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The Kr 3d correlation satellites have been studied experimentally by using linearly polarized synchrotron radiation and the gas-phase end-station of the FinEstBeAMS beamline to record polarization dependent photoelectron spectra. An analysis of these spectra has allowed the photoelectron anisotropy parameters characterizing the angular distributions, and the intensity branching ratios, related to the photoionization partial cross sections, to be evaluated. The correlation satellites have also been studied theoretically by employing the R-matrix method to calculate photoionization partial cross sections and photoelectron angular distributions.