1 files changed, 9 insertions, 7 deletions
diff --git a/Master/texmf-dist/doc/latex/exam-n/sample/cosmo1.tex b/Master/texmf-dist/doc/latex/exam-n/sample/cosmo1.tex
index cd9ae51974f..27045d026a6 100644
--- a/Master/texmf-dist/doc/latex/exam-n/sample/cosmo1.tex
+++ b/Master/texmf-dist/doc/latex/exam-n/sample/cosmo1.tex
@@ -1,10 +1,11 @@
 \documentclass[compose]{exam-n}
 
 \usepackage{graphics}
+\graphicspath{{fig/}}
 
 \begin{document}
 
-\begin{question}{20}  \author{Andrew Davies}
+\begin{question}{20}  \author{Reginald Q Whimsy}
 % Have a blank line here, to check that the question number remains
 % nicely lined up, even if there are lines between the environment
 % opening and the text.
@@ -22,15 +23,15 @@ included as a graphic.  Fully zenned up?  Then let us begin\dots.
 
 \part Show that, under the action of gravity alone, the scale size
 of the Universe varies according to
-\begin{equation*}
+\begin{equation}
 \ddot{R}=-\frac{4\pi G \rho_0}{3R^2}
-\end{equation*}
+\end{equation}
 \partmarks*{4}
 and that, consequently,
 \begin{equation*}
 \dot{R}^2=-\frac{8\pi G \rho_0}{3R}=-K.
-\end{equation*}
 \partmarks*{3}
+\end{equation*}
 
 Express $K$ in terms of the present values of the Hubble constant
 $H_0$ and of the density parameter $\Omega_0$.
@@ -68,6 +69,10 @@ More content&in row 2
 \end{tabular}
 \caption{\label{t:dullness}A remarkably dull table}
 \end{table}
+Finis.
+\begin{questiondata}
+Hubble's law: $v=H_0 D$
+\end{questiondata}
 \partmarks{4}
 \begin{solution}
 Explanations are superfluous; all that is, is.
@@ -84,8 +89,5 @@ adds nothing to our understanding of our place in the cosmos, but it
 you work out how many deuterium nuclei decayed during the typing of
 this table?).
 \end{solution}
-\begin{questiondata}
-Hubble's law: $v=H_0 D$
-\end{questiondata}
 \end{question}
 \end{document}