Table 1
Number of observations of each star in our sample with the different spectrographs (the HPF spectrograph, H: HARPS, S: SOPHIE, HN: HARPS-North).
| Star | HPF | H | S | HN | Total |
|---|---|---|---|---|---|
| S488 | 6 | 6 (43) | |||
| S815 | 5 | 5 (33) | |||
| S995 | 11 | 2 | 2 | 15 | |
| S1083 | 32 | 3 | 2 | 4 | 41 |
| S1268 | 38 | 2 | 2 | 4 | 46 |
| S1429 | 39 | 4 | 2 | 9 | 54 |
| S1557 | 5 | 5 (42) | |||
| S2207 | 14 | 4 | 2 | 6 | 26 |
| YBP778 | 3 | 1 | 4 (27) | ||
| YBP1062 | 3 | 1 | 4 (26) | ||
| YBP1137 | 4 | 4(17) | |||
| YBP2018 | 4 | 1 | 5(39) |
Notes. Only observations that were not reported in Brucalassi et al. (2017) are listed. Stars that were not in the original sample are marked in bold. The number in parentheses shows the total number of observations over the entire survey for the given target.
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