Spectral energy distribution of both HR 2562 B (blue dots) and VHS 1256 b (red line and dot). The vertical lines highlight the J and F1065C bands for comparison purposes (see main text). The fluxes were normalized at 10 pc. The filled red area and errorbars correspond to 1−σ uncertainties. The error bars of the first and last points in the Y-, J-, H-, and K-bands of HR 2562 B IFS data were set to zero for aesthetic purposes. The dark red dots are the synthetic MIRI photometry of VHS 1256 b.