Open Access
Table B.4.
Same as Table B.2.
| Arm | Group | p-value | Nspiral | Retrieved | % retrieved | Extra | % extra |
|---|---|---|---|---|---|---|---|
| Norma | [7, 4] | 0.00 | 56 | 56 | 100.00 | 11 | 19.64 |
| Sct-Cen | [8, 4] | 0.47 | 108 | 108 | 100.00 | 25 | 23.15 |
| Sgr-Car | [2, 6, 5] | 0.02 | 98 | 98 | 100.00 | 35 | 35.71 |
| Local | [0] | 0.27 | 88 | 88 | 100.00 | 24 | 27.27 |
| Perseus | [14, 16, 15, 13, 12, 17] | 0.43 | 341 | 337 | 98.83 | 49 | 14.37 |
| Outer | [1] | 0.00 | 208 | 208 | 100.00 | 113 | 54.33 |
Notes. In this test case, random noise is added to the (x,y) coordinates of the stars in the mock spiral arms, and a large number of inter-arms’ Cepheids is included in the sample. The table also indicates the number and percentage of inter-arms’ stars wrongly included in the spiral arms.
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