All Tables

Table 1: Details of the XMM-Newton X-ray observations.
Table 2: $3-\sigma$ Upper limits to the X-ray flux of LBQS 2212-1759 derived from the EPIC-pn observations.
Table 3: Optical and UV fluxes measured though the various OM filters.
Table 4: The flux of LBQS 2212-1759 as a function of wavelength, from the near-IR to the EUV. The values in the optical and UV have been obtained by averaging fluxes from individual OM exposures. All fluxes have been corrected for foreground galactic reddening.
Table 5: Intensities and full width at half maximum ( FWHM) of the main emission lines in the spectrum of LBQS 2212-1759; all intensities are in units of ${\rm 10^{-16}~erg~cm^{-2}~s^{-1}}$ and have been corrected for galactic extinction. Their uncertainties are typically 10%. The FWHM are expressed in ${\rm km~s^{-1}}$ and have an uncertainty of ${\rm \pm50~km~s^{-1}}$ .