The relationship between the emission line, continuum luminosity, and Baldwin effect in blazars - I. The case of the Mg II λ2798 Å emission line

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Fig. 6.

Left panel: Relationship between the 3000 Å continuum luminosity and the Mg II λ2798 Å emission line luminosity for the binned data of the FSRQ sample. Right panel: BE relationship for the binned data of the FSRQ sample. In both panels, the solid line represents the fit to the binned data.

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