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The depth of maximum shower development and its fluctuations: cosmic ray mass composition at <i>E</i><sub>0</sub>≥10<sup>17</sup> eV
We present new data on Cherenkov light observations obtained during the period 1994-2009, after a modernization of the Yakutsk EAS array.A complex analysis of xmax and its fluctuations σ(xmax) was performed over a wide energy range.With the new data, according to QGSJet II model, an estimation was made of the …