Open Access

Table B.1.

Synthetic line lists associated to our stars and used with LSD.

Name Mask Nlines Nobs ⟨S/N⟩V vrange
[km s−1]
HD 1835 6000_4.5 6960 16 479 ±20
HD 28205 6000_4.5 6980 5 346 ...
HD 30495 6000_4.5 7270 3 505 ±20
HD 43162 5500_4.5 5340 11 298 ±16
5500_4.5 5340 8 359 ±16
HD 82443 5250_4.5 6180 9 441 ±20
HD 114710 6000_4.5 7250 12 1028 ±22
HD 149026 6000_4.0 4430 3 325 ...
HD 189733 5000_4.5 6615 8 350 ±17
HD 190406 6000_4.5 6960 8 497 ...
HD 206860 6000_4.5 7260 17 396 ±22
6000_4.5 7260 10 560 ±22
HD 219828 6000_4.0 4430 10 273 ...

Notes. The columns indicate: identifier of the star, properties of the line list in the form temperature[K]_logarithm surface gravity[cm s−1], number of lines used in LSD, number of observations, mean signal-to-noise ratio of the Stokes V LSD profile, velocity range centred on the radial velocity of the star encompassing both the absorption of the Stokes I LSD profiles and the lobes of Stokes V LSD profiles. When the Stokes V LSD profiles does not exhibit a clear Zeeman signature, the velocity range is not shown. For two stars, HD 43162 and HD 206860, we have two epochs so we list the values for each.

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