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Table E.1

JHKs sources and L detections in the Quintuplet cluster.

Seq Field dRA dDec J σ J H σ H Epoch1 Ks1 σ Ks1 Epoch2 Ks2 σ Ks2 Epoch3 Ks3 σ Ks3 L σ L μ αcosδ σ μ αcosδ μ δ σ μ δ Mem Exc p clus
[′′] [′′] [mag] [mag] [mag] [mag] [year] [mag] [mag] [year] [mag] [mag] [year] [mag] [mag] [mag] [mag] [mas/yr] [mas/yr] [mas/yr] [mas/yr]

Field 1

1 1 3.255 –6.710 12.466 0.066 11.698 0.039 2003.556 11.234 0.178 2008.562 11.031 0.004 –99.000 –99.000 –99.000 10.829 0.005 –1.321 0.557 6.373 0.720 0 0 –99.000
2 1 –0.324 5.428 14.187 0.050 11.118 0.067 2003.556 9.385 0.064 2008.562 9.511 0.007 –99.000 –99.000 –99.000 7.830 0.002 –3.090 0.283 –0.645 0.754 0 0 –99.000
...
723 1 0.000 –0.000 14.904 0.067 11.314 0.083 2003.556 9.726 0.016 2008.562 –99.000 –99.000 –99.000 –99.000 –99.000 –99.000 –99.000 –99.000 –99.000 –99.000 –99.000 –1 –99 –99.000
724 1 –4.330 0.523 15.495 0.128 11.182 0.110 2003.556 7.741 0.016 2008.562 –99.000 –99.000 –99.000 –99.000 –99.000 –99.000 –99.000 –99.000 –99.000 –99.000 –99.000 –1 –99 –99.000
...

Field 2

3133 2 6.599 –26.482 16.218 0.069 13.084 0.074 2008.562 11.780 0.001 2011.718 11.873 0.006 2012.452 11.773 0.022 10.521 0.005 0.229 0.359 0.641 0.403 1 0 0.623
3134 2 8.071 –26.940 16.506 0.058 13.580 0.064 2008.562 12.189 0.002 2011.718 12.270 0.003 2012.452 12.167 0.001 10.949 0.004 –0.208 0.363 0.371 0.408 1 0 0.785
...

Field 3

4893 3 37.289 –42.957 15.922 0.075 13.128 0.068 2008.649 11.855 0.018 2009.266 11.946 0.010 2012.452 11.980 0.001 10.777 0.000 –0.580 0.293 1.253 0.292 1 0 0.522
4894 3 22.644 –33.950 15.825 0.071 15.129 0.046 2008.649 14.930 0.033 2009.266 14.835 0.007 2012.452 14.911 0.003 14.580 0.079 2.066 0.298 –3.504 0.273 0 0 0.000
...

Field 4

6566 4 22.048 10.509 15.729 0.049 12.466 0.074 2009.274 11.066 0.006 2012.452 11.077 0.001 –99.000 –99.000 –99.000 9.889 0.024 –0.043 0.395 –0.068 0.576 1 0 0.706
6567 4 38.605 8.312 15.828 0.080 11.931 0.094 2009.274 10.379 0.003 2012.452 10.317 0.001 –99.000 –99.000 –99.000 9.138 0.018 2.154 0.396 –1.774 0.575 0 0 0.008
...

Field 5

7907 5 19.300 –14.900 12.928 0.055 9.594 0.194 2009.274 8.427 0.198 2012.586 7.601 0.002 –99.000 –99.000 –99.000 6.281 0.004 8.176 3.260 –0.836 0.720 0 1 0.004
7908 5 35.105 –11.798 13.951 0.066 10.202 0.097 2009.274 8.915 0.097 2012.586 9.089 0.001 –99.000 –99.000 –99.000 6.697 0.074 5.465 1.121 0.976 1.001 0 1 0.000
...

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. The proper motions of each star relative to the cluster motion are given as μαcosδ and μδ with their respective uncertainties in milliarcseconds/year. Membership candidates as well as L-band excess sources are indicated in the columns “Mem” and “Exc”, but membership selection is not absolute (1: cluster member candidate, 0: likely non-member, 1: membership unknown). Stars in the outer fields are considered members if their formal membership probability, pclus, exceeds 0.4. The first few bright sources shown for reference here are Wolf-Rayet cluster stars, yet their motions are uncertain owing to non-linearity effects in Ks. The full version of the table is available at the CDS.

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