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Table E.1

Weak and forbidden lines at visible wavelengths.

Species λ0 (a) υLSR Δυ (b) Sν,obs Sν,obsdν Sν,modeldν(c) Eu (d)
[Å] [km s−1] [km s−1] [Jy] [10−15 W m−2] [10−15 W m−2] [cm−1]
O I 5577.339 41.3(0.5) 20.7(1.1) 0.81(.04) 0.32(.05) 0.0017 33 793
O I 6300.304 43.4(0.2) 24.0(0.5) 5.25(.08) 2.13(.05) 0.36 15 868
O I 6363.776 41.9(0.3) 20.2(0.6) 2.02(.05) 0.68(.03) 0.12 15 868
Ca II 7291.469 41.5(0.2) 14.7(0.4) 23.40(.40) 5.03(.17) 6.6 13 711
Ca II 7323.887 41.4(0.1) 17.5(0.2) 18.90(.20) 4.79(.07) 5.0 13 650
Fe II 7452.561 41.4(0.4) 15.2(0.8) 1.47(.07) 0.32(.02) 0.049 15 845
Fe I 7723.207 41.4(0.7) 12.7(1.6) 0.60(.07) 0.11(.02) 5.1 31 323
C I 8727.126 43.1(0.2) 16.3(0.4) 6.50(.13) 1.29(.04) <0.001 21 648
C I 9850.250 39.8(0.8) 21.0(1.9) 0.96(.07) 0.22(.01) <0.001 10 193

Notes. (a) Wavelength in standard air. (b) FWHM of the Gaussian fit to the line profile. (c)Integrated flux in the reference model, corrected for extinction at AV = 0.99 magnitudes (estimated by comparing the observed flux density at 730 nm with a Kurucz’s Atlas 9 grid model for log g = 1.5 and Teff = 8500 K at a distance of 1 kpc). (d)Energy of the upperstate of the transition. References: entries in Col. 2 come from the NIST Atomic Spectroscopy Database. The numbers in parentheses (…) are the root-mean-square uncertainties derived from the Gaussian fits.

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