Colour predictions including the effects of intergalactic
attenuation for a 600 Myr starburst (solid lines), a 3 Myr starburst
(long-dashed lines), a Type I QSO (dot-dashed lines) and a Type II
QSO with high equivalent width emission lines (dotted lines). In the
third and fifth rows, the B, V, i, z, J and H magnitudes
refer to the HST B435, V606, i775,
z850, J110 and H160 bands, respectively.
The fourth row magnitudes refer to the UKIDSS ZYJHK bands.