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This article has an erratum: [https://doi.org/10.1051/0004-6361/202243237e]


Fig. 5

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Mean parallax shift, in two-degree bins, versus ecliptic longitude in the solution with 14 million stars for a mission length of 10 yr. The blue curve is the running mean smoothed with a linear kernel of width 13. The theoretical value of −0.023 μas is shown with the red line.

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