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Table 1.

Atomic parameters for spectral lines employed in our work.

Atom Ionization λ0 nλ Δλ elow eupp log10gf Elow α σ / a 0 2 $ \sigma/{a}_{0}^{2} $
[nm] [mÅ] [eV]
Fe I 617.334 15 35 5P1 5D0 −2.880 2.223 0.266 280.6
Ca II 854.209 17 100 2D5/2 2P3/2 −0.360 1.700 0.275 291.0

Notes. λ0 is the central wavelength for the electronic transition associated with the spectral line; nλ is the number of observed wavelengths for each spectral line; Δλ is the spectral sampling in mÅ; elow and eupp are the electronic configurations of the lower and upper energy level, respectively; Elow is the excitation potential (in eV) of the lower energy level. These atomic data are adopted from NIST (Kramida et al. 2023). In particular, Nave et al. (1994) is used for Fe and Edlén & Risberg (1956) for Ca. The α and σ / a 0 2 $ \sigma/{a}_{0}^{2} $ are the velocity exponent and collision cross-section parameters (in units of Bohr’s radius, a0), respectively, as defined in the Anstee, Barklem, and O’Mara collision theory for the broadening of metallic lines by neutral hydrogen collisions (Anstee & O’Mara 1995; Barklem & O’Mara 1997; Barklem et al. 1998).

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