We show that the late time Price’s power-law tail for perturbations of Schwarzschild, $t^{-2\ell -3}$ as $t\to \infty$, with $\ell$ the orbital quantum number, can be obtained from a sum of Schwarzschild–de Sitter quasinormal modes in the limit of vanishing cosmological constant, $\mathrm{\Lambda }\to 0^{+}$.

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• Classical black holes