Left: the NuSTAR (black) and Swift (red) spectra of Mrk 817. The spectra are fit with the model detailed in Table 1, and the corresponding data/model ratio is also shown. The disk reflection spectrum is typical in all aspects, and the low-energy absorption may be tied to a transient outflow like those seen in sources like NGC 5548 and NGC 3783. Right: The best-fit model for the NuSTAR (black) and Swift (red) spectra of Mrk 817, including low-energy absorption and relativistic disk reflection. The model is shown here without the data, to illustrate its features prior to convolution with the detector responses.