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.
Object J H

Quasar A $18.04\pm0.05$ $16.36 \pm 0.05$

Quasar B >23.0 $22.12 \pm 0.10$

Star S1 $17.57 \pm 0.05$ $16.72 \pm 0.05$

Star P $21.76 \pm 0.10$ $20.93 \pm 0.05$

Lens G $22.76 \pm 0.20$ $21.25 \pm 0.10$

**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.
Object	J	H
Quasar A	$18.04\pm0.05$	$16.36 \pm 0.05$
Quasar B	>23.0	$22.12 \pm 0.10$
Star S1	$17.57 \pm 0.05$	$16.72 \pm 0.05$
Star P	$21.76 \pm 0.10$	$20.93 \pm 0.05$
Lens G	$22.76 \pm 0.20$	$21.25 \pm 0.10$

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