We describe the analysis of longitudinal air shower profiles as measured by
the fluorescence detectors of the Pierre Auger Observatory and present the
measurement of the depth of maximum of extensive air showers, Xmax, with
energies >10^18 eV. The measured energy evolution of the average of Xmax and
its fluctuations are compared to air shower simulations for different primary
particles.Comment: to appear in the Proceedings of the International Symposium on the
Recent Progress of Ultra-high Energy Cosmic Ray Observation, Nagoya 201