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Table 2.

Emission lines of GRB host, GRB site and companion galaxy.

Line λrest GRB host Core+Bar GRB site Region 15 Region 17 Companion
O II 3726.032 15.49 ± 2.49
O II 3728.815 14.67 ± 1.51
Hβ 4861.333 328.16 ± 14.98 19.04 ± 0.25 2.88 ± 0.44 5.39 ± 0.09 3.77 ± 0.05 25.0 ± 13.1
O III 4958.911 77.54 ± 15.3 1.55 ± 0.38 0.81 ± 0.13 0.54 ± 0.06 17.5 ± 7.9
O III 5006.843 157.6 ± 10.1 3.90 ± 0.96 5.50 ± 0.67 2.21 ± 0.11 2.13 ± 0.06 34.8 ± 7.1
He I 5875.624 35.4 ± 1.9 1.73 ± 0.11 0.51 ± 0.04 0.38 ± 0.03
O I 6300.304 34.68 ± 4.04 1.31 ± 0.07 0.57 ± 0.06 0.40 ± 0.02
N II 6548.050 100.55 ± 20.93 6.98 ± 0.28 0.47 ± 0.26 1.74 ± 0.06 1.07 ± 0.04 3.39 ± 2.9
Hα 6562.819 906.93 ± 21.41 52.75 ± 0.29 7.97 ± 0.35 14.9 ± 0.06 10.44 ± 0.05 69.1 ± 5.5
N II 6583.460 333.90 ± 21.89 23.84 ± 0.30 1.65 ± 0.29 5.91 ± 0.06 3.69 ± 0.05 50.22 ± 9.8
S II 6716.440 204.56 ± 21.95 8.58 ± 0.28 1.86 ± 0.36 3.05 ± 0.06 1.95 ± 0.04 13.99 ± 4.1
S II 6730.810 146.18 ± 21.48 7.14 ± 0.29 1.38 ± 0.39 2.19 ± 0.06 1.42 ± 0.04 19.53 ± 4.5
Ar III 7135.790 6.66 ± 1.29 0.82 ± 0.11 1.17 ± 0.20 2.25 ± 0.54 0.22 ± 0.02

Notes. The GRB host and HII regions were measured from integrated spectra extracted from the MUSE cube, values at the GRB site were obtained from the late time X-shooter spectrum, the spectrum of the companion was obtained from separate PMAS/CAHA observations of the galaxy. The values in “GRB site” refer to the values from the X-shooter spectrum. In the MUSE data, the [O II]λ3727,29 is out of range. Fluxes in units of 10−16 erg s−1 cm−2 and are corrected for Galactic and intrinsic extinction using the Balmer decrement.

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