\begin{table}%t2 \caption{\label{param}Line parameters of newly detected masers.} %\centerline { \begin{tabular}{l c c c c c c c c c l} \hline \hline %\\ Source &\textit{D}$^{a}$&Epoch&Tel.&$\int S ~\rm{d} \textit{V}^{b}$&$V_{\rm{LSR,opt}}^{b}$ &$\Delta V_{1/2}^{b}$&\textit{V}-range&Channel&rms&$L_{\rm{H_{2}O}}^c$ \\ & & & & & & & & Width & & \\ &(Mpc) & & & (mJy km s$^{-1}$)& (km s$^{-1}$) & (km s$^{-1}$) &(km s$^{-1}$)& (km s$^{-1}$)& (mJy)&(\solum) \\ \hline NGC~3256 & 37.4& Aug. 2007 & Tid &315 & $2827\pm6$ & $63\pm14$ & 2065, 3407& 0.5 & 3 & 10.9\\ & & Apr. 2008 & ATCA&27.0 & $2822.1\pm0.9$ & $7.7\pm2.3$ & 2611, 2878& 3.7 & 4 & 1.0\\ & & & &32.8 & $2840.2\pm2.4$ & $15.6\pm6.3$ & & & 7 & 2.4\\ & & Apr. 2008 & Tid &400 & $2797\pm2$ & $40.0^{d}$ & 2067, 3409& 0.5 & 3 & 12.9\\ & & & & & & & & & & \\ NGC~3620 & 22.4& Feb.--March 2005& Tid &150 & $1823^{d}$& $10.0^{d}$ & 1000, 2346& 0.5 & 7& 4.7$^{e}$ \\ & & & &255.2 & $1833^{d}$& $4.4\pm0.5$ & & & & \\ & & Apr. 2006 &ATCA & 71.3 & $1821.1\pm0.1$ & $2.5\pm0.2$ & 1777, 1854& 0.2 & 3 & 2.1$^{f}$\\ & & & & 12.7 & $1825.1\pm0.1$ & $1.4\pm0.4$ & & & & \\ & & & & 97.2 & $1827.4\pm0.8$ & $12.3\pm1.4$ & & & & \\ & & Aug. 2007 & Tid & 376 & $1826.1\pm0.8$ & $20.0^{d}$ & 952, 2298 & 0.5 & 3 & 4.3\\ & & Mar. 2008 & Tid & 103.7& $1820^{d}$ & $6.1\pm1.7$ & 1385, 2245 & 0.5 & 5 & 3.2$^{e}$ \\ & & & & 124.7& $1828^{d}$ & $4.3\pm0.8$ & & & & \\ & & Apr. 2008 & Tid & 114.4& $1817.5\pm3.4$ & $10.4\pm6.8$ & 994, 2339 & 0.5 & 5 & 2.5$^{e}$\\ & & & & 98.8 & $1824.7\pm0.8$ & $3.8\pm2.6$ & & & & \\ \hline \end{tabular}} \par \medskip $^a$ Distances have been estimated by using velocities taken from the NASA/IPAC Extragalactic Database (NED) and adopting a Hubble constant of $H_{\rm{0}}= \rm{75 ~ km~ s^{-1}~ Mpc^{-1}}$.\\ $^b$ Integrated flux densities, centre velocities, and full width to half maximum ({\it FWHM}) linewidths of the observed features are obtained from Gaussian fits.\\ $^c$ Isotropic luminosities are derived from $L_{\rm{H_{2}O}}/[\solum]=0.023 \times \int S ~ \rm{d}\textit{V}/[\rm{Jy \ km \ s^{-1}}] \times \textit{D}^{2}/[\rm{Mpc^{2}}]$.\\ $^{d}$ Values obtained by forcing the fit.\\ $^e$ The water maser emission consists of two features.\\ $^{f}$ The water maser emission consists of three features. \end{table}