Frame-to-frame deviations in Decl of VB 10 from its model motion at zero (Ψ = 0, filled circles) and non-zero planetary signal (Ψ ≠ 0, open circles), the epoch average deviations (large diamonds), and the single-frame precisions σ1 (asterisks) for the cases a), b), and c) of reference field configurations shown in Fig.1.
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