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Table 1

Parameters of the five N I lines used in the abundance analysis.

Line label λair ∕nm Lower χlow ∕eV Upper χup ∕eV log gf log(γrad.∕s−1) αH
N I 744 744.229 3s 4P3∕2 10.330 11.996 − 0.403 + 8.751 530 0.2271
lN I 822 821.633 3s 4P5∕2 10.336 11.844 + 0.138 + 8.745 497 0.2286
N I 863 862.923 3s 2P3∕2 10.690 12.126 + 0.077 + 8.713 576 0.2337
N I 868 868.340 3s 4P3∕2 10.330 11.758 + 0.106 + 8.740 481 0.2306
N I 1011 1010.89 11.753 3d 4F5∕2 12.979 + 0.444 + 7.773 750 0.2671

Notes. The table lists: wavelengths in air λair; electronic configurations and spectroscopic terms of the lower and upper states, with excitation energies χlow and χup ; oscillator strengths f; natural broadening coefficients γrad. (FWHM in angular frequency units); and ABO broadening cross-sections σH at reference velocity v = 104 m s−1 and exponents αH, such that the cross-section is proportional to vα (Anstee & O’Mara 1995). Data sources are the same as used to construct the non-LTE model atom (Sect. 2.4); in particular, the transition probabilities were drawn from Tachiev & Froese Fischer (2002).

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