| Star | AO (0.5'') | AO (1.0'') | SDI (0.5'') | SDI (1.0'') | RV 70% | RV 90% | RV 95% |
| HD25874 | 9.5-71
|
11.2-68
|
11.2-68
|
11.3-67
|
2
|
4
|
9
|
| HD32778 | 8.7-72
|
9.0-71
|
8.9-71
|
9.3-71
|
- | - | - |
| HD91204 | 9.5 | 70
|
10.1 | 68
|
10.0-68
|
10.0-67
|
3
|
13
|
30
|
| HD120780 | 8.9-66
|
9.8 | 60
|
10.0-59
|
10.3-57
|
3
|
35
|
23
|
| HD145825 | 9.3-57
|
10.9-41
|
10.6-44
|
11.0-40
|
3
|
11
|
15
|
Notes. Columns 2 and 3 show the AO reduced contrast limits and their associated T5 mass limits at the age of each star for angular separations of 0.5'' and 1.0'' respectively. Columns 4 and 5 show the same results but for the SDI reduction. Columns 6-8 show the minimum mass that was ruled out at confidence levels of 70, 90 and 95% respectively. These masses were for all separations and therefore show only the lowest mass reached by the simulations and are not constrained within a separation limit. Note the lack of this data for HD32778 due to the limited radial-velocity data set.
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