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Table C.1.

Detected point sources in the NACO Ks and H-band large field mosaics.

RA (a) Dec (b) x y Ks (c) ΔKs (d) H(e) ΔH(f) Young (g)
[pixel] [pixel] mag
17:45:40.0422 −29:00:22.5957 1855.890 1939.880 7.775 0.027 9.722 0.029 0
17:45:41.1800 −29:00:46.8150 735.726 167.445 8.958 0.027 10.885 0.029 0
17:45:40.2610 −29:00:27.1686 1640.090 1605.210 9.187 0.027 11.078 0.029 1
17:45:41.0410 −29:00:22.5504 888.853 1956.410 9.196 0.027 11.220 0.029 0
17:45:39.3937 −29:00:14.5744 2491.110 2522.010 9.253 0.027 11.256 0.029 0
17:45:40.4742 −29:00:34.4292 1427.760 1072.310 9.259 0.027 11.266 0.029 0
17:45:39.7906 −29:00:35.0284 2088.830 1019.040 9.397 0.027 12.748 0.029 0
17:45:40.1109 −29:00:36.2632 1777.920 932.658 9.699 0.027 11.949 0.029 0
17:45:41.2051 −29:00:38.8751 716.755 751.979 9.712 0.027 11.900 0.029 0
17:45:40.8397 −29:00:33.9616 1074.340 1110.860 9.825 0.027 12.586 0.029 0

Notes. We only include the first ten lines of the table in the printed edition of this work. A value > 99 in the table indicates that the corresponding measurement is not available.

(a)

Right ascension.

(b)

Declination.

(c)

Magnitude in the NACO Ks band filter.

(d)

Uncertainty in Ks. The 1σ uncertainty of the zero point, is ΔZPKs = 0.06.

(e)

Magnitude in the NACO H band filter.

(f)

Uncertainty in H. For more information see also footnotee. The 1σ uncertainty of the zero point is ΔZPH = 0.06.

(g)

Spectroscopically identified early type star, according to Do et al. (2009) and Bartko et al. (2009).

The full table is available at the CDS.

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