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Quasi-periodic pulsations (QPPs) in solar flares have been widely observed, and can be used as a coronal plasma diagnostics tool. A total of 181 GOES class solar flares have been identified from a single active region (best known as NOAA 12192), which can be tracked for at least three Carrington rotations. Many of these flares show evidence of quasi-periodic pulsations, and a total of 30 flares have QPPs that can be detected in the power spectrum using a highly robust method that takes full account of red noise and data uncertainties. A statistical study is being undertaken using X-ray and microwave observations from GOES, SDO/EVE, Fermi, Vernov, and Nobeyama Radioheliograph. The aim of this investigation is to determine whether there is any relationship between the QPP periods and the flare or active region properties.