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We are conducting a large spectroscopic survey of over 130 Southern ZZ Cetiswith the Goodman Spectrograph on the SOAR Telescope. Because it employs asingle instrument with high UV throughput, this survey will both improve thesignal-to-noise of the sample of SDSS ZZ Cetis and provide a uniform datasetfor model comparison. We are paying special attention to systematics in thespectral fitting and quantify three of those systematics here. We show thatrelative positions in the $\log{g}$-$T_{\rm eff}$ plane are consistent forthese three systematics.

Understanding Systematics in ZZ Ceti Model Fitting to Enable Differential Seismology