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Table 1

Parameters of spectroscopic targets.

ID RA Dec J H K s Sp. Typ. E(JKs) E(HKs) A K s d
(J2000) (J2000) (mag) (mag) (mag) (mag) (mag) (mag) (kpc)

1 14:46:23.78 –59:23:37.89 10.17 9.05 8.77 K3III 0.74 0.27 0.45 0.06
2 14:46:24.94 –59:23:27.27 10.29 9.32 8.95 O7V/III 1.55 0.47 0.93 2.91
3 14:46:25.25 –59:23:12.45 11.40 10.41 9.99 O7V/III 1.62 0.52 0.97 4.61
4 14:46:25.25 –59:23:16.04 11.78 10.80 10.41 B
5 14:46:25.63 –59:23:30.37 11.18 10.20 9.86 O6-7V/III 1.53 0.44 0.92 4.88
6 14:46:25.77 –59:23:35.66 10.62 9.73 9.27 O4-5V/III 1.56 0.56 0.94 4.23
7 14:46:26.01 –59:23:48.28 13.21 12.39 11.96 B
8+ 14:46:26.41 –59:23:28.83 8.41 7.42 6.87 WN8-9h

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

(∗)

Typical error is 0.01 mag.

(†)

Star 1 is likely a foreground star and not a member of the cluster.

(‡)

Magnitudes adopted from 2MASS.

(+)

Also named WR 62-2.

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