Table 7.
Properties of the interstellar medium in the host galaxy.
| Transition | EWr | Flux |
|---|---|---|
| (Å) | (10−18 erg cm−2 s−1) | |
| Absorption lines | ||
| Mn IIλ 2594 | 0.18 ± 0.13 | … |
| (< 0.39) | ||
| Fe IIλ 2600 | 0.07 ± 0.13 | … |
| (< 0.39) | ||
| Mn IIλ 2606 | −0.12 ± 0.15 | … |
| (< 0.45) | ||
| Mg IIλ 2796 | 0.51 ± 0.04 | … |
| Mg IIλ 2804 | 0.46 ± 0.04 | … |
| Mg Iλ 2852 | 0.14 ± 0.04 | … |
| (< 0.16) | ||
| Ca IIλ 3934 | 0.03 ± 0.01 | … |
| Ca IIλ 3969 | 0.01 ± 0.01 | … |
| (< 0.03) | ||
| Emission lines | ||
| Hβ | … | 3.68 ± 0.78 |
| [O III] λ 4363 | … | 0.25 ± 0.16 |
| … | (< 0.48) | |
| [O III] λ 4959 | … | 1.96 ± 0.81 |
| … | (< 2.43) | |
| [O III] λ 5007 | … | 12.96 ± 1.11 |
| Hα | … | 10.43 ± 0.76 |
| [N II] λ 6584 | … | 0.12 ± 0.54 |
| … | (< 1.62) | |
Notes. We report rest-frame equivalent widths EWr for absorption lines and fluxes for emission lines. For lines detected with a significance of < 3σ, we also report the < 3σ upper limits. The rest-frame equivalent widths are measured by averaging the measurements from the X-shooter spectra between tmax+32.7 days and tmax+94.3 days of each line species. The emission lines are measured from the FORS2 spectrum at tmax+637 days. The emission-line fluxes are not corrected for reddening.
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