Table C.3
Emission line measurements of the host galaxy system of LSQ14mo in the observed frame.
| Position A | ||||||||||||
|
|
||||||||||||
| Line | λ (Å) | Flux | Error | rms | EW (Å) | Luminosity | ||||||
|
|
||||||||||||
| [ O ii ] | 3727 | 498 | 3 | 0.7 | 58 | 101 | ||||||
| [ Ne iii ] | 3868 | 39.2 | 3.5 | 1.2 | 4.6 | 7.9 | ||||||
| Hδ | 4102 | 23.1 | 2.3 | 0.8 | 2.7 | 4.7 | ||||||
| Hγ | 4340 | 53 | 2 | 0.6 | 3 | 11 | ||||||
| [ O iii ] | 4363 | 4.63 | 1.28 | 0.47 | 1.1 | 0.94 | ||||||
| Hβ | 4861 | 137 | 1 | 0.4 | 11 | 28 | ||||||
| [ O iii ] | 4959 | 121 | 1 | 0.3 | 12 | 25 | ||||||
| [ O iii ] | 5007 | 332 | 8 | 2.1 | 32 | 67 | ||||||
| [ O i ] | 6300 | 35 | 2 | 0.6 | 5 | 7 | ||||||
| [ N ii ] | 6548 | 11.6 | 1.6 | 0.6 | 1.7 | 2.4 | ||||||
| Hα | 6563 | 425 | 3 | 0.6 | 68 | 86 | ||||||
| [ N ii ] | 6583 | 48 | 2 | 0.6 | 8 | 10 | ||||||
| [ S ii ] | 6717 | 93 | 3 | 0.9 | 15 | 19 | ||||||
| [ S ii ] | 6731 | 60 | 3 | 0.9 | 10 | 12 | ||||||
|
|
||||||||||||
| Position B | ||||||||||||
|
|
||||||||||||
| Line | λ (Å) | Flux | Error | rms | EW (Å) | Luminosity | ||||||
|
|
||||||||||||
| [ O ii ] | 3727 | 74 | 0.8 | 0.13 | 90 | 15 | ||||||
| [ Ne iii ] | 3868 | 12 | 0.4 | 0.13 | 9 | 2.4 | ||||||
| Hδ | 4102 | 7.4 | 0.33 | 0.11 | 4 | 1.5 | ||||||
| Hγ | 4340 | 13 | 0.2 | 0.06 | 14 | 2.7 | ||||||
| [ O iii ] | 4363 | – | – | – | – | – | ||||||
| Hβ | 4861 | 31 | 0.4 | 0.08 | 40 | 6.3 | ||||||
| [ O iii ] | 4959 | 39 | 0.3 | 0.08 | 45 | 8.0 | ||||||
| [ O iii ] | 5007 | 119 | 3.5 | 0.49 | 144 | 24 | ||||||
| [ O i ] | 6300 | 6.1 | 0.63 | 0.20 | 11 | 1.2 | ||||||
| [ N ii ] | 6548 | – | – | – | – | – | ||||||
| Hα | 6563 | 80 | 1.1 | 0.13 | 219 | 16 | ||||||
| [ N ii ] | 6583 | 2.7 | 0.41 | 0.13 | 9 | 0.6 | ||||||
| [ S ii ] | 6717 | 7.8 | 0.79 | 0.21 | 23 | 1.6 | ||||||
| [ S ii ] | 6731 | 6.9 | 0.81 | 0.21 | 25 | 1.4 | ||||||
|
|
||||||||||||
| Position C | ||||||||||||
|
|
||||||||||||
| Line | λ (Å) | Flux | Error | rms | EW (Å) | Luminosity | ||||||
|
|
||||||||||||
| [ O ii ] | 3727 | 53 | 1.0 | 0.19 | 60 | 10.8 | ||||||
| [ Ne iii ] | 3868 | 8.8 | 0.54 | 0.15 | 9 | 1.8 | ||||||
| Hδ | 4102 | – | – | – – | – | |||||||
| Hγ | 4340 | 9.3 | 0.43 | 0.13 | 4 | 1.9 | ||||||
| [ O iii ] | 4363 | – | – | – – | – | |||||||
| Hβ | 4861 | 23 | 0.5 | 0.12 | 21 | 4.8 | ||||||
| [ O iii ] | 4959 | 26 | 0.7 | 0.18 | 23 | 5.2 | ||||||
| [O iii ] | 5007 | 77 | 6.2 | 1.11 | 70 | 15.7 | ||||||
| [O i ] | 6300 | – | – | – – | – | |||||||
| [ N ii ] | 6548 | – | – | – – | – | |||||||
| Hα | 6563 | 64 | 1.5 | 0.24 | 107 | 13.0 | ||||||
| [ N ii ] | 6583 | 3.7 | 0.83 | 0.24 | 8 | 0.7 | ||||||
| [ S ii ] | 6717 | 6.8 | 0.81 | 0.22 | 13 | 1.4 | ||||||
| [ S ii ] | 6731 | 5.0 | 0.80 | 0.22 | 11 | 1.0 | ||||||
Notes. The spectra have been corrected for Milky Way reddening corresponding to a dust extinction of AV = 0.20. We measured the emission line fluxes after subtracting the stellar continuum from the starlight spectral synthesis models. The error is derived by the Eq. (B.1). We fixed the FWHM widths at the values derived from the [ O iii ] λ4959 line, which correspond to the FORS2 resolution (9.05, 9.06, and 9.21 Å for positions A, B, and C, respectively). The relativity large rms and error of [ O iii ] λ5007 is due to a strong sky line nearby. For luminosity, we have not applied host galaxy dust reddening corrections. The internal host extinction at position A is AV = 0.26 derived by the intrinsic ratio of Hα and Hβ , and negligible at positions B and C. The unit of Flux, Error, rms of × 10-18 erg s-1 cm-2, Luminosity of × 1039 erg s-1.
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