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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 8.

Normalized K-band contrast curves for stars 4 and 67, along with average contrast curves for stars 4 through 62 (Good) and 67 through 106 (Bad). Note that while star 4 is more astrometrically stable than star 67, they have virtually identical contrast curves.

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