minor caption updates
@@ -1013,7 +1013,7 @@ Notice that RSD and magnification predictions are not currently validated. We do
\includegraphics[width=0.49\textwidth]{Cl_dd}
\includegraphics[width=0.49\textwidth]{Cl_dl}
\includegraphics[width=0.49\textwidth]{Cl_ll}
-\caption{Tests of the angular power spectra accuracy. The black dot-dashed line indicates the target numerical accuracy of $0.1\sigma_\ell$. {\sl Top:} benchmark comparisons for power spectra between number counts in pairs of redshift bins. Results are shown for analytic (solid) and binned (dashed) redshift distributions, for the bin pairs 1-1 (blue), 1-2 (orange), 2-2 (green). {\sl Middle:} same as the top panel for cross-correlations between number counts and weak lensing, this time including the tomographic bin combination 2-1 (red). {\sl Bottom:} same as the top panel, but for the weak lensing power spectra.}
+\caption{Tests of the angular power spectrum accuracy. The black dot-dashed line indicates the target numerical accuracy of $0.1\sigma_\ell$. {\sl Top:} benchmark comparisons for power spectra between number counts in pairs of redshift bins. Results are shown for analytic (solid) and binned (dashed) redshift distributions, for the bin pairs 1-1 (blue), 1-2 (orange), 2-2 (green). {\sl Middle:} same as the top panel for cross-correlations between number counts and weak lensing, this time including the tomographic bin combination 2-1 (red). {\sl Bottom:} same as the top panel, but for the weak lensing power spectra.}
\label{fig:cls_limber}
\end{figure}
\begin{figure}
@@ -1060,7 +1060,7 @@ We compared the difference between \ccl and the benchmarks for the cosmic shear,
\begin{figure}
\centering
\includegraphics[width=0.49\textwidth]{projected_xiggl_error_comparison_bothnz_p5sigma}
-\caption{Comparison between the predicted galaxy-galaxy lensing projected correlation function and the expected uncertainty for LSST for both redshift distributions.}
+\caption{Comparison between the predicted galaxy-galaxy lensing projected correlation function and the expected uncertainty for LSST for both analytic and histogram redshift distributions.}
\label{fig:corrval2}
\end{figure}
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