Open Access
Table A.1
Sources and characteristics of the used observational material taken from the ESO archives.
| N | Instrument | Program Id | Spectral range (Å) | R | S/N a |
|---|---|---|---|---|---|
| 1. | UVES | UVESPOP | 3040 − 10400 | 88 000 | 460 |
| 2. | UVES | 65.L-0507(A) | 3040 − 6835 | 41 000, 51 000 | > 150 |
| 3. | UVES | 67.D-0086(A) | 3280 − 6690 | 50000 | 100 |
| 4. | UVES | 67.D-0439(A) | 3024 − 6835 | 50 000, 57 000 | > 250 |
| 5. | UVES | 68.D-0094(A) | 3040 − 6835 | 41 000, 51 000 | > 200 |
| 6. | UVES | 68.B-0475(A) | 3040 − 6835 | 37 000, 46 000 | > 100 |
| 7. | UVES | 68.D-0546(A) | 3030 − 6830 | 41 000, 57 000 | 100 |
| 8. | UVES | 71.B-0529(A) | 3043 − 6808 | 41 000, 45 000 | 100 |
| 9. | UVES | 072.B-0585(A) | 3030 − 6835 | 41 000, 45 000 | > 100 |
| 10. | UVES | 076.B-0055(A) | 3732 − 5000 | 41 000 | 290 |
| 11. | UVES | 165.N-0276(A) | 3084 − 6835 | 68 000, 81 000 | 80 |
| 12. | UVES | 165.L-0263(A) | 3377 − 4653 | 41 000 | 120 |
| 13. | UVES | 165.L-0263(B) | 3559 − 4845 | 41 000 | > 150 |
| 14. | UVES | 170.D-0010 | 3030 − 6840 | 71 000 | 24 |
| 15. | UVES | 188.B-3002(C) | 4180 − 6213 | 47 000 | > 200 |
| 16. | UVES | 266.D-5655(A) | 3024 − 6835 | 65 000,74 000 | 90 |
| 17. | UVES | 280.D-5011 | 3330 − 6800 | 60000 | 20 |
| 18. | UVES | 109.22VP.001 | 3282 − 6686 | 58 600, 66 300 | > 100 |
| 19. | UVES | 109.22VP.002 | 3282 − 4563 | 58 600 | 117 |
| 20. | UVES | 110.240W.001 | 3282 − 6686 | 58 600, 66 300 | > 160 |
| 21. | UVES | 110.240W.002 | 3282 − 4563 | 58 600 | 145 |
| 22 | HARPS | 60.A-9700(G) | 3780 − 6910 | 115 000 | 175 |
| 23 | HARPS | 072.C-0488(E) | 3780 − 6910 | 115 000 | > 75 |
| 24 | HARPS | 096.D-0402(A) | 3780 − 6910 | 115 000 | 84 |
| 25 | FEROS | 072.D-0315(A) | 3528 − 9218 | 48 000 | 140 |
Notes. aThe signal-to-noise ratio is given for λ ~ 3400 Å. For the longer wavelengths, up to 6500 Å, S/N > 100. UVESPOP = Bagnulo et al. (2003).
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