Final spectral energy distribution of the directly imaged exoplanet 51 Eri b. The new K1 and K2 GPI spectra along with the updated LP and new MS photometry are shown with red squares. The GPI J and H spectra, updated to account for the revised stellar flux, from the discovery paper (Macintosh et al. 2015), are plotted with blue circles. The filter extent is shown with the horizontal line over each band. To reduce crowding in the spectra, the errors for one out of every two data points are plotted. The data used to create this figure are available.