\begin{table}%t1
\caption{The integrated properties of our sample of 9~blue LSBGs. The morphological types have been determined by R\"onnback \& Bergvall (\cite{ronnback1}). Absolute magnitudes are based on distances derived from the model by Schechter (\cite{Schechter}), assuming a distance to the Virgo~cluster of 17~Mpc and a Hubble constant of $H_0=75$~km~s$^{-1}$~Mpc$^{-1}$. Unless stated otherwise, $m_B$ represents the integrated $B$-band magnitude inside the $\mu_{B,0}$~= 26.5~mag~arcsec$^{-2}$ isophote. Here, $\mu_0$ represents the "true'' central surface brightness and~$\mu^D_0$ the central surface brightness of the disk extrapolated to the centre. Both have been corrected for inclination assuming an infinitely thin disk. $\it BVR$ are in the Cousins system and $\it JHK'$ in the Johnson system, while $i$ is in the Thuan-Gunn system. All magnitudes have been corrected for galactic extinction (Burstein \& Heiles \cite{Burstein & Heiles}). {\it EW} represents the equivalent width of the H$\alpha$~emission line. All photometric data come from R\"onnback \& Bergvall (\cite{ronnback1}) and Bergvall et~al. (\cite{bergvall2}), except the $\langle$$B-R$$\rangle$ entries, which come from the ESO/Uppsala~survey (Lauberts \& Valentijn \cite{lauberts}).}\label{observations}
%\centerline
{
\begin{tabular}{lllllllllllllll}
\hline
\hline
ESO id.  & Type &$m_{B}$  &$M_{B}$  & $\mu_{B,0}$ & $\mu^D_{B,0}$ & $B-V$ & $\langle$$B-R$$
\rangle$ & $V-i$ & $B-J$  & $J-H$  & $J-K'$  & O/H & {\it EW} & $\log$ \\
& &  &  & (mag & (mag &  &  & & & & & & (\AA ) & $M({\rm HI})$\\
&  &  & & arcsec$^{-2}$) & arcsec$^{-2}$)  &  &  &  &  &  &  &  &  & ($M_\odot$) \\
\hline
074-16  & SBcd & 16.0     & $-17.3$    & 23.9  & 23.6 & 0.44 & 0.42 &  0.08 & 1.76  &  0.5 &      &      &    & 9.69\\ 
084-41  & Sd   & 17.2     &            & 25.2  & 24.7 & 0.44 & 0.47 &  0.08 & 1.71  &      &      &      &    &\\
146-14  & Sdm  & 15.4$^{a}$ & $-16.9$    & 23.6  & 23.8 & 0.36 & 0.30 &  0.02 & 1.72  &  0.7 & 0.7  & 7.61 & 37 & 9.57\\
288-48  & Pec. & 16.8     & $-14.4$    & 22.0  & 23.3 & 0.43 & 0.41 &  0.02 & 1.70  &      &      &      &    &\\
462-36  & SBd  & 16.4     &            & 22.8  & 23.1 & 0.46 & 0.42 &  0.10 & 1.94  &      & 0.7  &      &    &\\
505-04  & Sm   & 15.3     & $-16.9$    & 22.7  & 21.3 & 0.49 & 0.42 & $-0.01$ &       &      &      & 7.68 & 15 & 8.67\\
546-09  & Sm   & 15.2     & $-18.0$    & 21.9  & 22.7 & 0.43 & 0.43 &  0.24 & 1.80  &      &      & 7.95 &    & 9.27\\
546-34  & Sm   & 15.7     & $-15.8$    & 24.5  & 22.8 & 0.38 & 0.43 &  0.01 & 1.40  &      &      & 7.64 & 37 & 8.81\\
602-26  & Pec. & 17.1     &            & 24.7  & 23.6 & 0.31 & 0.39 &  0.05 & 1.40  & 0.7  &      &      &    &\\
\hline
\end{tabular}}
\medskip
$^a$ Magnitude based on the $\mu_B$ = 25 mag arcsec$^{-2}$ isophote.
\end{table}