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Table 3

Position, photometry, and spectral parameters of the spectroscopic targets.

ID RA Dec J H K s Sp. Typ. E(J − Ks) E(H − Ks) A K s d Member
(J2000) (J2000) (mag) (mag) (mag) (kpc)

VVV CL009:
1 11:56:00.21 –63:19:01.05 12.21 12.12 12.07 B7–8V 0.18 0.05 0.12 2.70 yes
2 11:56:02.37 –63:19:05.98 11.89 11.37 11.11 O8–9V 0.96 0.32 0.63 5.52 yes
3 11:56:02.55 –63:19:05.19 12.25 11.70 11.47 B1–2V 0.91 0.26 0.59 4.22 yes
4 11:56:03.03 –63:19:00.72 13.33 12.68 12.25 B0–1Ve 1.21 0.47 0.79 5.53 ?
5 11:56:03.07 –63:18:54.63 11.87 11.31 11.04 O8–9V 1.02 0.34 0.66 5.25 yes
6 11:56:03.78 –63:18:54.44 10.55 9.93 9.65 WN7/Of yes
7 11:56:03.90 –63:18:59.49 11.73 11.12 10.83 O9–B0V 1.09 0.36 0.71 4.67 yes
8 11:56:04.38 –63:18:54.44 12.14 11.59 11.34 O9–B0V 0.95 0.29 0.62 5.39 yes
9 11:56:06.05 –63:18:59.26 12.70 11.89 11.65 K1–2V 0.39 0.13 0.25 0.26 no
VVV CL011:
1 12:12:40.61 –62:42:31.30 13.44 13.00 12.79 B3/5V 0.74 0.23 0.48 4.65 yes
2 12:12:41.13 –62:42:30.71 11.72 10.60 10.05 WN9 / OIf+ 1.60 0.45 1.04 10.29 yes
3 12:12:41.36 –62:42:32.18 13.39 12.49 12.20 B0–1V 1.33 0.32 0.87 5.20 ?
4 12:12:41.40 –62:42:29.86 13.81 12.77 12.24 B1–2V 1.71 0.56 1.11 4.73 yes
VVV CL036:
1 14:09:00.49 –61:15:54.01 15.28 12.45 11.06 B0–1V 4.41 1.46 2.87 1.92 yes
2 14:09:01.97 –61:16:02.80 13.50 9.25 6.99 M6–7I 5.56 2.04 3.62 yes
3 14:09:02.37 –61:16:02.90 16.78 13.69 11.88 B0–1 5.05 1.85 3.29 2.02 no
4 14:09:02.75 –61:15:58.94 14.25 10.95 9.32 B2–3I 5.00 1.66 3.25 2.60 yes
5 14:09:02.83 –61:15:33.48 15.53 12.65 11.24 B0–1V 4.45 1.45 2.90 1.80 yes
6 14:09:03.28 –61:16:05.87 15.33 12.65 11.33 ?
7 14:09:03.37 –61:15:44.62 15.79 12.44 10.79 O8–9V 5.21 1.75 3.39 1.46 yes
8 14:09:04.23 –61:16:06.59 12.17 11.13 10.56 O9–B0V 1.76 0.61 1.15 2.96 ?
9 14:09:04.30 –61:15:53.78 13.37 10.66 9.16 WN6 4.04 1.35 2.63 2.18 yes
10 14:09:04.67 –61:16:13.99 14.65 12.15 10.93 B0–1V 3.93 1.32 2.56 2.29 yes
VVV CL073:
1 16:30:21.57 –48:12:55.84 13.05 11.76 11.27 M7–8III no
2 16:30:23.73 –48:13:04.90 15.40 12.51 11.08 WN9 / O4–6If+ 4.25 1.33 2.76 7.47 yes
3 16:30:23.92 –48:13:24.68 12.51 11.41 10.96 B0–1 1.71 0.49 1.11 3.60 ?
4 16:30:23.98 –48:13:05.48 14.71 11.53 9.92 WN7 4.70 1.53 3.06 5.46 yes
5 16:30:24.43 –48:13:29.53 12.98 10.54 9.50 K1–2III no
VVV CL074:
1 16:32:05.24 –47:49:29.13 16.40 13.53 12.09 O8–9III 4.52 1.54 2.94 5.86 yes
2 16:32:05.27 –47:49:14.25 16.92 13.23 10.31 WC8 6.18 2.53 4.02 1.54 yes
3 16:32:05.46 –47:49:28.10 14.72 11.82 10.17 WN8 4.48 1.58 2.92 2.68 yes
4 16:32:05.47 –47:49:33.99 16.02 13.30 11.93 B0–1 4.30 1.47 2.80 5.45 yes
5 16:32:05.49 –47:49:29.80 15.64 12.90 11.54 O7–8III 4.31 1.46 2.81 4.84 yes
6 16:32:05.55 –47:49:33.19 16.00 13.24 11.89 O8–O9III 4.23 141 2.75 5.07 yes
7 16:32:05.67 –47:49:30.00 15.98 13.46 12.19 O7–8III 4.00 1.37 2.60 7.16 yes
8 16:32:05.86 –47:49:30.48 16.65 13.35 11.73 M2–3III no
9 16:32:05.93 –47:49:30.92 15.22 12.53 11.31 WN7 / O4–6If+ 3.81 1.13 2.48 13.57 yes
10 16:32:06.43 –47:49:26.46 16.33 12.74 11.11 ?
11 16:32:06.99 –47:49:21.05 16.30 13.05 11.58 M1–2I yes
VVV CL099:
1 17:14:24.26 –38:09:48.61 13.60 11.87 11.00 O9V 2.78 0.94 1.81 3.13 yes
2 17:14:24.41 –38:09:50.76 14.72 13.11 12.31 O9–B0V 2.56 0.83 1.66 5.80 yes
3 17:14:24.50 –38:09:54.59 14.38 12.97 12.38 B1–2V 2.11 0.62 1.37 3.63 no
4 17:14:24.71 –38:09:49.35 12.62 10.93 9.91 WN6+O 2.53 0.86 1.65 4.84 yes
5 17:14:25.42 –38:09:50.40 13.43 11.70 10.64 WN6 2.62 0.91 1.70 6.59 yes
6 17:14:25.58 –38:09:55.97 14.22 12.60 11.79 B0/O9V 2.58 0.85 1.68 4.53 yes
7 17:14:25.66 –38:09:53.72 11.67 10.06 9.26 WC8 1.98 0.42 1.29 3.34 yes
8 17:14:26.10 –38:09:49.58 13.98 12.27 11.10 O9–B0V 3.07 1.24 2.00 2.99 yes
9 17:14:26.34 –38:09:43.81 10.91 9.01 8.26 M4–5V no
10 17:14:26.42 –38:09:49.87 15.21 12.96 12.02 M1–2V no
11 17:14:26.45 –38:09:53.23 15.07 13.03 12.16 M1–2V no
12 17:14:26.68 –38:09:45.05 14.12 12.41 11.51 M4–5V no

Notes. Columns: name of the star, its position (RA and Dec), J, H and Ks photometry (in mag), spectral type, E(J − Ks) and E(H − Ks) colour excesses (in mag), extinction (AKs) and distance (d), respectively. The final column provides our diagnostic with regards to cluster membership (or otherwise).

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