Fig. 8.
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Combined photometric and spectroscopic spectral energy distribution of WISE1810. All OSIRIS, EMIR and Schneider et al. (2020) spectra are smoothed for the clarity of the figure. Photometric fluxes (red dots) correspond to, from blue to red wavelengths, the i, z, y, J, H, K, W1, W2, and W3 bands. Horizontal error bars stand for the effective width of the filters while vertical error bars account for the photometric uncertainties.
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