We present a summary of the measurements of mass sensitive parameters at the highest cosmic ray energies done by several experiments. The X sub(max) distribution as a function of energy has been measured with fluorescence telescopes by the HiRes, TA and Auger experiments and with Cherenkov light detectors by Yakutsk. The left angle bracketX sub(max)right angle bracket or the average mass ( left angle bracketInAright angle bracket ) has been also inferred using ground detectors, such as muon and water Cherenkov detectors. We discuss the different data analyses elaborated by each collaboration in order to extract the relevant Information. Special attention is given to the different approaches used in the analysis of the data measured by fluorescence detectors in order to take into account detector biases. We present a careful analysis of the stability and performance of each analysis. The results of the different experiments will be compared