\begin{table}%t2
\par
\caption{\label{tab2}Energy and intensity of the lines detected in the combined RGS spectrum of \object{NGC~1365}.}
%\centerline
{\begin{tabular}{c|c|c|c|c|c} 
\hline \hline
Energy (eV) & Intensity $(I)$ & $I/I$[{\sc o vii}(f)] & $I/I$[{\sc o vii}(f)] & Transition $(E_{{\rm lab}})$$^a$ & Contribution by \\
(eV) & (10$^{-5}$~s$^{-1}$ cm$^{-2}$) & \object{NGC~1365} & \object{NGC~1068} & (eV) & thermal plasma (\%)$^b$ \\ 
\hline
$367.4\pm0.2$ & $1.4\pm^{0.4}_{0.5}$ & $0.60\pm^{0.18}_{0.19}$ & $1.16\pm^{0.05}_{0.19}$ & C{\sc vi} Ly-$\alpha$ (367.56) & $100 \pm 50$ \\
$430.72\pm^{0.02}_{0.09}$ & $0.7\pm0.4$ & $0.30\pm^{0.15}_{0.17}$ & $0.35\pm^{0.02}_{0.17}$ &    N{\sc vi} He-$\alpha$ (r) (430.75)  & $90 \pm 50$ \\
$(r) - 4.4$ & $<$0.6 & $<$0.25 & $0.08 \pm 0.02$ & N{\sc vi} He-$\alpha$ (i) (426.37)  & $\le$100\\
$(r) - 10.8$ & $1.8\pm0.3$ & $0.73\pm^{0.13}_{0.14}$ & $0.89\pm^{0.03}_{0.14}$ & N{\sc vi} He-$\alpha$ (f) (419.86) & $26 \pm 7$ \\
$435.26\pm^{0.16}_{0.30}$ & $0.6\pm^{0.2}_{0.3}$ & $0.27\pm^{0.10}_{0.11}$ & $<$0.06 & C{\sc vi} Ly-$\beta$ (435.91) & $70 \pm 40$ \\
$459.0\pm^{0.5}_{0.3}$ & $0.40\pm^{0.17}_{0.18}$ & $0.16\pm 0.07$ & $0.11\pm^{0.01}_{0.07}$ &     C{\sc vi} Ly-$\gamma$ (459.42) & $90 \pm 50$ \\
$499.96\pm^{0.04}_{0.22}$ & $1.2\pm0.2$ & $0.52\pm^{0.09}_{0.10}$ & $0.41\pm^{0.02}_{0.10}$ &    N{\sc vii} Ly-$\alpha$ (500.31) & $100 \pm 30$  \\
$573.99\pm^{0.05}_{0.05}$ & $1.0 \pm 0.2$ & $0.41\pm^{0.09}_{0.10}$ & $0.38\pm^{0.03}_{0.10}$ &     O{\sc vii} He-$\alpha$ (r) (574.02) & $110 \pm 30$ \\
$(r) - 5.3$ & $0.6\pm0.2$ & $0.23\pm^{0.09}_{0.10}$ & $0.12\pm^{0.02}_{0.10}$ & O{\sc vii} He-$\alpha$ (i) (569.07) & $34 \pm 12$ \\
$(r) - 13.0$ & $2.4\pm0.3$ & $1.00\pm0.13$ & $1.00\pm^{0.04}_{0.13}$ & O{\sc vii} He-$\alpha$ (f) (561.06) & $40 \pm 8$  \\
$653.4\pm0.6$ & $2.5\pm0.2$ & $1.03\pm^{0.08}_{0.09}$ & $0.52\pm^{0.02}_{0.09}$ & O{\sc vii} Ly-$\alpha$ (653.70) & $110 \pm 20$ \\
$726.00\pm^{0.35}_{0.13}$ & $1.89\pm^{0.18}_{0.19}$ & $0.78\pm0.08$ & $0.14\pm^{0.01}_{0.08}$ & Fe{\sc xvii} 3$^s$2$^p$ (726.29)  & $86 \pm 11$ \\
$738.1\pm^{0.3}_{0.9}$ & $0.47 \pm^{0.15}_{0.13}$ & $0.20 \pm 0.06$ & $0.104 \pm 0.014$ & O{\sc vii} RRC$^c$ (739.11) & $60 \pm 20$ \\
& & & &  &  \\
$773.54\pm^{0.02}_{0.34}$ & $0.75\pm^{0.13}_{0.13}$ & $0.31\pm^{0.05}_{0.06}$ & $0.09\pm^{0.01}_{0.06}$ & O{\sc viii} Ly-$\beta$ (774.71)$^d$  & $83 \pm 16$  \\
$824.57\pm0.07$ & $1.49\pm^{0.16}_{0.17}$ & $0.62\pm 0.07$ & $0.12\pm^{0.01}_{0.07}$ & Fe{\sc xviii} 3$^d$2$^p$ (824.72)  & $98 \pm 14$ \\
$872.0\pm0.7$ & $0.42\pm^{0.12}_{0.13}$ & $0.18\pm 0.05$ & $0.06\pm^{0.01}_{0.05}$ & OVIII RRC (871.52)$^e$  & $60 \pm^{70}_{40}$ \\
$921.63\pm^{0.25}_{0.12}$ & $0.42\pm^{0.17}_{0.18}$ & $0.18\pm^{0.07}_{0.08}$ & $0.10\pm^{0.01}_{0.08}$ &   Ne{\sc ix} He-$\alpha$ (r) (922.14)  & $130 \pm 60$\\
$(r) - 7.2$ & $<$0.33 & $<$0.14 & $<$0.05 &  Ne{\sc ix} He-$\alpha$ (i) (915.13) & $<$100 \\
$(r) - 13.0$ & $0.40\pm^{0.11}_{0.12}$ & $0.17\pm 0.05$ & $0.10\pm^{0.01}_{0.05}$ & Ne{\sc ix}He-$\alpha$ (f) (905.11) & $90 \pm 30$ \\
$1021.13\pm^{1.20}_{0.10}$ & $1.0\pm0.2$ & $0.43\pm^{0.09}_{0.10}$ & $0.11\pm^{0.01}_{0.10}$ &     Ne{\sc x} Ly-$\alpha$ (1021.92) & $120 \pm 30$ \\
$1353.2\pm^{2.1}_{1.4}$ & $0.57\pm^{0.15}_{0.16}$ & $0.24\pm^{0.06}_{0.07}$ & $<$0.05 & Mg{\sc xi} He-$\alpha$ (r) (1352.24) & $110 \pm 15$ \\
$(r) - 8.0$ & $<$0.6 & $<$0.25 & $<$0.04 & Mg{\sc xi} He-$\alpha$ (i)  (1343.44) & $\le$100 \\
$(r) - 21.0$ & $0.33\pm^{0.15}_{0.16}$ & $0.14\pm^{0.06}_{0.07}$ & $<$0.04 & Mg{\sc xi} He-$\alpha$ (f)  (1331.90) & $90 \pm 50$ \\
$1473.0\pm^{3.7}_{1.7}$ & $0.50\pm^{0.18}_{0.19}$ & $0.21\pm^{0.07}_{0.08}$ & $<$0.04 & Mg{\sc xii} Ly-$\alpha$ (1472.51) & $90 \pm 30$ \\
$1896.9\pm0.7$ & $<$47 & $<$33 & $<$0.33 & Si{\sc xiii} He-$\alpha$ (r) (1867.47) & $\le$100 \\
$(r) - 13.8$  & $<$2.4 & $<$1.0 & $<$0.05 & Si{\sc xiii} He-$\alpha$ (i) (1853.61) & $\le$100 \\
$(r) - 27.8$  & $1.9\pm^{1.1}_{0.7}$ & $0.8\pm^{0.5}_{0.3}$ & $<$0.04 & Si{\sc xiii} He-$\alpha$ (f) (1839.76) & $90 \pm 30$ \\
$1892.7\pm0.8$$^f$ & $1.1\pm0.4$ & $0.46\pm 0.18$ & $<$0.05 & & ... \\
\hline
\end{tabular}}\medskip
\par
$^a$ Most likely identification. The laboratory energy is shown in brackets.
$^b$ Contribution to the total intensity due to the best-fit model in Table~3. Values higher than 100\% mean that the model over-predicts the data at that energy.
$^c$ Fit with a single Gaussian ($\sigma \le 8$~eV). Possible blending with Fe {\sc xvii} 2$^{\rm s}$2$^{\rm p}$ (738.98~eV): see Sect.~4.1 for the results of a fit with two Gaussians.
$^d$ Possible blending with Fe{\sc xviii} 3$^{\rm s}$2$^{\rm p}$ (773.02~eV).
$^e$ Fit with a single Gaussian ($\sigma \le 3$~eV). Possible blending with Fe{\sc xviii} 2$^{\rm s}$2$^{\rm p}$ (872.75~eV). See Sect.~4.1 for the results of a fir with two Gaussians. $^f$~Unidentified. 
\end{table}