Table A.2.
Line fluxes for the sources and regions in the FoV1
| Sp | OII-R100 | OII-R2700 | Hβ-R100 | Hβ-R2700 | OIII-R100 | OIII-R2700 | Hα-R100 | Hα-R2700 | NII-R100 | NII-R2700 |
|---|---|---|---|---|---|---|---|---|---|---|
| E | 8.71±0.48 | 8.52±0.43 | 4.50±0.17 | 4.46±0.24 | 15.49±0.19 | 14.48±0.28 | 21.03±0.33 | 18.59±0.56 | 5.54±0.27 | 4.52±0.48 |
| E1c | 8.08±0.56 | 8.91±0.56 | 4.65±0.19 | 4.77±0.29 | 15.46±0.22 | 14.47±0.34 | 22.91±0.52 | 18.57±0.71 | 5.24±0.43 | 4.12±0.61 |
| Eext | 10.04±0.56 | 10.77±0.83 | 15.38±1.512 | 13.82±2.34 | 0.14±2.64 | |||||
| ES | 1.95±0.18 | 1.51±0.17 | 0.70±0.08 | 0.70±0.08 | 2.00±0.09 | 1.98±0.09 | 3.88±0.11 | 3.09±0.25 | 0.98±0.09 | 1.25±0.23 |
| EN | 4.74±0.24 | 4.39±0.25 | 2.81±0.10 | 2.42±0.14 | 10.26±0.11 | 9.14±0.16 | 11.88±0.20 | 10.49±0.32 | 3.33±0.17 | 1.85±0.27 |
| ENa | 1.15±0.07 | 1.41±0.11 | 0.73±0.04 | 0.86±0.07 | 2.93±0.05 | 2.95±0.08 | 3.02±0.05 | 3.34±0.20 | 0.81±0.04 | 0.88±0.19 |
| ENb | 1.86±0.12 | 1.35±0.10 | 1.00±0.05 | 0.87±0.05 | 3.47±0.05 | 3.10±0.06 | 4.06±0.10 | 3.39±0.12 | 1.21±0.08 | 0.56±0.10 |
| ENc | 0.40±0.05 | 0.35±0.07 | 0.20±0.04 | 0.14±0.03 | 0.91±0.04 | 0.69±0.03 | 0.99±0.05 | 0.76±0.06 | 0.22±0.04 | 0.16±0.05 |
| W 3 | 1.28±0.28 | 4.93±0.52 | 1.08±0.41 | |||||||
| W1c | 1.10±0.24 | 2.78±0.32 | 3.02±0.49 | 1.13±0.26 | 1.32±0.41 | |||||
| Wext | 2.12±0.66 | 7.35±0.64 | 6.00±0.74 | 5.77±0.78 | 3.01±0.68 | |||||
| C1 | 1.41±0.12 | 1.14±0.13 | 0.54±0.09 | 0.31±0.08 | 1.55±0.10 | 1.52±0.09 | 1.74±0.12 | 1.39±0.24 | 0.38±0.10 | < 0.876 |
| C2 | 0.54±0.10 | 0.47±0.11 | 0.31±0.07 | 1.59±0.09 | 1.27±0.06 | 1.07±0.122 | 0.88±0.13 | < 0.465 | ||
| C3 | 0.55±0.17 | 0.26±0.07 | 0.32±0.06 | 0.77±0.08 | 0.64±0.07 | 1.49±0.19 | 1.19±0.18 | 0.54±0.15 | ||
| L1 | 0.49±0.11 | 0.30±0.07 | 0.28±0.05 | 3.17±0.08 | 2.95±0.06 | 1.28±0.12 | 1.29±0.12 | < 0.429 | ||
| L2 | 0.64±0.06 | 0.40±0.04 | ||||||||
| L3 | 0.70±0.09 | 0.77±0.05 | 0.50±0.12 | 0.49±0.12 | ||||||
| L4 | (0.74±0.06)4 | (0.31±0.05)4 | 0.76±0.09 | 0.59±0.13 | 0.29±0.08 | |||||
| L5 | 0.71±0.10 | 0.41±0.05 | 3.16±0.12 | 2.56±0.06 | 1.89±0.232 | 1.55±0.11 | < 0.565 | |||
| L6 | 0.61±0.08 | 0.59±0.06 | 0.51±0.08 | 0.52±0.10 |
Notes. 1From the integrated spectra in the apertures defined in Fig. A.1, in units of 10−18 erg/s/cm−2. For E and W galaxies we also include values in apertures of 1 arcsec in diameter as in Álvarez-Márquez et al. (2023). No aperture corrections, nor 10 percent correction for R100 fluxes are applied. 2 The fit for the Hα -[NII] complex gives no flux for the [NII]lines. 3 For W, R100 Hβ flux is contaminated by the lens galaxy. For the Hα flux the R100 spectrum is preferred because the large velocity range covered by the aperture induces a significant increase of noise in the high resolution spectrum. 4 Difference between R100 and R2700 fluxes are larger than × 2, and not considered. The upper limits correspond to 3-σ the noise level.
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