The Sloan Digital Sky Survey Reverberation Mapping Project: Biases in
  z>1.46 Redshifts due to Quasar Diversity
  We use the coadded spectra of 32 epochs of Sloan Digital Sky Survey (SDSS)
Reverberation Mapping Project observations of 482 quasars with z>1.46 to
highlight systematic biases in the SDSS- and BOSS-pipeline redshifts due to the
natural diversity of quasar properties. We investigate the characteristics of
this bias by comparing the BOSS-pipeline redshifts to an estimate from the
centroid of HeII 1640. HeII has a low equivalent width but is often
well-defined in high-S/N spectra, does not suffer from self-absorption, and has
a narrow component that, when present (the case for about half of our sources),
produces a redshift estimate that, on average, is consistent with that
determined from [OII] to within 1-sigma of the quadrature sum of the HeII and
[OII] centroid measurement uncertainties. The large redshift differences of
~1000 km/s, on average, between the BOSS-pipeline and HeII-centroid redshifts
suggest there are significant biases in a portion of BOSS quasar redshift
measurements. Adopting the HeII-based redshifts shows that CIV does not exhibit
a ubiquitous blueshift for all quasars, given the precision probed by our
measurements. Instead, we find a distribution of CIV centroid blueshifts across
our sample, with a dynamic range that (i) is wider than that previously
reported for this line, and (ii) spans CIV centroids from those consistent with
the systemic redshift to those with significant blueshifts of thousands of
kilometers per second. These results have significant implications for
measurement and use of high-redshift quasar properties and redshifts and
studies based thereon.
