The Milky Way’s nuclear star cluster: Old, metal-rich, and cuspy - Structure and star formation history from deep imaging

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Volume 641 (September 2020)

A&A, 641 (2020) A102

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Table C.2.

Detected point sources in the deep, central NACO Ks holographic image.

RA ^(a)	Dec ^(b)	x	y	K_s ^(c)	ΔK_s ^(d)	Detection frequency ^(e)
		[pixel]	[pixel]	mag
17:45:40.2592	−29:00:27.1576	149.575	428.095	9.152	0.007	1.00
17:45:40.1169	−29:00:27.5128	288.144	399.977	9.835	0.004	1.00
17:45:40.1242	−29:00:29.0311	278.870	288.077	10.000	0.008	1.00
17:45:39.9217	−29:00:26.7214	478.121	455.703	10.039	0.003	1.00
17:45:40.0470	−29:00:26.8603	357.112	447.165	10.183	0.004	1.00
17:45:40.0935	−29:00:31.2332	307.259	125.243	10.196	0.005	1.00
17:45:40.1893	−29:00:27.4726	217.530	403.918	10.561	0.006	1.00
17:45:40.1418	−29:00:29.9707	260.729	219.002	10.656	0.005	1.00
17:45:39.8100	−29:00:29.7463	582.408	231.098	10.713	0.005	1.00
17:45:39.7921	−29:00:29.8077	599.586	226.320	10.713	0.005	0.99

Notes. The last column lists the fraction of bootstrap images, in which any given source was detected. A value > 99 in the table indicates that the corresponding measurement is not available.

^(a)

Right ascension.

^(b)

Declination.

^(c)

Magnitude in the NACO K_s band filter.

^(d)

Uncertainty in K_s. The 1σ uncertainty of the zero point, is ΔZP_{K_s} = 0.06.

^(e)

Fraction of bootstrapped images in which the source was detected.

The full table is available at the CDS.

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