Galaxy evolution in the Deep fields using photometric redshifts
D. Le Borgne, B. Rocca-Volmerange, V. de Lapparent, R. Carlberg, H. Courtois, T. Sousbie.

We show the potential of using photometric redshifts to study galaxy evolution in the Deep fields. Estimates of the redshift distributions in these fields will be presented, and the importance of the choice of templates will be discussed.