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] | |||||
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Field 1 | |||||||||||||||||||||||||
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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 |
... | |||||||||||||||||||||||||
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Field 2 | |||||||||||||||||||||||||
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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 |
... | |||||||||||||||||||||||||
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Field 3 | |||||||||||||||||||||||||
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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 |
... | |||||||||||||||||||||||||
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Field 4 | |||||||||||||||||||||||||
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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 |
... | |||||||||||||||||||||||||
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Field 5 | |||||||||||||||||||||||||
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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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