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Table 2.

Details of individual detections.

Source ID Detect. sources Sep. Proj. sep. PA fr L Δmag Pspur
(arcsec) (au) (deg) (%) (mag) (mag) (%)
G203.3166+02.0564 A 12.41 9185 45.8 1.65 ± 0.19 6.2 4.5 0.37
B 12.3 9099 46.7 4.58 ± 0.28 5.0 3.3 0.18
C 5.113 3784 11.7 1.06 ± 0.07 6.6 4.9 0.11
D 3.848 2848 317 0.62 ± 0.04 7.2 5.5 0.075
E 4.605 3408 288 3.05 ± 0.20 5.5 3.8 0.036
F 6.36 4706 276 0.50 ± 0.03 7.4 5.7 0.24
G 2.738 2026 276 4.25 ± 0.27 5.1 3.4 0.011
H 2.445 1809 165 0.69 ± 0.04 7.1 5.4 0.029
I 9.226 6827 110 0.20 ± 0.02 8.5 6.8 1.4

G232.6207+00.9959 A 14.22 23 880 32.2 38.06 ± 1.30 6.3 1.0 0.83
B 15.77 26 500 57.2 10.53 ± 0.38 7.7 2.4 3.4
C 8.575 14 410 21.2 4.94 ± 0.40 8.6 3.3 2.2
D 9.392 15 780 48.7 18.47 ± 0.66 7.1 1.8 0.75
E 8.403 14 120 309 69.04 ± 2.60 5.7 0.4 0.17
F 5.114 8591 43.9 9.90 ± 0.39 7.8 2.5 0.37
G 9.182 15 430 133 21.94 ± 0.80 6.9 1.6 0.57

G263.7759−00.4281 A 10.28 7199 45.5 3.09 ± 0.22 9.5 3.8 1.2
B 10.33 7229 46.3 2.57 ± 0.20 9.7 4.0 1.4
C 2.812 1968 123 13.35 ± 1.10 7.9 2.2 0.03

G265.1438+01.4548 A 13.51 9456 354 9.87 ± 0.70 6.3 2.5 1.5
B 14.27 9986 331 6.37 ± 0.51 6.8 3.0 2.3
C 12.65 8853 313 11.58 ± 0.82 6.1 2.3 1.2
D 10.41 7289 314 5.27 ± 0.43 7.0 3.2 1.4
E 10.32 7222 313 3.79 ± 0.37 7.4 3.6 1.8
F 7.199 5039 50.4 4.21 ± 0.33 7.2 3.4 0.83
G 7.153 5007 198 5.40 ± 0.46 7.0 3.2 0.67
H 14.03 9822 119 13.05 ± 0.96 6.0 2.2 1.3
I 13.49 9443 125 25.14 ± 1.80 5.3 1.5 0.75
J 16.32 11 430 134 107.10 ± 7.60 3.7 -0.1 0.32
K 9.092 6364 328 14.08 ± 1.10 5.9 2.1 0.52

G268.3957−00.4842 A 9.047 6333 275 0.16 ± 0.01 10.9 7.0 32
B 1.929 1350 168 8.58 ± 0.45 6.6 2.7 0.05
C 4.769 3338 183 1.97 ± 0.10 8.2 4.3 1.1
D 8.202 5741 197 8.88 ± 1.40 6.5 2.6 0.81
E 8.355 5848 198 41.94 ± 1.70 4.8 0.9 0.29

G269.1586−01.1383A A 8.474 5932 208 77.45 ± 2.90 7.7 0.3 2.4
B 8.544 5981 156 31.55 ± 1.30 8.7 1.3 5.5

G305.2017+00.2072A A 1.485 5940 78.5 16.64 ± 1.20 7.4 1.9 0.24
B 8.77 35 080 165 17.18 ± 1.10 7.4 1.9 7.8

G310.0135+00.3892 A 2.604 8464 225 9.91 ± 0.68 4.8 2.5 0.11
B 16.32 53 040 133 0.20 ± 0.01 9.1 6.8 69

Notes. We provide their separations both in arcsec and au and their apparent L′-band magnitudes determined relative to the primaries. Errors on the physical separations are based on the distance uncertainties provided in the RMS catalogue and following Reid et al. (2009) models, i.e. 10%. Δmag is the magnitude difference between the secondary and the primary, directly retrieved from the flux ratio. The last column provides the probabilities of chance projection of all the detected sources. The boldface spurious association values in the last columns indicate a non-negligible probability of being background sources.

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