Table 3
Calibration stars used for the instrumental response correction, including their observation frequency and the astrophysical parameters used as input to generate our SED models.
| Target | Teff (K) | log 𝑔 (dex) | υ sin i (km s−1) | υmic (km s−1) | [M/H] | #nights |
|---|---|---|---|---|---|---|
| HD 36267 | 15 250 | 4.2 | 127 | 0.6 | 0.0 | 29 |
| HD 152614 | 11 750 | 3.9 | 109 | 1.5 | 0.0 | 40 |
| HD 149212 | 10500 | 3.8 | 157 | 0.0 | 0.4 | 10 |
| HD 14055 | 10250 | 4.3 | 235 | 2.6 | −0.1 | 58 |
| HD 87887 | 10250 | 3.7 | 22 | 1.2 | 0.1 | 26 |
| HD 42818 | 10000 | 4.2 | 275 | 2.5 | 0.1 | 18 |
| HD 214994 | 9500 | 3.6 | 15 | 2.1 | 0.2 | 6 |
| HD 46300(a) | 9500 | 2.0 | 100 | 2.0 | 0.0 | 36 |
| HD 118098 | 8300 | 3.7 | 213 | 2.3 | −0.2 | 66 |
| GSC4293-0432 | 8000 | 4.0 | 40 | 3.1 | 0.3 | 2 |
| HD 56169 | 7900 | 2.7 | 216 | 3.3 | −0.6 | 27 |
| HD 184006 | 7800 | 3.0 | 245 | 3.6 | −0.4 | 46 |
| HD 147449 | 7100 | 4.0 | 79 | 2.9 | 0.0 | 17 |
| HD 84937 | 6400 | 3.8 | 5 | 1.7 | −2.1 | 12 |
Notes. Errors on the astrophysical parameters derived from atmospheric modelling in GSSP are on the order of 100 K in Teff, 0.1 dex in log 𝑔, 1 km s−1 in υ sin i, 0.1 km s−1 in υmic, and 0.1 dex in [M/H]. (a)The model for this object was taken from the synthetic library of Munari et al. (2005).
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