Observed spectral energy distribution of TMR-1C (filled black circles, based on Table 1 and on values reported in T98; filled black circles with downward-heading arrows indicate upper 3σ flux limits). The black solid line represents the spectral energy distribution of a NEXTGen stellar model source (Hauschildt et al. 1999) with T_eff = 4000   K, log    g = 5.0 and extincted by A_V = 23.0 mag. The shaded band indicates the range in flux distribution expected for objects of 3–7 M_Jup at the age of 1 Myr and seen behind A_V = 10–22 mag of extinction, which are consistent overall with the observed SED of TMR-1C for λ < 2.5   μm.