Photometric spectral energy distribution of HD 235088 (circles) from 0.3 through ~25 µm. A black-body source with a temperature of 5050 K (solid line) is added for the sole purpose of demonstrating that all fluxes are photospheric in origin and there are no infrared flux excesses at long wavelengths. Vertical error bars denote flux uncertainties and horizontal error bars account for the width of the photometric passbands.