Amend sigmaM cosmologies 1-3
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Comoving radial distance, $\chi$ & (\ref{eq:comrdist}) & CCL1-5,7-11 & $0.01 \leq z\leq 1000$ & $5\times 10^{-7}$ & Fig. \ref{fig:distancegrow}\\
Growth factor, $D$ & (\ref{eq:growth}) & CCL1-5 & $0.01 \leq z\leq 1000 $ & $6\times 10^{-6}$ & Fig. \ref{fig:distancegrow}\\
- $\sigma(M)$ (BBKS) & (\ref{eq:sigR}) & CCL1 & $10^{10}\leq M/{\rm M}_\odot\leq 10^{16}$ & $3\times 10^{-5}$ & Fig. \ref{fig:hmf}\\
+ $\sigma(M)$ (BBKS) & (\ref{eq:sigR}) & CCL1-3 & $10^{10}\leq M/{\rm M}_\odot\leq 10^{16}$ & $3\times 10^{-5}$ & Fig. \ref{fig:hmf}\\
$\log[\sigma^{-1}(M)]$ (BBKS) & (\ref{eq:tildesig}) & CCL1 & $10^{10}\leq M/{\rm M}_\odot\leq 10^{16}$ & $10^{-3}$ & Fig. \ref{fig:hmf}\\
$\mathcal H \equiv \log[(M^2/\bar{\rho}_m)dn/dM]$ & (\ref{eq:newhmf}), \citet{Tinker2010} & CCL1 & $10^{10}\leq M/{\rm M}_\odot\leq 10^{16}$ \& $z=0$ & $5\times 10^{-5}$ & Fig. \ref{fig:hmf}\\
$P(k)$ (BBKS) & (\ref{eq:bbks}) & CCL1-3 & $10^{-3}\leq k/(h/{\rm Mpc})\leq 10$ \& $0\leq z\leq 5$ & $10^{-5}$ & -\\
