Table 5
Calibrated emission-line fluxes (see Fig. 9).
Slit | Wavelength | Ion | Fobs | Fcorr | EW |
(Å) | (Å) | ||||
|
|||||
PA = 253° (B600) | 3727 | [O ii] | 22.21 ± 0.34 | 25.61 ± 0.30 | 25.35 ± 0.86 |
4861 | Hβ | 11.83 ± 0.67 | 12.63 ± 0.49 | 14.91 ± 0.59 | |
4959 | [O iii] | 1.96 ± 0.21 | 2.22 ± 0.19 | 2.49 ± 0.22 | |
5007 | [O iii] | 5.91 ± 0.50 | 6.62 ± 0.64 | 7.42 ± 0.75 | |
|
|||||
PA = 113° (R400) | 4861 | Hβ | 13.25 ± 0.13 | 266.06 ± 2.50 | 1.44 ± 0.17 |
6548 | [N ii] | 17.87 ± 0.29 | 111.11 ± 2.61 | 2.49 ± 0.78 | |
6563 | Hα | 126.04 ± 1.64 | 776.18 ± 13.08 | 18.06 ± 0.25 | |
6583 | [N ii] | 54.35 ± 0.60 | 330.07 ± 4.99 | 7.44 ± 0.41 | |
6716 | [S ii] | 36.58 ± 0.67 | 203.25 ± 2.01 | 5.06 ± 0.43 | |
6731 | [S ii] | 28.09 ± 0.77 | 142.09 ± 1.17 | 3.54 ± 0.26 | |
|
|||||
PA = 253° (R400) | 4861 | Hβ | 16.82 ± 0.34 | 71.44 ± 1.44 | 15.07 ± 1.01 |
4959 | [O iii] | 3.49 ± 0.47 | 14.37 ± 0.27 | 4.08 ± 0.27 | |
5007 | [O iii] | 10.34 ± 0.24 | 42.08 ± 0.99 | 10.87 ± 0.85 | |
6300 | [O i] | 2.43 ± 0.97 | 5.28 ± 0.98 | 2.55 ± 0.48 | |
6548 | [N ii] | 10.26 ± 0.82 | 26.53 ± 1.15 | 4.01 ± 1.44 | |
6563 | Hα | 73.48 ± 1.58 | 208.12 ± 4.58 | 108.02 ± 3.13 | |
6583 | [N ii] | 30.31 ± 0.54 | 77.65 ± 1.60 | 38.89 ± 1.18 | |
6716 | [S ii] | 16.60 ± 0.21 | 43.07 ± 0.87 | 25.67 ± 0.66 | |
6731 | [S ii] | 10.81 ± 0.14 | 26.23 ± 0.64 | 15.73 ± 0.44 |
Notes. PA – Position Angle, EW – Equivalent Width. Reddening-corrected flux in units of 10-16 ergs cm-2 s-1 Å-1. Due to the fact that Hα/Hβ ratio could not be evaluated for the PA = 253° (B600), we use a galactic extinction of E(B − V) = 0.027 for this spectrum (Schlegel et al. 1998).
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