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.
Filter Airmass NDIT $\times$ DIT Resolution Exp. time

(mean) $\times$ NDITHER (FWHM) (total)

J 1.10 $3 \times 40 \times 37$ 0 $.\!\!^{\prime\prime}$ 085 4440 s

H 1.20 $3 \times 20 \times 104$ 0 $.\!\!^{\prime\prime}$ 070 6240 s

Ks 1.03 $2 \times 30 \times 14$ 0 $.\!\!^{\prime\prime}$ 097 840 s

**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.
Filter	Airmass	NDIT $\times$ DIT	Resolution	Exp. time
	(mean)	$\times$ NDITHER	(FWHM)	(total)
J	1.10	$3 \times 40 \times 37$	0 $.\!\!^{\prime\prime}$ 085	4440 s
H	1.20	$3 \times 20 \times 104$	0 $.\!\!^{\prime\prime}$ 070	6240 s
Ks	1.03	$2 \times 30 \times 14$	0 $.\!\!^{\prime\prime}$ 097	840 s

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