Spectral energy distribution of J0855–0714 (red symbols) is compared with various planetary atmosphere models (gray lines) of Morley et al. (2014), all of which are computed for a 50% cloudy atmosphere. Arrows indicate upper limits. The observing filters are labeled. The models in the left and right columns are calculated for log g = 5.0 and 4.0 (cm s^-2), respectively. The blue triangles represent the theoretical flux densities as integrated from the models using the corresponding filter passbands. All models are normalized to the emission of J0855–0714 at W2.