Fig. 6.

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Burstiness parameter κs vs. deviation from the local De-Looze relation Δ, color-coded by the C III] surface brightness ΣC III]. Galaxies detected both in [C II] and C III] emission are annotated and represented as filled circles. Galaxies at 6 < z < 9 from Vallini et al. (2021) are represented as gray stars. Linear fit on the detected sources is shown as a blue line with 1σ uncertainties as a shaded region.
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