Fig. 5
Ratios r010 computed for KIC 6106415 (left) and KIC 12258514 (right) using the mode frequencies extracted from the Kepler oscillation spectra (see text). The colored dashed lines correspond to 2nd-order polynomial fits to the observed ratios using either the raw covariance matrix (gray lines) or the covariance matrix modified through truncated SVD (see Sect. 3.3).
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