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Table 1

3σ-significant kinematic structures detected for level J = 3, 8–16 km s-1, NMC = 2000.

N Name U V ΔU ΔV N ∗ SN BSN D TD
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
55 831 31 533 24 298 36 439 11 410
1 Sirius 30 −3 3 1 31 434 + + +
2 Sirius 0 8 7 3 154 4821 + + + +
3 Sirius −11 9 3 1 83 879 + +
4 Coma B 9 −12 2 2 52 1102 + +
5 Coma B −2 −11 3 3 70 2753 + + +
6 Coma B −15 −7 1 1 79 673 + + +
7 Hyades −44 −18 6 2 90 2344 + +
8 Pleiades −22 −23 7 3 170 4257 + + +
9 Wolf630+Dehnen98 43 −22 9 2 168 1777 + +
10 Hercules −38 −49 9 3 116 1451 + +
11 Hercules −16 −48 2 1 22 197 + +
12 γLeo 52 0 1 2 27 96 + +
13 New 37 8 2 2 74 201 + + +
14 Antoja12(15) 48 −68 1 1 6 8 + +
15 Antoja12(12) 94 −13 1 1 38 10 + +
16 Bobylev16 −94 −5 1 1 17 14 + + + +
17 ϵInd −88 −48 2 2 12 24 +
18 Unknown −86 −76 2 1 8 12 +
19 Unknown −18 −67 1 1 22 70 + +

Notes. Columns 1–8 are for the total sample. Column 1 gives the order of positions of wavelet coefficients for J = 3 obtained for 2000 synthetic data samples. Column 2 is the name of the structure if available in literature. Columns 3 and 4 are central positions of kinematic structures in km s-1, their uncertainties (standard deviations) are given in Cols. 5 and 6 respectively also in km s-1. Column 7 is a percentage showing how many times the structure obtained by MC simulations appears in the wavelet space. The estimated number of stars in each group is given in Col. 8. Columns 9–12 show the presence of the structure in the SN, BSN, D and TD samples for J = 3 with + sign. Number of stars of each data sample is indicated in the row 3. Question marks correspond to tentatively new structures with a small detection percentage in MC simulation.

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