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Table 3.

Optical emission line ratios from NIRSpec integrated spectra.

Line ratio Integ. spec. (r = 0.5″) NE cone (r = 0.15″) SW cone (r = 0.15″)
tot sys out tot sys out tot sys out
log([O III]/Hβ) 0 . 66 0.02 + 0.01 $ 0.66_{-0.02}^{+0.01} $ 0 . 65 0.01 + 0.04 $ 0.65_{-0.01}^{+0.04} $ 0 . 96 0.10 0.07 $ 0.96_{-0.10}^{0.07} $ 0 . 96 0.02 + 0.03 $ 0.96_{-0.02}^{+0.03} $ 1 . 07 0.03 + 0.10 $ 1.07_{-0.03}^{+0.10} $ 0 . 82 0.03 + 0.09 $ 0.82_{-0.03}^{+0.09} $ 0.84 ± 0.1 1 . 01 0.03 + 0.09 $ 1.01_{-0.03}^{+0.09} $ 0 . 75 0.04 + 0.01 $ 0.75_{-0.04}^{+0.01} $
log([N II]/Hα) 0 . 57 0.03 + 0.16 $ -0.57_{-0.03}^{+0.16} $ 0 . 57 0.01 + 0.06 $ -0.57_{-0.01}^{+0.06} $ 0 . 11 0.21 + 0.35 $ -0.11_{-0.21}^{+0.35} $ 0 . 54 0.04 + 0.03 $ -0.54_{-0.04}^{+0.03} $ 0 . 45 0.17 + 0.08 $ -0.45_{-0.17}^{+0.08} $ −0.40 ± 0.1 −0.51 ± 0.01 0 . 84 0.05 0.24 $ -0.84_{-0.05}^{0.24} $ 0 . 32 0.02 + 0.04 $ -0.32_{-0.02}^{+0.04} $

Notes. Integrated spectrum emission lines from best-fit shown in Fig. 2; NE and SW cones from best-fit shown in Figs. B.1 and B.2, respectively.

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