All Tables

Table 1: Summary of the VLT adaptive optics observations of PKS 1830-211. The length of the individual exposures is DIT seconds. NDIT exposures are averaged for each of the NDITHER telescope positions. The value of the AO-corrected resolution is the FWHM of the core of the adaptive optics PSF.
Table 2: Astrometry of PKS 1830-211. All positions are given relative to the quasar Image A along with their 1- $\sigma$ error bars. The measurements have been transformed to match the coordinate system of NICMOS (Lehár et al. 2000), by using 8 stars common to the AO and NICMOS fields of view.
Table 3: Photometry of the objects in the vicinity of PKS 1830-211, along with their 1- $\sigma$ error bars. An additional error bar of 0.05 mag on the photometric zero point is not included here.