Final figure size adjustment

open-gamma-ray-astro · Oct 4, 2016 · 758f309 · 758f309
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diff --git a/proceeding/open-gamma-ray-astro-gamma2016.pdf b/proceeding/open-gamma-ray-astro-gamma2016.pdf
diff --git a/proceeding/text/content.tex b/proceeding/text/content.tex
@@ -8,7 +8,7 @@ \section{Data models and formats}
 \subsection{Data level 3 specifications}
 
 \begin{figure}[tb]
-\centerline{\includegraphics[width=0.7\textwidth]{figures/iact-dl3}}
+\centerline{\includegraphics[width=0.75\textwidth]{figures/iact-dl3}}
 \caption{
 Illustration of major components of IACT DL3 data (using a H.E.S.S. 1 Crab nebula observation). The \texttt{EVENTS} are stored as a table with the most relevant parameters shown. To derive spectra and morphology measurements of astrophysical sources, instrument response functions (IRFs) are used: effective area (\texttt{AEFF}), energy dispersion (\texttt{EDISP}), and point spread function (\texttt{PSF}). Sometimes background (\texttt{BKG}) models are also created and released as part of DL3 data (as an additional IRF component), and other times they are derived at the science tools level. Note that this picture is not complete, see the ``IACT DL3'' section.
 }