Table A.2:

List of detected point sources in the NACO H, , and L'-band observations. We only include the first ten lines of the table in the printed edition of this work.

ID	a	RAb	Decc	Hd	e	f	g	L'h	i
	['']	['']	['']
1	0.028	0.009	-0.027	17.50	0.05	15.7	0.04	0.0k	0.0
2	0.107	0.031	-0.102	18.19	0.06	16.39	0.04	0	0
3	0.163	-0.006	0.163	16.00	0.02	14.13	0.01	12.84	0.03
4	0.231	0.189	0.132	16.93	0.03	15	0.01	0	0
5	0.245	-0.231	-0.081	18.69	0.07	16.75	0.05	0	0
6	0.265	0.022	-0.264	16.53	0.03	14.7	0.02	0	0
7	0.321	0.296	0.124	16.47	0.02	14.61	0.01	0	0
8	0.347	-0.274	0.213	17.45	0.03	15.66	0.09	14.35	0.06
9	0.354	-0.053	0.35	17.22	0.03	15.39	0.02	0	0
10	0.363	0.02	-0.363	16.23	0.03	14.12	0.01	12.6	0.03

Notes.  ^(a) Distance from Sgr A* projected on the sky. ^(b) Offset in right ascension from Sgr A*. Uncertainties in the astrometric positions can be as large as 0.1'' because high precision astrometry was not at the focus of this work. The conversion to offsets from Sgr A* was done by assuming a pixel scale of 0.027'' per pixel (ESO NACO manual). The camera rotation angle was assumed 0 deg east of north and no camera distortion solution was applied. ^(c) Offset in declination from Sgr A*. For more information see also footnote^b. ^(d) Magnitude in the NACO H band filter. ^(e) Uncertainty in H, obtained by quadratically combining the formal uncertainty from PSF fitting, based on Gaussian read-out noise and Poisson photon noise, and the uncertainty due to the limited knowledge of the PSF. The 1 uncertainty of the zero point, , is not included in this column and has to be taken into account when considering absolute photometry. ^(f) Magnitude in the NACO band filter. ^(g) Uncertainty in . For more information see also footnote ^e. The 1 uncertainty of the zero point is . ^(h) Magnitude in the NACO L' band filter. ⁽ⁱ⁾ Uncertainty in L'. For more information see also footnote ^e. The 1 uncertainty of the zero point is . ^(j) A value of 0.0 in the table indicates that the corresponding measurement is not available.