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Table 5
Signal to noise measured around λ6000 for stars analyzed here and in Allen & Barbuy (2006a).
| Star | SN | Star | SN | Star | SN | Star | SN |
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|
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| HD 749 | 220 | HD 26967* | 180 | HD 107574 | 230 | HD 188985 | 150 |
| HD 2454 | 210 | HD 27271 | 220 | HD 113226* | 330 | HD 202109 | 190 |
| HD 5424 | 150 | HD 46407 | 160 | HD 116713 | 110 | HD 204075 | 320 |
| HD 8270 | 230 | HD 48565 | 220 | HD 116869 | 190 | HD 205011 | 210 |
| HD 9362* | 310 | HD 76225 | 140 | HD 123396 | 200 | HD 210709 | 170 |
| HD 12392 | 180 | HD 87080 | 200 | HD 123585 | 100 | HD 210910 | 260 |
| HD 13551 | 190 | HD 89948 | 370 | HD 139195 | 420 | HD 220009* | 390 |
| HD 13611* | 370 | HD 92545 | 140 | HD 147609 | 150 | HD 222349 | 130 |
| HD 20894* | 440 | HD 104979 | 140 | HD 150862 | 180 | BD+18 5215 | 100 |
| HD 22589 | 190 | HD 106191 | 110 | HD 181053 | 240 | HD 223938 | 360 |
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