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Table 2.

Parallax distributions from the initial sample of cluster members using a KDE based on Gaia DR2 data.

Stellar ϖmode ϖKDE [mas]
dmode dKDE [pc]
association [mas] 2.5th 25th 75th 97.5th [pc] 2.5th 25th 75th 97.5th
Alpha Persei 5.73192 5.32825 5.58102 5.84774 6.15589 174.461 187.678 179.178 171.006 162.446
NGC 1960 0.82873 0.65783 0.77649 0.87735 0.99241 1 206.665 1 520.149 1 287.846 1 139.795 1 007.648
IC 4665 2.88239 2.34501 2.72233 2.99779 3.28228 346.934 426.437 367.332 333.579 304.666
NGC 2547 2.52757 1.98269 2.40987 2.61619 2.89936 397.379 504.365 414.960 382.235 344.903
IC 2602 6.57185 6.11623 6.42974 6.70321 7.08069 152.164 163.499 155.527 149.182 141.229
IC 2391 6.59159 6.14352 6.44991 6.71406 7.11775 151.708 162.773 155.040 148.941 140.494
The Pleiades 7.35915 6.77853 7.18755 7.51509 8.02017 135.885 147.524 139.129 133.065 124.685
Blanco 1 4.17949 3.98254 4.13539 4.30490 4.47278 239.264 251.096 241.815 232.293 223.574
The Hyades 21.08226 16.44997 19.67124 22.48718 27.34499 47.433 60.790 50.835 44.469 36.569
32 Ori MG 9.62252 (a) 8.30029 8.97758 10.19470 10.76314 103.922 (b) 120.477 111.388 98.090 92.909

Notes.

(a)

This value is not the ϖmode it is the 50th percentile of the parallax PDF, ϖKDE.

(b)

The value is calculated using the value marked asa.

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