Top panel: SED of Swift J1745−26 from OIR to X-rays, for September 2012 (blue points) and March 2013 (green points) observations. The SED is built with data points de-reddened with A_V = 7.69. The result of the fit (plotted in black) is the sum of: multi-colour black body accretion disc (in red with R_in = 1600 ISCO for Sept. 2012, and in yellow with R_in = 2900 ISCO for March 2013, respectively), X-ray power law (blue for Sept. 2012 and pink for March 2013 resp.), and potentially stellar contribution (grey upper limit). Bottom panel: broad-band SED of Swift J1745−26 from radio to X-rays for September 2012 observations, including our best fit obtained by adjusting only infrared, optical to X-ray data points (with same colour coding and R_in = 1600 ISCO). For comprehensiveness, we also include radio data points reported in Tetarenko et al. (2015).