Table 2: Details of NIR observations. "Observing ID'' refers to the number of the data set in column one of Table 1. $\lambda$ is the central wavelength of the broad-band filter used. DIT is the detector integration time in seconds. NDIT is the number of exposures of integration time DIT that were averaged on-line by the instrument. Nis the number of images taken. The total integration time amounts to DIT $~\times~$ NDIT $~\times~$ N. Seeing is the value measured by the Differential Image Motion Monitor (DIMM) on Paranal at visible wavelengths. It provides a rough estimate of atmospheric conditions during the observations.
Observing $\lambda$ DIT NDIT N Pixel scale Seeing

ID

1 1.7 $\mu$ m 15 s 2 50 0.013'' $\sim$ 1.1''

2 2.2 $\mu$ m 15 s 2 217 0.027'' $\sim$ 1.0-1.5''

3 3.8 $\mu$ m 0.2 s 150 100 0.027'' $\sim$ 1.3-1.8''

4 2.2 $\mu$ m 30 s 1 330 0.027'' $\sim$ 1.0-1.8''

5 3.8 $\mu$ m 0.2 s 150 60 0.027'' $\sim$ 0.7''

6 2.2 $\mu$ m 30 s 1 391 0.027'' $\sim$ 0.7''

**Table 2:** Details of NIR observations. "Observing ID'' refers to the number of the data set in column one of Table 1. $\lambda$ is the central wavelength of the broad-band filter used. DIT is the detector integration time in seconds. NDIT is the number of exposures of integration time DIT that were averaged on-line by the instrument. Nis the number of images taken. The total integration time amounts to DIT $~\times~$ NDIT $~\times~$ N. Seeing is the value measured by the Differential Image Motion Monitor (DIMM) on Paranal at visible wavelengths. It provides a rough estimate of atmospheric conditions during the observations.
Observing	$\lambda$	DIT	NDIT	N	Pixel scale	Seeing
ID
1	1.7 $\mu$ m	15 s	2	50	0.013''	$\sim$ 1.1''
2	2.2 $\mu$ m	15 s	2	217	0.027''	$\sim$ 1.0-1.5''
3	3.8 $\mu$ m	0.2 s	150	100	0.027''	$\sim$ 1.3-1.8''
4	2.2 $\mu$ m	30 s	1	330	0.027''	$\sim$ 1.0-1.8''
5	3.8 $\mu$ m	0.2 s	150	60	0.027''	$\sim$ 0.7''
6	2.2 $\mu$ m	30 s	1	391	0.027''	$\sim$ 0.7''

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