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A total of 107 glitches were identified in 36 pulsars, where 61 have previously been reported and 46 are new discoveries. Glitch parameters were measured by fitting the timing residual data. Observed relative glitch sizes \\Delta\\nu_g/\\nu range between 10^-10 and 10^-5, where \\nu = 1/P is the pulse frequency. We confirm that the distribution of \\Delta\\nu_g/\\nu is bimodal with peaks at approximately 10^-9 and 10^-6. 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