SED of HIP 92043. Optical, near infrared and LABOCA 870 μm point in black, the Spitzer IRS spectrum in blue, Herschel fluxes in red. Uncertainties are 1-σ and may be smaller than the data point. The stellar photosphere is denoted by a dotted line. The solid black line denotes the sum of the stellar photosphere and a pair of black bodies (70 and 30 K, dashed lines). The solid grey lines denote the effect on the SED of altering the cold component temperature by ±10 K.