deletions | additions       diff --git a/sky-ratio-table.tex b/sky-ratio-table.tex  index d868528..d4edf0f 100644  --- a/sky-ratio-table.tex  +++ b/sky-ratio-table.tex 
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\begin{table}  \begin{tabular}{cccccccc}  & \begin{tabular}{ccccccc}  \textbf{Log ratio} & & \textbf{Mean} & & & \textbf{Standard deviation} & \\\textbf{Analysis} &  & bayestar & non-spinning & spinning & bayestar & non-spinning & spinning \\&  $\displaystyle \vphantom{\frac{0}{0}} \mathcal{R}^\mathrm{B}_{\mathrm{CR}_{0.5}}$ & $0.095$ & $0.008$ & ? & $0.117$ & $0.041$ & ? \\&  $\displaystyle \vphantom{\frac{0}{0}} \mathcal{R}^\mathrm{B}_{\mathrm{CR}_{0.9}}$ & $0.075$ & $0.005$ & ? & $0.094$ & $0.048$ & ? \\&  $\displaystyle \vphantom{\frac{0}{0}} \mathcal{R}^\mathrm{B}_{A_\ast}$ & $0.106$ & $0.018$ & ? & $0.447$ & $0.313$ & ? \end{tabular}  \caption{\label{tab:sky-ratio} Comparison of sky localization areas produced by the low-latency \textsc{bayestar} (B) analysis, the nonspinning SpinTaylorT4 (ns) analysis and the high-latency fully spinning SpinTaylorT4 (s) analysis to the medium-latency TaylorF2 analysis. The mean and standard deviation of the log ratio for the $50\%$ credible region $\mathrm{CR}_{0.5}$, the $90\%$ credible region $\mathrm{CR}_{0.9}$ and the searched area $A_\ast$ are listed for each analysis.}