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Table 7

Astrometric parameters of the kinematic members derived in this work with their associated membership probability.

Object RA Dec σpos μα μ δ EpRA EpDec 2MASS Ks NEp Dt Prob
[h m s] [°] [mas] [mas/yr] [mas/yr] [yr] [yr] [mag] [yr]

2MASS J16264172-2453586 16 26 41.7218 –24 53 58.618 5 –11.8 ± 0.7 –21.4 ± 1.4 2007.9 2007.8 13.740 ± 0.045 6 29.6 0.99
2MASS J16264441-2447138 16 26 44.4164 –24 47 13.835 6 -4.8 ± 2.1 –23.2 ± 2.2 2006.7 2006.7 10.635 ± 0.021 7 29.6 1.00
2MASS J16264890-2449087 16 26 48.9022 –24 49 8.673 4 –13.4 ± 1.5 –23.0 ± 1.3 2007.0 2007.0 14.206 ± 0.068 5 12.1 1.00
2MASS-6X J16265634-2442375 16 26 56.3364 –24 42 37.616 3 –13.2 ± 1.3 –25.1 ± 1.1 2007.2 2007.2 15.759 ± 0.131 4 5.4 1.00
2MASS J16265843-2445318 16 26 58.4414 –24 45 31.878 6 –11.3 ± 1.7 –25.1 ± 1.9 2007.6 2007.6 7.549 ± 0.046 6 9.9 1.00
2MASS J16265861-2446029 16 26 58.6166 –24 46 2.864 2 -6.3 ± 0.9 –20.0 ± 0.8 2007.4 2007.5 13.314 ± 0.027 8 12.1 0.97
UGCS J162700.96-244339.5 16 27 0.9758 –24 43 39.530 2 –17.7 ± 0.8 –26.5 ± 0.6 2007.6 2007.7 5 6.1 1.00

Notes. The full table is available at the CDS. Colums (7) and (8) provide the mean epoch corresponding to the J2000 RA, Dec positions, Col. (10) lists the number of epochs of the observations, Col. (11) their time base and Col. (12) the membership probability. μα stands for μαcos(δ). Note that Ks magnitudes without error are just estimative. Objects not detected by 2MASS or WISE were searched in the 2MASS 6X (Cutri & IPAC/WISE Science Data Center Team 2012) and the UKIDSS (Lawrence et al. 2007) catalogues and attributed their identificators. A local identificator (BXhhmmss.sss+dddmmss.ss) was attributed to the faintest source not found in these catalogues.

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