deletions | additions       diff --git a/sky-ratio-table.tex b/sky-ratio-table.tex  index 6b385de..6d17b63 100644  --- a/sky-ratio-table.tex  +++ b/sky-ratio-table.tex 
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\begin{table}  \begin{tabular}{ccccccc} \begin{tabular}{ccccc}  \textbf{Log ratio} & & \textbf{Mean} & & & \textbf{Standard deviation} & \\   & \textsc{bayestar} &non-spinning &  spinning & \textsc{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 nonspinning  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.} \end{table}