  We study the relationship between signatures of high redshift ionization in
large-angle CMB polarization power spectra and features in the Planck 2015
data. Using a principal component (PC) ionization basis that is complete to the
cosmic variance limit out to $z_{\rm max}=30,40,50$, we find a robust $>95\%$
CL preference for ionization at $z>15$ with no preference for $z>40$. This
robustness originates from the $\ell \sim 10$ region of the data which show
high power relative to $\ell \le 8$ and result in a poor fit to a steplike
model of reionization. Instead by allowing for high redshift reionization, the
PCs provide a better fit by $2\Delta \mathrm{ln}\mathcal{L} = 5-6$. Due to a
degeneracy in the ionization redshift response, this improved fit is due to a
single aspect of the model: the ability to accommodate $z>10$ component to the
ionization as we illustrate with a two-step reionization model. For this and
other models that accommodate such a component, its presence is allowed and
even favored; for models that do not, their poor fit reflects statistical or
systematic fluctuations. These possibilities produce very different and
testable predictions at $\ell \sim 15-20$, as well as small but detectable
differences at $\ell>30$ that can further restrict the high redshift limit of
reionization.
