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Table 2.
Spectral properties of the templates used to derive radial velocities with TODMOR in the VIS and NIR channel spectra.
| Name | Teff, 1 | Teff, 2 | Spectral-line broadening |
L2/L1 |
||
|---|---|---|---|---|---|---|
| (K) | (K) | VIS | NIR | VIS | NIR | |
| (km s−1) | (km s−1) | |||||
| EZ Psc | 3300 ± 100 | 2900 ± 100 | 5.5 ± 0.1 | 7.1 ± 0.1 | 0.11 ± 0.01 | 0.12 ± 0.01 |
| GJ 1029 | 3100 ± 100 | 2900 ± 100 | 4.1 ± 0.1 | 3.6 ± 0.1 | 0.24 ± 0.01 | 0.32 ± 0.01 |
| Ross 59 | 3900 ± 100 | 3600 ± 100 | 1.6 ± 0.1 | 4.9 ± 0.1 | 0.10 ± 0.01 | 0.11 ± 0.01 |
| NLTT 23956 | 3100 ± 100 | 3000 ± 100 | 6.0 ± 0.1 | 5.9 ± 0.1 | 0.29 ± 0.01 | 0.37 ± 0.01 |
| GJ 3612 | 3600 ± 100 | 3300 ± 100 | 2.2 ± 0.1 | 4.6 ± 0.1 | 0.21 ± 0.01 | 0.25 ± 0.01 |
| GJ 1182 | 3300 ± 100 | 2900 ± 100 | 2.4 ± 0.1 | 4.0 ± 0.1 | 0.20 ± 0.01 | 0.29 ± 0.01 |
| UU UMia | 3500 ± 51 | 3300 ± 51 | 2.6 ± 0.1 | 6.0 ± 0.1 | 0.22 ± 0.01 | 0.27 ± 0.01 |
| LP 395-8 | 3600 ± 100 | 3300 ± 100 | 15.0 ± 0.1 | 18.1 ± 0.1 | 0.14 ± 0.01 | 0.11 ± 0.01 |
| GJ 810A | 3400 ± 100 | 3300 ± 100 | 4.3 ± 0.1 | 4.9 ± 0.1 | 0.61 ± 0.01 | 0.47 ± 0.01 |
Notes. Uncertainties indicate the step size used in the grid of models.
(a)
Real templates are used instead of synthetic. Effective temperatures from Passegger et al. (2018).
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