Figure 5 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 5.

Top: star 27 (POSS-J on the left, 2MASS on the right) obviously with a close companion that confused the first-moment centering. Bottom: star 9, similarly illustrated. No companion to star 9 is detected. The positional shift is assumed to be instrumental.

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