being heavily blended with $\lambda$6355. In addition, as was pointed out by @Maund07, the $\lambda$5876 feature has become more prominent and the red wing of its absorption now shows a notch due to D absorption.

Also, by this time the  H&K feature has developed a P-Cygni profile with quite a strong emission component. In addition, the near-IR triplet absorption has strengthened dramatically. The previously identified absorption from near 4300 Å and 5000 Å  becomes stronger, broader, and more complex with time. This is likely due to line blanketing which was also seen in SN 2002ap [@Foley03].

The broad absorption near 9000 Å could be $\lambda$9266 at about $-9000$ [km s$^{-1}$]{}. In addition, strong, relatively broad absorption from $\lambda$7774 is again seen in these observations, but at roughly $-8000$ [km s$^{-1}$]{}. However, this feature coincides with a telluric absorption band in the day 41 and 57 spectra, making the velocity determination difficult and uncertain.

Late-Time Spectra {#ss:late}
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A late-time spectrum from @Maund07 (256 days past explosion) and our late-time spectra (309 and 340 days past explosion) are presented in Figure \[f:late\_spec\] and are compared with similar late-time spectra of SNe 1993J and 2002ap. [SN 2001ig]{} has reached the nebular phase 