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Fig. 15.

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Target and averaging kernel for the reference model, localized just above the near-core region, based on dipole oscillation modes with radial orders n = 1–60. The averaging kernels shows a single peak at the location of the target kernel. Some residual amplitude remains in the envelope of the star. The target kernel used is a modified Gaussian located at r = 0.18 and a width of 0.01.

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