Fig. 1

Comparison of black hole mass (MBH) estimates (left panel) and bolometric luminosity (Lbol) estimates (right panel) for a set of QSOs that have at least two spectra from different datasets. The estimate from the primary dataset is plotted on the x-axis and the estimate from the secondary dataset is plotted on the y-axis, where the hierarchy is based on preferences outlined in Sect. 4. The color of the solid core circle identifies the primary dataset, which is either SDSS (blue), zCOSMOS-Deep (purple), or zCOSMOS-Bright (red). The color of the outer circle identifies the secondary dataset, which may be zCOSMOS-Bright (red) or IMACS (green). The Lbol estimates, derived from direct measurements of the local continuum from the spectra, are very consistent between datasets. The MBH estimates show more scatter and a small systematic variation about the 1:1 line.
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