Figure 2 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 2.

Linear mapping between M_K(0) and H_K(0) using HST parallaxes and proper motions for targets scattered over the entire sky. rms residual is 0.7 mag. The linear fit (M_K(0) = a + b H_K(0)) coefficient errors are 1σ. Stellar classifications range from white dwarfs to Cepheids, as listed in Table 1.

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