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\subsection{Archival Data}  In addition to the new data taken with FLAMES, we also used archival HI data from the GASS survey \cite{Kalberla_2010}. GASS is a survey of Galactic HI taken with the Parkes antenna, with a beam size of 16$^\prime$, a spectral resolution of 1 km/s, and an rms noise of 57 mK. These data allow us to map out the structure of Complex WD on the sky, and compare the spectrum of the HI emission to Ca II H \& K absorption along the line of sight. We present in Figure \ref{fig:WD} an image of Complex WD from GASS, along with the positions of clouds noted found  in the \citet{1991A&A...250..509W} catalog, and the line-of-sight toward USNO-A0600-15865535.