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Fig. 1.

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Example of UV spectrum together with the best fit (yellow line) and the various spectral components. The QSFit code assumes, for calculating luminosities, a standard ΛCDM cosmology with H0 = 70 km s−1 Mpc−1, ΩM = 0.3, and ΩΛ = 0.7 (Calderone et al. 2017).
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