GRB 190114C in the nuclear region of an interacting galaxy - A detailed host analysis using ALMA, the HST, and the VLT

Free Access

Table 4.

Emission lines, identified in the X-shooter spectrum, and their measured fluxes corrected for Galactic extinction only.

Line	F_λ
	[10⁻¹⁷ erg cm⁻² s⁻¹]
[O II] 3726	12.6 ± 0.3
[O II] 3729	16.2 ± 0.3
[Ne III] ^(a)	2.9 ± 0.4
Hγ ^(b)	4.3 ± 0.3
Hβ ^(b)	14.5 ± 0.3
[O III] 4959 ^(a)	12.8 ± 0.3
[O III] 5007 ^(a)	38.8 ± 0.3
He I 5876	2.9 ± 0.5
[O I] 6300	2.3 ± 0.3
Hα	89.7 ± 0.8
[N II] 6583	14.8 ± 0.6
[S II] 6717	8.9 ± 0.3
[S II] 6733	7.1 ± 0.3
[S III] 9071 ^(a)	10.9 ± 0.5
He I 10833	11.2 ± 0.5
Paγ ^(c)	4.9 ± 0.5

Notes. We did not correct for host extinction here because of the uncertainty in deriving the extinction (see text).

^(a)

Fluxes obtained by simple integration,

^(b)

The line is affected by line-of-sight absorption in the afterglow continuum, fluxes are obtained by fitting a single Gaussian to the emission part.

^(c)

The line suffers from residual sky emission, the flux is obtained by using the unaffected blue wing of the line and approximating it with a Gaussian with a fixed centre.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.