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Table 1.

Spectral lines and their associated atomic parameters for the three spectral ranges considered.

Spectral range Δλ nλ λ0 elow eupp log10gf Elow α
[nm] [mÅ] [Å] [eV]
630.2 20 55 Fe I 6301.501 5.0P2.0 5.0D2.0 −0.718 3.654 0.243 835.356
20 55 Fe I 6302.494 5.0P1.0 5.0D0.0 −1.236 3.686 0.239 850.930
1082.7 18 275 Si I 10827.091 3.0P2.0 3.0P2.0 0.239 4.953 0.231 729.807
1565.0 40 125 Fe I 15648.515 7.0D1.0 7.0D1.0 −0.669 5.426 0.229 974.195
40 125 Fe I 15662.018 5.0F5.0 5.0F4.0 0.19 5.83 0.240 1196.950

Notes. The first column provides the label used for each spectral region (which might include more than one spectral line). Regarding the symbols: Δλ is the pixel size in m Å; nλ is the number of wavelengths used for that spectral line; λ0 is the central wavelength for the electronic transition associated with the spectral line; elow and eupp are the electronic configurations of the lower and upper energy level, respectively; and Elow is the excitation potential (in eV) of the lower energy level. These atomic data are adopted from Nave et al. (1994). The α and 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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