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Table 1

Measurements for the resonance emission lines seen in the Subaru spectrum of V4332 Sgr.

λlab (air) λ obs Ion V h FWHM a FWHM a Flux Flux cleanb EW
[Å] [Å] [km s-1] [Å] [km s-1] [erg s-1 cm-2] [erg s-1 cm-2] [Å]

5889.950 5888.82 ± 0.14 Na i D2 –57.5 ± 7.2 2.72 ± 0.05 138.5 (1.81 ± 0.01)e–15c (2.21 ± 0.06)e–15c
5895.924 5894.77 ± 0.07 Na i D1 –58.7 ± 3.6 2.68 ± 0.06 136.3 (2.00 ± 0.01)e–15c (2.22 ± 0.07)e–15c
6572.779 6571.12 ± 0.02 Ca i –75.7 ± 0.7 1.21 ± 0.13 55.2 (7.34 ± 0.43)e–16 9.5 ± 1.3
7664.911 7663.13 ± 0.03 K i –69.7 ± 1.1 3.54 ± 0.02 138.5 (5.73 ± 0.02)e–14 (6.00 ± 0.02)e–14d 285.4 ± 33.1
7698.974 7697.22 ± 0.01 K i –68.3 ± 2.9 3.36 ± 0.04 130.9 (4.89 ± 0.01)e–14d (4.83 ± 0.02)e–14d 267.2 ± 17.7
7800.268 7798.52 ± 0.01 Rb i –67.2 ± 0.2 1.58 ± 0.31 60.7 (1.49 ± 0.08)e–15 6.0 ± 0.6
7947.603 7945.98 ± 0.03 Rb i –61.2 ± 1.3 1.01 ± 0.08d 38.1e (3.54 ± 0.13)e–16e 0.85 ± 0.1e

Notes.

(a)

From a fit of a Lorentzian profile; full width at half-maximum is not corrected for the instrumental profile (FWHM ≈ 0.15 Å);

(b)

integrated flux with interstellar and strongest telluric features removed from the profile;

(c)

results from a deblending procedure with a double Lorentzian profile; simple integral for both doublet lines gives summary flux of (3.26 ± 0.06)e–15 erg s-1 cm-2 and cleaned flux of (3.48 ± 0.06)e–15 erg s-1 cm-2;

(d)

line blends with a TiO band; width and flux measurements uncertain.

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