Table 3
Angular diameters obtained with VEGA/CHARA and the corresponding surface brightnesses.
| Star | mV | mK | AV |  |
 |
 |
u[710] |  |
 |
 |
|---|---|---|---|---|---|---|---|---|---|---|
| [mag] | [mag] | [mag] | [mag] | [mas] | [mas] | [mag] | [mas] | |||
| HD 11037 | 5.910±0.010 | 3.666±0.010 | 0.031 | 2.216 |  |
1.3 | 0.631 |  |
 |
|
| HD 13468* | 5.940±0.010 | 3.666±0.010 | 0.028 | 2.248 |  |
1.6 | 0.628 |  |
 |
0.886±0.009 |
| HD 22798 | 6.220±0.010 | 3.880±0.010 | 0.012 | 2.329 |  |
2.9 | 0.631 |  |
 |
|
| HD 23526* | 5.910±0.010 | 3.634±0.010 | 0.053 | 2.228 |  |
0.6 | 0.631 |  |
 |
0.915±0.020 |
| HD 360* | 5.990±0.010 | 3.653±0.010 | 0.028 | 2.311 |  |
0.5 | 0.658 |  |
 |
0.906±0.014 |
| HD 40020* | 5.890±0.010 | 3.419±0.010 | 0.040 | 2.434 |  |
0.4 | 0.668 |  |
 |
1.012±0.022 |
| HD 43023 | 5.830±0.010 | 3.704±0.010 | 0.003 | 2.123 |  |
1.1 | 0.631 |  |
 |
|
| HD 5268 | 6.150±0.010 | 3.910±0.010 | 0.043 | 2.200 |  |
0.5 | 0.628 |  |
 |
Notes. For each star, we consider an uncertainty of 0.01 magnitude for mV and mK (Laney et al. 2012). The angular diameter of stars marked with an asterisk is based on PIONIER/VLTI observations provided in the extended data Table 2 of Pietrzyński et al. (2019). This is reported here in the last column.
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