Fig. 3. Influence of the different cosmologies on multi-wavelength redshift distributions of galaxies. Coding for the lines is the same as in Fig. 1. Data are from Crampton et al. (1995) (Canada-France Redshift Survey), and Ashby et al. (1996) (North Ecliptic Pole region). The predicted curves in the I band and at 60 µm have been renormalised to the total number of galaxies in the data.