Energy distribution of SAGE1CJ053634. The diamonds indicate photometric measurements with their 1σ error-bars. The arrows indicate the 3σ upper limits. The predominance of warm silicate emission and the lack of cooler material in SAGE1CJ053634 is evident. The dot-dashed line shows the best fitting clumpy torus model (Nenkova et al. 2008). The clumpy torus model reproduces the strength and band ratio of the silicate emission well. PAH emission can be identified, see also the residual (solid grey). The grey dotted line shows the possible contribution from an elliptical host galaxy. The thick grey line shows the sum of the clumpy torus model and host galaxy emission.