Kinematically consistent decomposition shows [O II] in quasars is dominated by star formation rather than AGN, allowing its use as a reliable SFR tracer that correlates tightly with bolometric luminosity over black hole mass or Eddington ratio.
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Tracing Star Formation in Quasar Hosts via [O II] $\lambda$3727: A Kinematically Consistent Approach
Kinematically consistent decomposition shows [O II] in quasars is dominated by star formation rather than AGN, allowing its use as a reliable SFR tracer that correlates tightly with bolometric luminosity over black hole mass or Eddington ratio.