Open Access

Table 2

Properties of the synthetic line lists.

Name Instrument Nobs Mask λ⟩ (nm) ⟨geff Nlines
HD 63433 Neo-Narval 9 5500_4.5 447 1.23 3826
HD 63935 Neo-Narval 4 5500_4.5 447 1.23 3827
HD 63935 HARPSpol 4 5500_4.5 447 1.23 3682
HD 89345 Neo-Narval 5 5500_4.0 440 1.21 5167
HD 152843 Neo-Narval 3 6250_4.0 430 1.21 3401
HD 158259 Neo-Narval 3 5750_4.5 440 1.23 3309
HD 260655 SPIRou 1 4000_5.0 1680 1.25 2432
HAT-P-22 Neo-Narval 2 5500_4.5 447 1.23 3826
DS Tuc A HARPSpol 10 5500_4.5 447 1.23 3702
Kepler-444 Neo-Narval 4 5000_4.5 443 1.22 6046
K2-116 SPIRou 3 4500_4.5 1700 1.24 3868
TOI-836 SPIRou 1 4500_4.5 1700 1.24 3764
TOI-1136 Neo-Narval 6 5750_4.5 440 1.23 3311
TOI-1860 Neo-Narval 20 5750_4.5 440 1.23 3313
TOI-2076 Neo-Narval 6 5000_4.5 443 1.22 6046
Wolf 503 SPIRou 3 4500_4.5 1700 1.24 3905

Notes. The columns indicate: identifier of the star, instrument used for the observations, number of observations, properties of the line list in the form Teff (K)_logarithm surface gravity (cm s−1), number of lines used in LSD, average wavelength of the mask, and average effective Landé factor of the mask. The lower number of lines used for HARPSpol stems from the narrower wavelength coverage compared to Neo-Narval. For HD 63433, the values refer to the observations taken in 2024 (see also Table B.1).

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