Fig. 2. Influence of the different cosmologies on the mid-IR/FIR/submm counts. Data are from Elbaz et al. (1999) (15 µm), Kawara et al. (1998) and Puget et al. (1999) (175 µm), Smail et al. (1997), Eales et al. (1999) and Barger et al. (1999a) (850µm). Coding for the lines is the same as in Fig. 1.