xA quasar line widths give a virial luminosity estimator L = L0 FWHM^4, but the evidence shown relies on fitted orientation corrections rather than an independent calibration.
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Quasar emission lines as virial luminosity estimators
xA quasar line widths give a virial luminosity estimator L = L0 FWHM^4, but the evidence shown relies on fitted orientation corrections rather than an independent calibration.