addressed comment on 4.3 text
@@ -901,7 +901,7 @@ Our results are shown in Figure \ref{fig:emuacc}. For cosmologies without neutri
\subsection{Halo bias and halo mass function}
-Independent codes were utilized to test the accuracy of halo mass function predictions. These predictions are computed from power spectra obtained using the BBKS approximation. For the halo mass function, we compare the value of $\sigma$,
+An independent code was utilized to test the accuracy of halo mass function predictions. Our predictions are computed from power spectra obtained using the BBKS approximation. For the halo mass function, we compare the value of $\sigma$,
\begin{equation}
\tilde\sigma\equiv\log[\sigma^{-1}(M)],\label{eq:tildesig}
\end{equation}
