Accurate photometry with adaptive optics in the presence of anisoplanatic effects with a sparsely sampled PSF - The Galactic center as an example of a challenging target for accurate AO photometry

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Table 1:

Details of the imaging observations used in this work.
Date	$\lambda_{\rm central}$	$\Delta\lambda$	N^a	NDIT^b	DIT^c
	[ $\mu$ m]	[ $\mu$ m]			[s]
29 April 2006	1.66	0.33	32	28	2

^a Number of (dithered) exposures ^b Number of integrations that were averaged on-line by the read-out electronics ^c Detector integration time. The total integration time of each observation amounts to $N\times {\rm NDIT} \times \rm DIT$ .

Source LaTeX | All tables | In the text

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