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Discovery of the Most Distant Double Peaked Emitter at z=1 369

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Figure

Figure 1. Rest-frame NUV spectrum of J0331–2755 showing the double-peaked Mg ii line. The vertical dash-dotted line indicates the expected position of Mg ii λ2799
Figure 2. (a) Radio 1.4 GHz, (b) IR 5.8 μm, (c) optical R-band, and (d) X-ray 0.5–8 keV images of J0331–2755
Figure 4. X-ray spectrum of J0331–2755 overlaid with the best-fit model. The bottom panel shows the deviation of the data from the model in units of σ , with error bars of size unity
Figure 5. Redshift–luminosity distribution of double-peaked emitters (adapted from Strateva et al

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