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\begin{table}
\centering
\footnotesize
\begin{tabular}{lllccccc}
\hline
Object\footnote{SDSS name} & $M_{BH}$\footnote{Central BH mass} & z\footnote{Redshift} & $\sigma_{BLR}$ \footnote{Sigma of gaussian fit to the broad component of Hα emission line}&$L_{BLR} $ H$\alpha$ \footnote{Luminosity of the broad component of Hα emission line}& $m_{abs}^{sph}$\footnote{Absolute magnitude of spheroidal component (bulge) of IMBH host galaxy in the respective photometric band}& $M_{sph}^{ * }$\footnote{Mass of spheroidal component (bulge) of IMBH host galaxy}& $L_{X}$\footnote{X-ray luminosity of IMBH. It is computed from the flux in a respective X-ray catalog unless a reference or a star symbol (this work) is indicated}\\
\hline
 & ($10^3 M_{\odot}$) & &(km s$^{-1}$)  & ($10^{39}$ erg s$^{-1}$)&  & ($ 10^9 M_{\odot}$)& ($10^{40}$ erg s$^{-1}$) \\
\hline
\hline
J122732.18+075747.7 & 69$\pm$20  & 0.033 & 216$\pm$20 & 1.34 $\pm$0.35& -17.8 (r) & 0.9 & 0.55 ({\it XMM})\\
J171409.04+584906.2  & 115$\pm$23 & 0.029 & 373$\pm$31 &0.94$\pm$0.24 &-17.4 (r) & 0.7 & 2.5 ({\it XMM}) \\
J111552.01-000436.1 & 115$\pm$36 & 0.031 & 315$\pm$41 & 1.97$\pm$0.80 &-16.8 (r) & 0.4 & 4.9 ({\it XMM})\\
J110731.23+134712.8 & 120$\pm$24 & 0.045 & 232$\pm$32 & 4.45$\pm$0.68 & -18.0 (K) & 0.3 & 190 ({\it Chandra})$^\star$ \\
J134244.41+053056.1 & 153$\pm$7 & 0.037 & 216$\pm$10 & 3.07$\pm$0.35 & -20.7 (K) & 3.5 & 13.5 ({\it Swift})\\
\hline
J152304.97+114553.6 &  70$\pm$19 & 0.036 & 350$\pm$30 & 0.44$\pm$0.21& & 0.7 &  0.4 ({\it Chandra})\footnote{Baldassare, V. F., Reines, A. E., Gallo, E. & Greene, J. E. A ∼50,000 M Solar Mass Black Hole in the Nucleus of RGG 118. ApJ 809, L14 (2015).}\\
J153425.58+040806.7 & 112$\pm$6 & 0.140 & 249$\pm$6 & 5.26$\pm$0.29&  & 1.3 & 85 ({\it Chandra})\footnote{\label{dong12} {Dong, R., Greene, J. E. & Ho, L. C. X-Ray Properties of Intermediate-mass Black Holes in Active Galaxies. III. Spectral Energy Distribution and Possible Evidence for Intrinsically X-Ray-weak Active Galactic Nuclei. ApJ 761, 73 (2012). } } \\
J160531.84+174826.1 & 116$\pm$10 & 0.031 & 315$\pm$12 & 1.96$\pm$0.21 & & 1.7 &  12.7 ({\it XMM})\\
J112333.56+671109.9 & 157$\pm$34 & 0.055 & 341$\pm$34 & 2.73$\pm$0.54& & 2.4 & 53.5 ({\it XMM})\\
J022849.51-090153.8 & 202$\pm$12 & 0.072 & 250$\pm$7 & 18.1$\pm$0.92 & & 0.7 & 275 ({\it Chandra})\footnotemark[\ref{dong12}] \\
\hline
\end{tabular}
\caption{IMBHs and some of their properties. 
Upper part of the table are objects found in this work; 5 objects in the bottom part were known previously but we give their characteristics measured with our uniform method. }
\label{}
\end{table}
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