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Considering the limit $W, n\\to\\infty$, we prove that the behaviour of the second correlation function of such matrices in the bulk of the spectrum, as $W\\gg \\sqrt{N}$, is determined by the Wigner -- Dyson statistics. 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Considering the limit $W, n\\to\\infty$, we prove that the behaviour of the second correlation function of such matrices in the bulk of the spectrum, as $W\\gg \\sqrt{N}$, is determined by the Wigner -- Dyson statistics. 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