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authorallen <allen@5301f0c2-dbc4-4cee-b2f5-8d7afba4d129>2002-09-08 20:27:04 +0000
committerallen <allen@5301f0c2-dbc4-4cee-b2f5-8d7afba4d129>2002-09-08 20:27:04 +0000
commit52b166e4e714d54266251967931a352a461f6734 (patch)
tree5ae1eca29df7dbe2a3a961bf777401102106bf37
parent77cd6917f6eacae5abf7820181083c1253a0e512 (diff)
typo
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/Extract/trunk@65 5301f0c2-dbc4-4cee-b2f5-8d7afba4d129
-rw-r--r--doc/documentation.tex2
1 files changed, 1 insertions, 1 deletions
diff --git a/doc/documentation.tex b/doc/documentation.tex
index aac6987..c6b5738 100644
--- a/doc/documentation.tex
+++ b/doc/documentation.tex
@@ -395,7 +395,7 @@ for extracting close to the event horizon for perturbations of black holes.
\subsection{Calculate $S$ factor and Mass Estimate}
\begin{equation}
-S(\hat{r}) = \left(\frac{\partial\hat{r}}{\partial r}\right)^2 \int g_{tt} \ d\t d\p
+S(\hat{r}) = \left(\frac{\partial\hat{r}}{\partial r}\right)^2 \int \gamma_{rr} \ d\t d\p
\end{equation}
\begin{equation}