Notes. The stars are listed in order of increasing TIC (TESS Input Catalogue) number (Col. 1), with another ID (preferably the HD number) given in Col. 2 and the V magnitude in Col. 3. The Heliocentric Julian Date (HJD) of mid-observation, the instrument with which it was obtained (F = FEROS; H = HARPS; N = HARPS-N; S = SALT-HRS; U = UVES), and the resulting S/N appear in Cols. 4 to 6. The values of T_eff in Col. 7 are from the TIC (they are listed as published there even though effective temperatures cannot be determined with 1 K precision). The following columns contain the results of our measurements: the stellar radial velocity v_r and its uncertainty σ(v_r) (Cols. 8 and 9; the entries were left blank when these values could not be determined); the mean magnetic field modulus ⟨B⟩, its uncertainty σ(⟨B⟩), and the number N_g of Gaussians fitted to the Fe II λ 6149.2 Å line for its determination (Cols. 10 to 12); the mean quadratic magnetic field ⟨B_q⟩, its formal uncertainty σ(⟨B_q⟩), and the number N_l of diagnostic lines from which it was derived (Cols. 13 to 15); the upper limit (v sin i)_max of the projected equatorial velocity and the formal uncertainty σ(v sin i) of the v sin i determination (Cols. 16 and 17). The values of the radial velocity and of the projected equatorial velocity are derived from analysis of the same sample of N_l lines as used for the ⟨B_q⟩ determination. For spectra in which the Fe II λ 6149.2 Å line is not resolved into its magnetically split components, the entries in Cols. 8 to 10 are left blank; a dash (‘–’) in Col. 11 identifies those spectra in which the mean quadratic magnetic field is below the detection threshold, and in Col. 14, those spectra in which the rotational Doppler broadening is below the detection threshold. (For TIC 93522454, the ⟨B_q⟩ value derived from the first UVES spectrum was given as it is only marginally below the formal detection threshold and as significant values of similar order were determined from the other UVES observations of this star.)