Fig. 4.

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Measured C III]/He II versus C III]/C IV ratios for GN-z11 shown along with predictions from photoionisation due to AGN (circles) and star formation (stars) from Feltre et al. (2016) and Gutkin et al. (2016) in the range of Z/Z⊙ = 0.066 − 0.131 and gas densities in the range log10(nH)/cm−3 = 2 − 4. Based on the observed line ratios, neither photoionisation from AGN nor star formation alone can conclusively explain the observations, placing GN-z11 right between the model predictions from the two.
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