Spectral energy distribution of HD 141011 and the infrared measurements from Spitzer (black line, gray shading for the uncertainty, and triangle for the upper limit). We overplot in colors the four SED models that are compatible with the mid-infrared excess, all with a minimum particle size of 1 μm. The plain lines represent the stellar photosphere and disk emission, while the dashed lines isolate the contribution of the disk alone. The inset is a zoom in the 10–40 μm range, highlighting the model mismatch between 15 and 25 μm.