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.
Object X Y

(arcsec) (arcsec)

Quasar A 0.0 0.0

Quasar B $+0.649\pm 0.001$ $-0.724\pm 0.001$

Star P $+0.333\pm 0.002$ $-0.504\pm 0.002$

Lens G $+0.498\pm 0.004$ $-0.456\pm 0.004$

**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.
Object	X	Y
	(arcsec)	(arcsec)
Quasar A	0.0	0.0
Quasar B	$+0.649\pm 0.001$	$-0.724\pm 0.001$
Star P	$+0.333\pm 0.002$	$-0.504\pm 0.002$
Lens G	$+0.498\pm 0.004$	$-0.456\pm 0.004$

Source LaTeX | All tables | In the text

	1 Introduction
	2 VLT adaptive optics observations and reduction
	3 Deconvolution and astrometry
	4 Discussion and conclusions
	References