CHORIZOS mode SED. Blue error bars are used for the input photometry that was used for the fit (Gaia DR2 G + G_BP + G_RP, Johnson U + B + V, and 2MASS J + H + K_s) and red error bars for the discarded input photometry (WISE W1 + W2 + W3 + W4). In each case, the vertical error bar is the photometric uncertainty, and the horizontal error bar is a representation of the wavelength coverage of each filter. Green stars are used for the model photometry.