, showWatermark]{PhDThesis}
%%% Author: Alexandre BIGOT, alexandre.bigot@iphc.cnrs.fr
%%% Tweaks: Thibault BARNOUIN, thibault.barnouin@astro.unistra.fr
%% Identification
%% The class identifies itself and the LaTeX version needed
\NeedsTeXFormat{LaTeX2e}
\ProvidesClass{PhDThesis}[Minimal class for PhD thesis manuscript]
%% Load the article class file
\LoadClass[a4paper,twoside,12pt]{report}
%% Load packages
\RequirePackage{hyperref} % Extensive support for hypertext
\PassOptionsToPackage{a4paper,inner=30mm,outer=20mm,top=25mm,bottom=30mm}{geometry}\RequirePackage{geometry} % Flexible and complete interface to document dimensions
\PassOptionsToPackage{main=english,french}{babel}\RequirePackage{babel} % Multilingual support
\PassOptionsToPackage{T1}{fontenc}\RequirePackage{fontenc} % Standard package for selecting font encodings
\RequirePackage{pdfpages} % Insert pdf as pages
\RequirePackage{lmodern} % Make sure thesis is ready for printing
\RequirePackage{graphicx} % Enhanced support for graphics
\RequirePackage{xcolor} % Driver-independent color extensions
\RequirePackage{amsmath} % AMS mathematical facilities
\RequirePackage{amssymb} % AMS mathematical symbols
\RequirePackage{amsfonts} % TeX fonts from the American Mathematical Society
\RequirePackage{fancyhdr} % Extensive control of page headers and footers
\RequirePackage{caption} % Better captions for tables and figures
\RequirePackage{listings} % For code citing
\RequirePackage{xparse} % For better parameter handling
\PassOptionsToPackage{export}{adjustbox}\RequirePackage{adjustbox} % Framing
% \PassOptionsToPackage{lang-warn=false}{datatool-base}\RequirePackage{datatool-base} % Remove missing datatool warning for french
\PassOptionsToPackage{acronym,toc,nopostdot}{glossaries}\RequirePackage{glossaries} % Create acronym and glossary tables
\PassOptionsToPackage{most}{tcolorbox}\RequirePackage{tcolorbox} % Coloured boxes
\RequirePackage{colortbl} % Coloured row and columns in tables
\PassOptionsToPackage{nottoc}{tocbibind}\RequirePackage{tocbibind} % Add bibliography/index/contents to Table of Contents
\PassOptionsToPackage{nohints,tight}{minitoc}\RequirePackage{minitoc} % Produce a table of contents for each chapter, part or section
\PassOptionsToPackage{title}{appendix}\RequirePackage{appendix} % Extra control of appendices
\let\oldappendices=\appendices
\renewcommand\appendices{\oldappendices\adjustmtc}
\PassOptionsToPackage{modulo}{lineno}\RequirePackage{lineno} % Line numbers on paragraphs
\RequirePackage{macros} % Personal macros for bibliography
%% Switches
\newif\ifshowNotes
\newif\ifshowLineNumbers
%
%% Class options
\DeclareOption{showNotes}{\showNotestrue}
\DeclareOption{showLineNumbers}{\linenumbers} % show line numbers if switched on
\ProcessOptions\relax % to process options
%%%%%%%%%%%%%%%% Commands and default values for Covers %%%%%%%%%%%%%%%%
% Author name
\makeatletter
\newcommand{\Firstname}[1]{\gdef\@Firstname{#1}}
\Firstname{Firstname}
\newcommand{\Lastname}[1]{\gdef\@Lastname{#1}}
\Lastname{Lastname}
\renewcommand{\author}[2]{\Firstname{#1}\Lastname{#2}\hypersetup{pdfauthor={#1 #2},pdfcreator={#1 #2}}}
% University name and logo
\newcommand{\UniversityName}[1]{\gdef\@UniversityName{#1}}
\UniversityName{Universit\'e de Strasbourg}
\newcommand{\UniversityLogo}[1]{\gdef\@UniversityLogo{#1}}
\UniversityLogo{Images/Covers/Logo\_Unistra.pdf}
\newcommand{\University}[2]{\UniversityName{#1}\UniversityLogo{#2}}
% Labo name and logo
\newcommand{\LaboName}[1]{\gdef\@LaboName{#1}}
\LaboName{My Laboratory}
\newcommand*{\LaboLogo}[1]{\gdef\@LaboLogo{#1}}
\LaboLogo{}
\newcommand{\Labo}[2]{\LaboName{#1}\LaboLogo{#2}}
% Doctoral school name and logo
\newcommand{\DoctoralSchoolName}[1]{\gdef\@DoctoralSchoolName{#1}}
\DoctoralSchoolName{\'Ecole Doctorale de physique et chimie-physique}
\newcommand{\DoctoralSchoolLogo}[1]{\gdef\@DoctoralSchoolLogo{#1}}
\DoctoralSchoolLogo{Images/Covers/logo\_ED182}
\newcommand{\DoctoralSchool}[2]{\DoctoralSchoolName{#1}\DoctoralSchoolLogo{#2}}
% Thesis title and subtitle in French and English
\newcommand{\ThesisDate}[1]{\gdef\@ThesisDate{#1}}
\ThesisDate{XX mois 20XX}
\newcommand{\TitreThese}[1]{\gdef\@TitreThese{#1}}
\TitreThese{Le titre de la thèse en français.}
\newcommand*{\SousTitreThese}[1]{\gdef\@SousTitreThese{#1}}
\SousTitreThese{}
\newcommand{\resume}[1]{\gdef\@resume{#1}}
\resume{1000 caract\`eres maximum}
\newcommand{\motscles}[1]{\gdef\@motscles{#1}}
\motscles{...}
\newcommand{\ThesisTitle}[1]{\gdef\@ThesisTitle{#1}\hypersetup{pdftitle={#1}}}
\ThesisTitle{Title of the thesis in english.}
\newcommand*{\ThesisSubTitle}[1]{\gdef\@ThesisSubTitle{#1}}
\ThesisSubTitle{}
\renewcommand{\abstract}[1]{\gdef\@abstract{#1}}
\abstract{1000 letters max}
\newcommand{\keywords}[1]{\gdef\@keywords{#1}\hypersetup{pdfkeywords={#1}}}
\keywords{...}
\newcommand{\PhDThesis@Abstractmaxchars}[1]{\edef\PhDThesis@Abstractmaxchars{#1}}
\PhDThesis@Abstractmaxchars{1000}
% Discipline
\newcommand{\Discipline}[1]{\gdef\@Discipline{#1}}
\Discipline{Physique}
\newcommand*{\Speciality}[1]{\gdef\@Speciality{#1}}
\Speciality{}
%%% Jury members title, name, position and affiliation
\newcommand{\person}[5]{\hspace{2mm}\bfseries{#1\, \MakeUppercase{#2}\, #3} & {#4, #5}\\}
% Directeurs
\newcommand{\directeurs}[1]{\gdef\@directeurs{#1}}
\directeurs{
\person{Civ.}{Lastname}{Firstname}{Pos.}{Affiliation}
\person{Civ.}{Lastname}{Firstname}{Pos.}{Affiliation}
}
% Rapporteurs
\newcommand{\rapporteurs}[1]{\gdef\@rapporteurs{#1}}
\rapporteurs{
\person{Civ.}{Lastname}{Firstname}{Pos.}{Affiliation}
\person{Civ.}{Lastname}{Firstname}{Pos.}{Affiliation}
}
% Jury
\newcommand{\jury}[1]{\gdef\@jury{#1}}
\jury{
\person{Civ.}{Lastname}{Firstname}{Pos.}{Affiliation}
\person{Civ.}{Lastname}{Firstname}{Pos.}{Affiliation}
\person{Civ.}{Lastname}{Firstname}{Pos.}{Affiliation}
}
\makeatother
%% Commands to hide parts from TOC
\newcommand{\nocontentsline}[3]{}
\let\origcontentsline\addcontentsline
\newcommand\stoptoc{\let\addcontentsline\nocontentsline}
\newcommand\resumetoc{\let\addcontentsline\origcontentsline}
\NewDocumentEnvironment{notes}{+b}{\ifshowNotes\color{gray}#1\color{black}\fi}{}
%% Define my colours
\definecolor{DarkBlue}{rgb}{0.0, 0.0, 0.55}
\definecolor{DarkRed}{rgb}{0.55, 0.0, 0.0}
\definecolor{DarkGreen}{rgb}{0.0, 0.2, 0.13}
\definecolor{DodgerBlue}{rgb}{0.12, 0.56, 1.0}
\colorlet{DodgerBlue2}{DodgerBlue!80}
%% Color commands
\newcommand{\mycolor}[2]{\color{#1}#2\color{black}\xspace}
\newcommand{\red}[1]{\color{red}#1\color{black}\xspace}
%% Page formating
\newcommand{\clearemptydoublepage}{%
\newpage{\pagestyle{empty}\cleardoublepage}}
%% Change hyperlinks style
\hypersetup
{
colorlinks=true,
linkcolor=black,
linktocpage=false, % to have the link on the page number in toc
filecolor=magenta,
urlcolor=DodgerBlue,
citecolor=DodgerBlue,
}
\makeatother
\let\oldtoc=\tableofcontents
\renewcommand\tableofcontents{\subpdfbookmark{Table of Contents}{name}{\hypersetup{hidelinks}\oldtoc}}
%
\let\oldlof=\listoffigures
\renewcommand\listoffigures{{\hypersetup{hidelinks}\oldlof\mtcaddchapter}}
%
\let\oldlot=\listoftables
\renewcommand\listoftables{{\hypersetup{hidelinks}\oldlot\mtcaddchapter}}
%
\let\oldpgls=\printglossaries
\renewcommand\printglossaries{
\printglossary[type=\glsdefaulttype,style=altlist,nonumberlist=true]\adjustmtc%
\printglossary[type=\acronymtype]\adjustmtc%
}
%% Fonts substitutions for non existing bold small caps in lmodern
\rmfamily
\DeclareFontShape{T1}{lmr}{b}{sc}{<->ssub*cmr/b/sc}{}
\DeclareFontShape{T1}{lmr}{bx}{sc}{<->ssub*cmr/bx/sc}{}
\sffamily
\DeclareFontShape{T1}{lmss}{m}{sc} { <-> ssub * phv/m/sc }{}
\DeclareFontShape{T1}{lmss}{bx}{sc} { <-> ssub * phv/bx/sc }{}
%% Table of contents configuration
\setcounter{minitocdepth}{3}
\setlength{\mtcindent}{24pt}
\renewcommand{\mtcfont}{\small}
\renewcommand{\mtifont}{\large\bf}
\renewcommand{\mtcSfont}{\small\bf}
\renewcommand{\mtcSSfont}{\small}
%\renewcommand{\mtctitle}{Contents}
%% Section configuration | Change the numerotations of sections
% \renewcommand{\thesection}{\Roman{section})}
% \renewcommand{\thesubsection}{\Roman{section}.\arabic{subsection})}
% \renewcommand{\thesubsubsection}{\Roman{section}.\arabic{subsection}.\alph{subsubsection})}
%% Command to create a glossary entry with correspondent acronym.
%Syntax: \newdualentry[acronym options]{label}{abbrv}{long}{description}
\DeclareDocumentCommand{\newdualentry}{ O{} m m m m } {
\newglossaryentry{#2_gls}{name={#3},
type={\glsdefaulttype},
long={#4},
description={#5},
#1
}
\newacronym[description={#4, \textit{Glossary:} \glslink{#2_gls}{#3} ;},#1]{#2}{#3}{#4\glsadd{#2_gls}}
% \newglossaryentry{#2}{name={#3},
% type={\acronymtype},
% short={#3},
% long={#4},
% description={#4, \textit{Glossary:} \glslink{#2_gls}{#3}},
% first={#3 (\capitalisewords{#4})\glsadd{#2_gls}},
% #1
% }
}
%% A simple box
\newenvironment{mybox}[0]{%
\tcolorbox[opacityback=0., standard jigsaw,breakable]}%
{\endtcolorbox}
%% Change left and right margins (used in front and back covers)
\newenvironment{changemargin}[2]{%
\begin{list}{}{%
\setlength{\topsep}{0pt}%
\setlength{\leftmargin}{#1}%
\setlength{\rightmargin}{#2}%
\setlength{\listparindent}{\parindent}%
\setlength{\itemindent}{\parindent}%
\setlength{\itemsep}{\parskip}%
\setlength{\parsep}{\parskip}%
}%
\item[]
}{\end{list}}
%% Save deault margin lengths
\newlength{\defaultOddsidemargin}
\setlength{\defaultOddsidemargin}{\oddsidemargin}
\newlength{\defaultEvensidemargin}
\setlength{\defaultEvensidemargin}{\evensidemargin}
% Warning on character count in resume/abstract
\makeatletter
\def\gobblechar{\let\char= }
\newcount\charcount
\def\countunlessnil{%
\ifx\char\nil \let\next=\relax%
\else%
\let\next=\auxcountchar%
\advance\charcount by 1%
\fi\next
}%
\def\auxcountchar{%
\afterassignment\countunlessnil\gobblechar%
}
\def\countchar#1{\edef\xx{#1}\charcount=0 \expandafter\auxcountchar\xx\nil}
\def\shownumchar#1{%
\countchar{#1}%
There are \the\charcount\ characters in [#1].%
}
\newcommand{\PhDThesis@checkResume}{%
\countchar{\@resume}%
\ifnum\charcount>\PhDThesis@Abstractmaxchars
\PhDThesis@warningAbstract{resume}{\PhDThesis@Abstractmaxchars}%
\fi
}
\newcommand{\PhDThesis@checkAbstract}{%
\countchar{\@abstract}%
\ifnum\charcount>\PhDThesis@Abstractmaxchars
\PhDThesis@warningAbstract{abstract}{\PhDThesis@Abstractmaxchars}%
\fi
}
\newcommand{\PhDThesis@warningAbstract}[2]{%
\@latex@warning@no@line{your #1 is longer than #2 characters}%
}

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@@ -0,0 +1,15 @@
\chapter*{Abstract}
\chaptermark{Abstract}
\markboth{ABSTRACT}{ABSTRACT}
\addcontentsline{toc}{chapter}{Abstract}
\stoptoc
\renewcommand\thesection{\arabic{section}}
\setcounter{section}{0}
\renewcommand*{\theHsection}{Abs.\the\value{section}}
...
\renewcommand*{\theHsection}{\theHchapter.\the\value{section}}
\renewcommand\thesection{\thechapter.\arabic{section}}
\resumetoc

View File

@@ -0,0 +1,4 @@
% Glossary
%Syntax: \newdualentry[acronym options]{label}{abbrv}{long}{description}
\newdualentry[longplural="galaxies"]{GAL}{GAL}{galaxy}{I don't know just an entry to test}

View File

@@ -1,17 +1,18 @@
\chapter*{List of Publications}
\chaptermark{List of Publications}
\markboth{LIST OF PUBLICATIONS}{LIST OF PUBLICATIONS}
\addcontentsline{toc}{chapter}{List of Publications}
%%% Add all relevant publications to ./papers.bib
%%% Define \firstauth{Name} and \addboldnames{{Name, I.},{Name, First-Name}} in PhDThesisED182.cls
%%% Will go through all references, add categories based on First Author, Second Author or Contributor
%%% Can also add conference talks and posters as non-articles
\chapter*{List of Publications}
\chaptermark{Publications}
\markboth{PUBLICATIONS}{PUBLICATIONS}
\addcontentsline{toc}{chapter}{List of Publications}
\begin{refsection}
\nocite{*}%
\newrefcontext[sorting=ynt]
\printbibliography[keyword={first},check=JoPR,type=article,heading=subbibliography,title={First Author}]%
\printbibliography[keyword={main},check=JoPR,type=article,heading=subbibliography,title={Main contribution}]%
\printbibliography[keyword={collab},check=JoPR,type=article,heading=subbibliography,title={Collaborator}]%
\printbibliography[nottype=article,heading=subbibliography,title={Conferences}]%
\printbibliography[keyword={collab},check=JoPR,type=article,heading=subbibliography,title={Analysis team}]%
\printbibliography[keyword={self},nottype=article,heading=subbibliography,title={Conferences}]%
\end{refsection}
\resetboldnames

View File

@@ -0,0 +1,15 @@
\chapter*{R\'esum\'e}
\chaptermark{R\'esum\'e}
\markboth{R\'ESUM\'E}{R\'ESUM\'E}
\addcontentsline{toc}{chapter}{R\'esum\'e}
\stoptoc
\renewcommand\thesection{\arabic{section}}
\setcounter{section}{0}
\renewcommand*{\theHsection}{Res.\the\value{section}}
...
\renewcommand*{\theHsection}{\theHchapter.\the\value{section}}
\renewcommand\thesection{\thechapter.\arabic{section}}
\resumetoc

8
Thesis/latexmkrc Normal file
View File

@@ -0,0 +1,8 @@
add_cus_dep('glo', 'gls', 0, 'makeglo2gls');
sub makeglo2gls {
system("makeindex -s '$_[0]'.ist -t '$_[0]'.glg -o '$_[0]'.gls '$_[0]'.glo");
}
add_cus_dep('acn', 'acr', 0, 'makeacn2acr');
sub makeacn2acr {
system("makeindex -s '$_[0]'.ist -t '$_[0]'.alg -o '$_[0]'.acr '$_[0]'.acn");
}

View File

@@ -1,9 +1,15 @@
\ProvidesPackage{macros}
%----------------------------------------------------------------------------------------
% DEFINE BIBLIOGRAPHY STYLE
%----------------------------------------------------------------------------------------
\usepackage{csquotes}
\usepackage[backend=biber,natbib=true,style=authoryear,uniquename=init,giveninits=true,isbn=false,url=false,doi=false,maxcitenames=3,minbibnames=6,maxbibnames=50,sorting=ynt]{biblatex}
\usepackage{microtype}
\usepackage[backend=biber,natbib=true,style=authoryear,uniquelist=false,uniquename=false,giveninits=true,isbn=false,url=false,doi=false,mincitenames=1,maxcitenames=2,minbibnames=6,maxbibnames=150,sorting=nyvt]{biblatex}
\addbibresource[glob]{papers.bib}
\addbibresource[glob]{biblio.bib}
\BiblatexSplitbibDefernumbersWarningOff
\emergencystretch=1em
\makeatletter
\def\nhblx@bibfile@name{papers-sort.bib}
\newwrite\nhblx@bibfile
@@ -52,17 +58,22 @@
\map{
\perdatasource{papers.bib}
\step[fieldsource=author, match=\regexp{^{#1}}, final]
\step[fieldset=keywords, fieldvalue={, first},append]
\step[fieldset=keywords, fieldvalue={,first},append]
}
\map{
\perdatasource{papers.bib}
\step[fieldsource=author, match=\regexp{^(?>\{[^\}]+\}\,\s[\w\-\.]+\sand\s){1}\{#1\}}, final]
\step[fieldset=keywords, fieldvalue={, main},append]
\step[fieldset=keywords, fieldvalue={,main},append]
}
\map{
\perdatasource{papers.bib}
\step[fieldsource=author, match=\regexp{^(?:.+?\sand\s){2}.*?\{#1\}}, final]
\step[fieldset=keywords, fieldvalue={, collab},append]
\step[fieldset=keywords, fieldvalue={,collab},append]
}
\map{
\perdatasource{papers.bib}
\step[fieldsource=author, match=\regexp{{#1}}, final]
\step[fieldset=keywords, fieldvalue={,self},append]
}
}
}

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