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Table 1

Final cluster candidate sample with positions and derived parameters.

VVV αδ (J2000) Radius E(BV) (mM)0 Distance D Z R GC Age
CC deg arcmin (pc) mag mag kpc kpc kpc log(t/1 yr)

168 18:00:50.2 42:11:31 0.4 (1.3) 1.0 ± 0.5 15.2 ± 0.5 11.0 1.8 3.8 9.0 ± 0.5
169 18:01:06.2 42:04:15 0.25 (0.8) 0.7 ± 0.5 15.3 ± 0.5 11.5 1.9 4.3 9.5 ± 0.5
170 18:01:03.0 42:03:09 0.25 (0.6) 1.0 ± 0.5 14.5 ± 0.5 7.9 1.3 1.9 9.0 ± 0.5
171 18:03:55.6 42:20:07 0.25 (0.9) 1.0 ± 0.5 15.5 ± 0.3 12.6 2.2 5.4 9.0 ± 0.5
172 18:06:06.6 42:09:46 0.3 (0.6) 0.5 ± 0.5 14.2 ± 0.5 6.9 1.2 2.0 9.5 ± 1.0
173 18:04:29.0 41:41:33 0.3 (1.6) 0.6 ± 0.5 13.5 ± 0.5 5.0 0.8 3.3 9.0 ± 1.0
174 18:02:34.6 41:31:08 0.4 (0.4) 0.9 ± 0.5 15.7 ± 1.0 13.8 2.2 6.4 9.0 ± 1.0
175 18:05:38.2 41:43:58 0.3 (0.8) 0.4 ± 0.5 14.7 ± 0.5 8.7 1.5 2.1 9.5 ± 0.5
176 18:05:00.8 41:22:49 0.2 (0.7) 0.9 ± 0.3 15.5 ± 0.5 12.6 2.1 5.3 9.0 ± 0.5

Notes. Columns are: Angular and linear radii, color excess E(BV), distance modulus (mM)0, heliocentric distance D, distance below the Galactic plane plane Z, galactocentric distance RGC, and age. See Sect. 3 for details. The cluster IDs continue the nomenclature last used in Lima et al. (2014).

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