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The Sloan Digital Sky Survey Reverberation Mapping Project : biases in z > 1 46 redshifts due to quasar diversity

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Figure

Figure 1. Distribution of redshifts and ipsf magnitudes for the sample of 482 z>1.46 SDSS-RM quasars
Figure 2. Examples of spectra for each of the six redshift quality categories described in Sectioncategory is given in the top right corner of each panel
Figure 3. The leftblack curve is a simple linear least-squaresP (middle) panel shows redshift differences between our He II redshifts and those determined for He II ([O II]) from an independent analysis usingREPSPEC
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