For , the truncated Perron formula and a contour shift give the displayed form of the Riemann–von Mangoldt explicit formula. The pole at one contributes and the Nontrivial zeros of the Riemann zeta function contribute the finite sum. One can choose a separated height in and then restore using the local zero count for the Riemann zeta function. The error absorbs the half-weight discrepancy at a prime power. Outside this range of , one needs the fuller error with the near-integer terms retained.
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