Figure 10 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 10.

Histograms of x and y residuals for the Q10-only four parameter modeling of only plates 3–7 (Figure 9) from Section 4.1. The residuals are well characterized with Gaussians with 1σ dispersions as indicated.

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