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Mapping the Quasar Main Sequence in the UV range: A Connection with the UV Fe III Emission
The quasar main sequence (MS) provides a consistent unification scheme for type I AGNs. This framework, constructed from the relative flux between the optical emissions $\mathrm{H}β$ and $\mathrm{Fe\,II\,(\lambda4570)}$, and the $\mathrm{FWHM(Hβ)}$, organizes quasars into two populations (B, A) and
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