Fig. 1.

Simulation of the astrometric model response to a step change U(y) in the position of chip 2 for the example sky field of dw14 offset by 73 px from the detector center. Dots show the response in the epoch residuals of reference stars, and the function WRF is the smoothed response in proper motions to the step change of proper motions of chip 2 stars. The function WCAL is the same, but for the reference stars distributed evenly over FoV.
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