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Table 4

L-band excess sources in the Quintuplet cluster.

Seq Field dRA dDec J σ J H σ H K s σ Ks L ′ σ L Mem
[asec] [asec] [mag] [mag] [mag] [mag] [mag] [mag] [mag] [mag]
1 1 10.68 –1.74 19.60 0.04 16.66 0.07 14.48 0.00 12.61 0.03 1
2 1 4.72 5.81 20.10 0.04 16.95 0.08 14.88 0.00 12.76 0.05 1
3 1 –18.62 –10.33 20.31 0.09 17.54 0.07 15.64 0.03 13.26 0.02 1
4 1 –18.84 –5.63 20.58 0.07 17.52 0.07 15.43 0.01 13.06 0.10 1
5 1 –5.86 4.61 20.71 0.05 17.33 0.08 15.32 0.01 13.15 0.03 1
6 1 –3.25 –13.71 21.06 0.06 17.88 0.07 15.55 0.02 12.88 0.08 1
7 1 1.73 12.35 21.11 0.06 17.75 0.09 15.42 0.00 13.24 0.03 1
8 1 –1.38 –18.67 21.21 0.05 17.51 0.09 15.27 0.02 12.41 0.02 1
9 1 0.40 4.28 21.17 0.14 18.57 0.09 16.24 0.12 14.46 0.02 1
10 1 18.59 –1.34 21.33 0.05 18.25 0.07 16.02 0.01 13.61 0.12 1
11 1 –13.45 –7.59 21.42 0.06 18.28 0.07 15.98 0.01 13.61 0.03 1
12 1 –12.22 7.91 21.63 0.19 18.60 0.11 16.24 0.02 13.94 0.09 1
13 1 0.62 1.25 21.71 0.23 17.60 0.17 15.32 0.04 12.88 0.01 1
14 1 10.29 –16.15 21.88 0.13 18.58 0.12 16.18 0.02 13.96 0.07 1
15 1 –4.33 6.38 21.91 0.09 18.75 0.13 16.38 0.00 14.46 0.06 1
16 1 –15.24 –0.78 22.12 0.10 18.79 0.12 15.93 0.01 13.22 0.01 1
17 1 –13.66 10.27 22.29 0.09 18.46 0.10 16.05 0.01 13.63 0.01 1
18 1 –8.33 –10.27 22.79 0.05 19.12 0.09 17.06 0.00 14.80 0.29 1
19 1 17.79 –8.60 22.15 0.13 18.65 0.10 16.23 0.04 13.52 0.10 –1
20a 2 –1.38 –18.67 21.21 0.05 17.51 0.09 15.89 0.01 13.13 0.00 1
21 2 –7.02 –26.19 21.21 0.05 17.97 0.10 15.69 0.00 13.28 0.01 1
22 2 –10.77 –29.58 21.97 0.19 18.85 0.14 16.96 0.01 14.74 0.04 1
23 4 28.73 18.35 17.67 0.09 15.22 0.06 13.87 0.00 12.34 0.04 1
24 5 26.71 –0.95 20.97 0.07 18.02 0.09 16.11 0.00 13.90 0.10 1
25 5 29.98 –6.28 21.07 0.05 17.92 0.07 16.15 0.01 13.71 0.01 1
26 5 18.59 –1.33 21.33 0.05 18.25 0.07 16.65 0.01 14.26 0.03 1
27b 5 17.79 –8.60 22.15 0.13 18.65 0.10 17.04 0.00 14.23 0.07 1
28 5 13.65 –9.39 20.67 0.09 17.62 0.11 16.64 0.01 14.39 0.13 –1

Notes. Positional offsets in right ascension and declination are given in arcseconds, relative to the Wolf-Rayet member Q12 in the cluster core, RA 17:46:15.13, Dec −28:49:34.7. Sources identified as proper motion members have a membership index of 1, while sources without reliable membership information are labelled as −1. Non-members are likely field stars and are not shown here.

(a)

Source 20 in Field 2 is identical to source 8 in Field 1.

(b)

Source 27 in Field 5 is identical to source 19 in Field 1.

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