  This is a short AAS Research Note on the analysis of new Chandra observations
of PG 1116+215, for which an extragalactic OVIII WHIM line was reported by
Bonamente et al. (2016). The new observations occurred at a time when the
source flux was three times lower, and the background was three times higher,
than in the earlier observations. The analysis described in this research note
show that the new observations are consistent with the old one at the
wavelengths of the OVIII WHIM line, and the lower signal-to-noise of the new
data did not permit a significant detection of the line in the new data.
