Table 4
Stellar counts after the corrections for incompleteness and field contamination.
| Target | rclus | rfield | Vlim |
|
|
|
| arcsec | arcsec | |||||
|
|
||||||
| NGC 152 | 90 | 150 | 22.5 | 1149 | 2931 | 1887 |
| Brück 6 | 18 | 90 | 22.5 | 50 | 129 | 105 |
| Kron 11 | 33 | 90 | 22.5 | 62 | 194 | 167 |
| Kron 8 | 33 | 90 | 23.0 | 187 | 491 | 367 |
| HW 6 | 24 | 90 | 22.7 | 50 | 104 | 66 |
| Lindsay 14 | 36 | 90 | 23.0 | 167 | 471 | 349 |
| Brück 2 | 20 | 90 | 22.0 | 23 | 66 | 62 |
| Brück 4 | 25 | 90 | 22.5 | 50 | 129 | 105 |
| HW 5 | 16 | 90 | 22.5 | 41 | 95 | 87 |
Notes. Columns correspond to the cluster name, the adopted cluster radius (rclus), the distance from the cluster centre to define the control field (rfield), the magnitude limit (Vlim), the number of observed stars in the cluster direction before any treatment for selection effects () and after the corrections for incompleteness () and field contamination ().
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