Table A.3
Characteristics of the used observational material.
| N | Telescope/spectrograph, | Spectral range (Å), | Objects | Method of analysis |
| PIDs | R, S/Na | |||
|
|
||||
| 1. | VLT2/UVES, | 3600–6800, | Sculptor: | Wobs(JNM15), |
| 087.D-0928A, | R≃ 45 000, | ET0381, 002_06, | synt | |
| 091.D-0912A | S/N = 30–45 | 03_059, 031_11, | ||
| 074_02 | ||||
| 2. | VLT2/UVES, | 3800–6800, | Scl07-49, 07-50, | Wobs(TJH10), |
| 079.B-0672A, | R≃ 45 000, | Fnx05-42, | synt | |
| 081.B-0620A, | S/N = 30–40 | Sex11-04, 24-72 | ||
| 281.B-50220A | ||||
| 3. | Magellan/MIKE, | 3460–9410, | Sculptor: | Wobs(SJF15), |
| SJF15 | R≃ 25 000, S/N≃ 80, | 11_1_4296, 6_6_402, | synt | |
| R≃ 33 000, S/N = 171 | S1020549 | |||
| 4. | Keck I/HIRES, | 3927–8362, | Scl 1019417 | Wobs(KC12) |
| KC12 | R≃ 29 300, S/N≃ 105 | |||
| 5. | Keck I/HIRES, | 3810–6700, | Ursa Minor: | Wobs(CH10) |
| CH10 | R≃ 35 000, S/N≃ 80 | COS233, JI19, 28104, | ||
| 33533, 36886, 41065 | ||||
| 6. | Keck I/HIRES, | 3927–8362, | UMi 20103 | Wobs(KC12) |
| KC12 | R≃ 34 500, S/N≃ 90 | |||
| 7. | Keck I/HIRES, | 4400–7500, | Ursa Minor: | Wobs(UCK15) |
| UCK15 | S/N≃ 25, 30, 12 | 718, 396, 446 | ||
| 8. | VLT2/FLAMES/UVES, | 4800–5750, 5840–6800, | Boötes I: | Wobs(GNM13) |
| P82.182.B-0372 | R≃ 47 000, | 33, 41, 94, 117 | ||
| S/N = 30, 60 | 127, 130 | |||
| 9. | VLT2/UVES, | 3300–4520, 4620–5600, 5680–6650 | Boo-1137 | Wobs(NYG10) |
| P383.B-0038 | R≃ 40 000, S/N = 70 | |||
| 10. | Magellan/MIKE, | 3500–9000, R≃ 28 000, | Boötes I: | Wobs(FNG16), |
| FNG16 | S/N = 25–30 | 127, 980 | synt | |
| 11. | Keck I/HIRES, | 4100–7200, | UMa II: | Wobs(FSG10) |
| FSG10 | R≃ 37 000, | S1, S2, S3 | ||
| S/N = 25–30 | ||||
| 12. | Magellan/MIKE, | 3350–5000, 4900–9300, | Leo IV-S1 | Wobs(SFM10) |
| SFM10 | R≃ 28 000, 22 000, | |||
| S/N = 25 | ||||
| 13. | VLT2/UVES, | 3758–4984, 4780–5758, 5834–6809 | HD 2796 | synt |
| 076.D-0546(A) | R≃ 71 050, S/N = 339, | |||
| R≃ 107 200, S/N = 256 | ||||
| 14. | VLT2/UVES, | 3758–4982, 4780–5757, 5834–6808 | HD 8724 | synt |
| 71.B-0529(A) | R≃ 40 970, S/N> 200 | HD 128279 | ||
| R≃ 45 250, S/N> 250 | ||||
| 15. | VLT2/UVES, | 4780–5757, 5834–6808 | HD 108317 | synt |
| 68.D-0546(A) | R≃ 56 990, S/N = 100 | HD 218857 | ||
| 16. | VLT2/UVES, | 3400–4510, S/N = 50 | HE2252-4225 | synt |
| 170.D-0010, | 3756–4978, 4785–5745, 5830–6795 | HE2327-5642 | ||
| 280.D-5011 | R≃ 50 000, S/N = 100 | |||
| 17. | VLT2/UVES, | 4774–5758, 5827–6809 | CD− 24° 1782 | synt |
| 165.N-0276(A) | R≃ 80 930, S/N = 138 | |||
| 18. | Magellan/MIKE, | 3320–9000, R≃ 60 000 | HD 108317 | synt |
| Rana Ezzeddine | CD − 24° 1782 | |||
| 19. | CFHT/ESPaDOnS, | 3696–10483 | HD 4306 | synt |
| 12BS04 | R≃ 85 400, S/N > 110 | BD− 11° 0145 | ||
| 20. | VLT2/UVES, | 3040–10400 | HD 122563 | synt |
| UVESPOP | R≃ 88 000, S/N = 460 | |||
| 21. | CFHT/ESPaDOnS, | 3695–10481 | HD 122563 | synt |
| 05AC23 (3 spectra) | R≃ 64 340, S/N = 93 | |||
| 22. | Keck I/HIRES, | 3805–5325, | HE0011-0035 | Wobs(CCT13) |
| CCT13 | R≃ 36 000, | HE0332-1007 | ||
| S/N > 100 | HE1356-0622 | |||
| HE1357-0123 | ||||
| HE2249-1704 | ||||
| 23. | Keck I/HIRES, | 3250–5990, | HE0048-0611 | Wobs(CCT13) |
| CCT13 | R≃ 36 000, | HE0122-1616 | ||
| S/N≥ 100 | HE0445-2339 | |||
| HE1416-1032 | ||||
| HE2244-2116 | ||||
| BS16550-087 | ||||
| 24. | Magellan/MIKE, | 3350–5000, R≃ 42 000, | HE0039-4154 | Wobs(CCT13) |
| CCT13 | 4900–9300, R≃ 32 000, | HE1416-1032 | ||
| S/N = 120, 90 | ||||
Notes.
The signal-to-noise ratio, as given in the original papers for a wavelength of about 5300 Å. Average S/N is indicated for the MW stars observed with VLT2/UVES and CFHT/ESPaDOnS.
Reference. CCT13 = Cohen et al. (2013), CH10 = Cohen & Huang (2010), FNG16 = Frebel et al. (2016), FSG10 = Frebel et al. (2010), GNM13 = Gilmore et al. (2013), JNM15 = Jablonka et al. (2015), KC12 = Kirby & Cohen (2012), NYG10 = Norris et al. (2010), SFM10 = Simon et al. (2010), SJF15 = Simon et al. (2015), TJH10 = Tafelmeyer et al. (2010), UCK15 = Ural et al. (2015), UVESPOP = Bagnulo et al. (2003).
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