Figure 9 from A Technique to Derive Improved Proper Motions for Kepler Objects of Interest

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A Technique to Derive Improved Proper Motions for Kepler Objects of Interest

Authors: G. Fritz Benedict, Angelle M. Tanner, Phillip A. Cargile, and David R. Ciardi

Benedict et al. 2014 The Astronomical Journal 148 108.

Provider: AAS Journals

Caption: Figure 9.

x and y residuals as a function of time for the Q10-only four parameter modeling from Section 4.1. The residual clumps from left to right are "plates" 3–7, first seen in Figure 4. Stars are labeled with a running number from 1 to 97. The residuals exhibit far less time dependency. Stars 9 and 27 continue to exhibit unmodeled behavior.

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