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Table C.1.

Properties of the 1052 candidate members.

statistical group source_id ra dec mean_X sd_X mean_Y sd_Y mean_Z sd_Z mean_U sd_U mean_V sd_V mean_W sd_W lower_mass map_mass upper_mass lower_Av map_Av upper_Av
[°] [°] [pc] [pc] [pc] [pc] [pc] [pc] [km s−1] [km s−1] [km s−1] [km s−1] [km s−1] [km s−1] [M] [M] [M] [mag] [mag] [mag]
Heleus 120101686623435648 56.05054 30.14774 190.76 4.79 283.42 6.89 198.45 4.92 8.73 0.71 21.84 1.003 2.25 0.80 0.293 0.323 0.398 0.551 0.810 1.468
Heleus 120108691713952256 55.75415 30.05330 177.56 6.55 260.63 9.48 182.57 6.72 8.61 0.80 21.83 1.036 2.65 0.91 0.187 0.234 0.301 1.061 1.689 2.341
Gorgophone_halo 120110409701337984 55.70667 30.13254 139.01 7.70 203.92 10.99 143.93 7.98 5.24 1.40 19.60 2.058 -4.73 1.43 0.046 0.044 0.075 0.219 0.129 1.208
Heleus 120114846403228928 55.95374 30.22572 190.83 2.21 282.43 3.19 198.59 2.29 8.69 0.66 21.84 0.968 2.32 0.70 0.871 0.964 1.084 0.826 1.154 1.627
Heleus 120175349606916736 55.47514 30.35383 177.01 8.02 258.06 11.33 183.77 8.42 8.56 0.89 21.21 1.069 1.99 0.98 0.073 0.084 0.144 0.813 1.142 2.176
Gorgophone_halo 120189265300085760 55.54816 30.60905 144.58 2.11 210.75 3.00 151.21 2.23 3.57 1.16 21.06 1.710 -4.83 1.22 0.493 0.555 0.638 1.297 1.644 2.067
Gorgophone_halo 120241285944294016 54.67945 30.08919 147.98 6.47 209.31 8.82 148.80 6.45 4.91 1.32 18.85 1.943 -3.21 1.31 0.176 0.217 0.281 1.573 2.029 2.784
Gorgophone_core 120329388609121536 54.17275 30.63557 150.33 1.37 208.22 1.94 152.19 1.41 3.78 0.82 20.99 1.135 -1.32 0.84 0.397 0.478 0.542 1.548 2.110 2.502
Gorgophone_halo 120389513854974208 54.95708 30.72561 154.74 6.05 221.00 8.39 160.31 6.30 3.20 1.22 20.61 1.817 -2.95 1.26 0.191 0.276 0.296 1.574 2.536 2.710
Heleus 120392537512343296 55.19657 30.74791 170.51 7.34 244.62 10.23 177.69 7.75 8.37 0.87 21.38 1.030 2.74 0.95 0.160 0.208 0.278 2.022 2.748 3.524

Notes. This table will be available in its entirety in machine-readable form at the CDS. For each candidate member we provide its parent statistical group, Gaia DR3 source id and sky coordinates, mean and standard deviation of the Cartesian ICRS phase-space coordinates X, Y, Z, U, V, and W, and lower percentiles (2.5%), maximum-a-posteriori, and upper percentiles (97.5%) of the estimated mass and extinction in the V band.

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