Table 3.
Fitting result of K − Pb corresponds to different combinations of the distance measurement.
| Significance | Groups | Num | β | log α |  |
|---|---|---|---|---|---|
| 1σ | A | 9 |
 |
 |
0.39 |
| A,B | 14 |
 |
 |
2.33 | |
| A,B,C | 19 |
 |
 |
3.51 | |
| 2σ | A | 5 |
 |
 |
0.82 |
| A,B | 7 |
 |
 |
3.36 | |
| A,B,C | 11 |
 |
 |
5.20 | |
| 3σ | A,B,C | 6 |
 |
 |
0.36 |
Notes. The different groups are denoted as follows: “A” corresponds to sources with a distance measured by the globular cluster; “B” is for sources with a distance measured by pulsar timing; and “C” corresponds to sources with a distance measured by the DM, and two systems with a distance measured by the globular cluster that do not have a not proper motion measurement also belong to Group C.
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