Comparison of the flux of the newly identified candidate (blue circles) with SEDs of different substellar objects of spectral types L3, L6, L9 (best fit), and T1. For each spectral type, we plot the object that provides the best fit according to the indicator. The inset plot at the top shows the values as a function of spectral type for ~400 objects taken from various libraries (Leggett et al. 2001; McLean et al. 2003; Cushing et al. 2005; Rayner et al. 2009). The vertical arrows indicate the spectral type of the plotted SEDs.