Table 1
Properties of the stars of the studied sample.
| HD | Name | Sp. class | m V | m K |
|
|
||||
| 3651 | 54 Psc | K0V | 5.88 | 4.00 |
| 9826 | υ And | F8V | 4.09 | 2.86 |
| 19994 | 94 Cet | F8V | 5.07 | 3.75 |
| 75732 | 55 Cnc | G8V | 5.96 | 4.05 |
| 167042† | – | K1IV | 5.97 | 3.58 |
| 170693 | 42 Dra | K1.5III | 4.82 | 2.09 |
| 173416 | G8III | 6.04 | 3.85 | |
| 185395 | θ Cyg | F4V | 4.49 | 3.54 |
| 190360 | – | G6IV | 5.73 | 4.11 |
| 217014 | 51 Peg | G2IV | 5.45 | 3.91 |
| 221345 | 14 And | K0III | 5.23 | 2.33 |
|
|
||||
| 1367 | ρ And | K0II | 6.18 | 4.23 |
| 1671 | – | F5III | 5.15 | 4.07 |
| 154633 | – | G5V | 6.11 | 3.93 |
| 161178 | – | G9III | 5.87 | 3.66 |
| 168151 | – | K5V | 4.99 | 3.94 |
| 209369 | 16 Cep | F5V | 5.03 | 3.96 |
| 218560 | – | K0III | 6.21 | 3.70 |
Notes. The eleven first ones (above the line) are known exoplanet hosts (except θ Cyg, see Ligi et al. 2012a). Photometry is given in the Johnson system (see Sect. 2).
HD 167042 was classified as a K1III giant by Hipparcos, but Sato et al. (2008) classify it as a less evolved subgiant because of its position on the H-R digram.
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