From ca3964cfed918b8c0956a68ce4fd4c4393cab760 Mon Sep 17 00:00:00 2001
From: ikelley <ikelley@0a4070d5-58f5-498f-b6c0-2693e757fa0f>
Date: Tue, 4 Jun 2002 12:50:57 +0000
Subject: changing the documentation.tex files to use our cactus style file

git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/IDAxiBrillBH/trunk@50 0a4070d5-58f5-498f-b6c0-2693e757fa0f
---
 doc/documentation.tex | 23 ++++++++++++++++++++---
 1 file changed, 20 insertions(+), 3 deletions(-)

diff --git a/doc/documentation.tex b/doc/documentation.tex
index 8567c19..a7350c5 100644
--- a/doc/documentation.tex
+++ b/doc/documentation.tex
@@ -1,16 +1,29 @@
 \documentclass{article}
+
+% Use the Cactus ThornGuide style file
+% (Automatically used from Cactus distribution, if you have a 
+%  thorn without the Cactus Flesh download this from the Cactus
+%  homepage at www.cactuscode.org)
+\usepackage{../../../../doc/ThornGuide/cactus}
+
 \begin{document}
 
 \title{IDAxiBrillBH}
 \author{Paul Walker, Steve Brandt}
-\date{1 September 1999}
+\date{$ $Date$ $}
+
 \maketitle
 
-\abstract{Thorn IDAxiBrillBH provides analytic initial data for a vacuum
+% Do not delete next line
+% START CACTUS THORNGUIDE
+
+\begin{abstract}
+  Thorn IDAxiBrillBH provides analytic initial data for a vacuum
   black hole spacetime:  a single Schwarzschild black hole in
   isotropic coordinates plus Brill wave.  This initial data is
   provided for the 3-conformal metric, it's spatial derivatives, and
-  extrinsic curvature.}
+  extrinsic curvature.
+\end{abstract}
 
 \section{Purpose}
 
@@ -158,4 +171,8 @@ interpolation.
 \bibitem{Camarda97a}
   K. Camarda, Ph.D thesis University of Illinois Urbana-Champaign, (1998)
 \end{thebibliography}
+
+% Do not delete next line
+% END CACTUS THORNGUIDE
+
 \end{document}
-- 
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