Red quasars are intrinsically X-ray weak with low alpha_OX values, tracing a distinct evolutionary stage of suppressed black hole accretion relative to stellar mass growth.
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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.
citing papers explorer
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SDSS-V: Revealing a weak accretion state in X-ray selected red quasars
Red quasars are intrinsically X-ray weak with low alpha_OX values, tracing a distinct evolutionary stage of suppressed black hole accretion relative to stellar mass growth.
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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.