sky-ratio-table.tex

\begin{table}
\begin{tabular}{ccccc}
\textbf{Logarithmic ratio} & \textbf{Mean} & & \textbf{Standard deviation} & \\   
 & \textsc{bayestar} & Spinning & \textsc{bayestar} & Spinning \\
$\displaystyle \vphantom{\frac{0}{0}} \mathcal{R}^X_{\mathrm{CR}_{0.5}}$ & $0.095$ & $0.022$ & $0.117$ & $0.067$ \\
$\displaystyle \vphantom{\frac{0}{0}} \mathcal{R}^X_{\mathrm{CR}_{0.9}}$ & $0.075$ & $0.028$ & $0.094$ & $0.063$ \\
$\displaystyle \vphantom{\frac{0}{0}} \mathcal{R}^X_{A_\ast}$ & $0.106$ & $0.002$ & $0.447$ & $0.397$
\end{tabular}
\label{tab:sky-ratio} \caption{Comparison of sky localization areas produced by the low-latency \textsc{bayestar} analysis and the high-latency fully spinning SpinTaylorT4 analysis with those produced by the medium-latency non-spinning 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}