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Table 3.
Emission line properties of the SMG constrained by our best fit of the spectrum in Fig. 8 (extracted from an aperture radius of 0.3″).
| σ [km s−1] | Δv [km s−1]a | F[O III]λ 5007Å | FHα | F[N II]λ 6584Å | F[S II]λ 6717Å | F[S II]λ 6731Å | |
|---|---|---|---|---|---|---|---|
| Scenario 1: Outflow | |||||||
| Narrow 1 | 470 ± 20 | 111 ± 2 | – | 856 ± 3 | 1772 ± 2 | 445 ± 2 | 275 ± 2 |
| Narrow 2 | 300 ± 100 | −760 ± 90 | 1300 ± 30 | 417 ± 2 | 464 ± 3 | – | – |
| Outflow | 1300 ± 500 | −2450 ± 40 | 2480 ± 50 | – | 2142 ± 2 | – | – |
| Scenario 2: BLR | |||||||
| Narrow 1 | 470 ± 20 | 72 ± 2 | – | 855 ± 1 | 1771 ± 1 | 445 ± 1 | 275 ± 1 |
| Narrow 2 | 300 ± 100 | −760 ± 90 | 1300 ± 30 | 346 ± 1 | 373 ± 2 | – | – |
| Outflow | 1300 ± 500 | −2450 ± 40 | 2480 ± 50 | – | – | – | – |
| BLR | 1370 ± 50 | −1600 ± 400 | – | 3021 ± 5 | – | – | – |
Notes. Emission line intensities are in units of 10−20 erg s−1 cm−2. aRelative to z = 4.6891 (Carniani et al. 2013).
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