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Table 1
Stars analysed in this study.
| Star | Instrument | R | λ (Å) | S/N |
|
|
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| Normal stars | ||||
| HD 22 136 | ESPaDOnS | 65 000 | 3690−10 481 | 504 |
| HD 160 762 | ESPaDOnS | 65 000 | 3690−10 481 | 600 |
| HD 162 586 | UVES | 110 000 | 3070−10 398 | 655 |
| HD 170 054 | ESPaDOnS | 65 000 | 3690−10 481 | 283 |
| HD 179 761 | ELODIE | 42 000 | 4000−6800 | 125 |
| HD 195 810 | ESPaDOnS | 65 000 | 3690−10 481 | 774 |
| HD 222 173 | ELODIE | 42 000 | 4000−6800 | 159 |
|
|
||||
| HgMn stars | ||||
| HD 27 295 | UVES | 110 000 | 3750−6800 | 218 |
| HD 57 608 | FEROS | 48 000 | 3528−9217 | 142 |
| HD 78 316 | UVES | 110 000 | 3750−6800 | 265 |
| HD 175 640 | UVES | 110 000 | 3750−5800 | 439 |
| HD 178 065 | UVES | 110 000 | 3750−5800 | 461 |
| HD 186 122 | ESPaDOnS | 65 000 | 3690−10 481 | 662 |
| HD 193 452 | CF4 | 120 000 | 4630−5478 | 556 |
|
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| Magnetic Bp stars | ||||
| HD 10 840 | UVES | 110 000 | 3070−10 398 | 824 |
| HD 45 583 | FEROS | 48 000 | 3528−9217 | 231 |
| HD 47 116 | UVES | 110 000 | 3070−10 398 | 527 |
| HD 49 333 | UVES | 110 000 | 3070−10 398 | 791 |
| HD 61 045 | ESPaDOnS | 65 000 | 3690−10 481 | 298 |
| HD 74 168 | UVES | 110 000 | 3070−10 398 | 334 |
| HD 74 535 | FEROS | 48 000 | 3528−9217 | 310 |
| HD 133 880 | ESPaDOnS | 65 000 | 3690−10 481 | 365 |
| HD 137 509 | UVES | 110 000 | 3690−10 481 | 430 |
| HD 147 010 | ESPaDOnS | 65 000 | 3690−10 481 | 587 |
| HD 199 728 | UVES | 110 000 | 3070−10 398 | 593 |
| HD 223 640 | UVES | 110 000 | 3070−10 398 | 560 |
| HD 304 842 | FEROS | 48 000 | 3528−9217 | 262 |
| HD 318 107 | ESPaDOnS | 65 000 | 3690−10 481 | 320 |
| BD+00 1659 | ESPaDOnS | 65 000 | 3690−10 481 | 475 |
| BD-19 5044L | ESPaDOnS | 65 000 | 3690−10 481 | 358 |
| BD+49 3789 | ESPaDOnS | 65 000 | 3690−10 481 | 191 |
Notes.Listed are the star designations, instrument used, spectral resolution, spectral range and the S/N.
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