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Fig. 7


Variations in postfit residuals obtained for different values of PPN β (x-axis) and γ (y-axis). Panels a) and c) are obtained by considering the variations in the whole data sets when for panels b) and d), variations in the Mercury flyby data (from Mariner and MESSENGER missions) are excluded from the analysis. The dashed line indicates the limit in γ given by Bertotti et al. (2003).

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