Broadband spectra computed for the suite of GRMHD simulations listed in Table 1. Each column corresponds to a different simulation, while each row shows the effect of varying one of the model parameters. The data points in the first column correspond to various observations of Sgr A*. The top “Fiducial” row uses parameters i = 60°, n_e = 3.2 × 10⁸, β_threshold = 0.2, θ_disk = 0.01, and T_{e, funnel} = 10. In each panel, the shaded gray area marks the variability of spectra computed from 100 snapshots; the black solid curve marks their average; the red dotted curve marks the average spectrum of the inner accretion flow; the green dotted curve marks the average spectrum computed after extrapolating the properties of the flow out to the Bondi radius; and the blue dashed curve marks the spectrum of the mean flow. We vary the normalization of the electron density n_e in the second row, the observer's inclination i in the third row, the threshold plasma-β in the fourth row, and the electron–ion temperature ratio θ_disk in the disk in the fifth row. In the sixth row, we either vary the funnel electron temperature T_{e, funnel} (solid curves) or the funnel electron–ion temperature ratio θ_funnel (dashed curves).