Figure 7 from A Technique to Derive Improved Proper Motions for Kepler Objects of Interest

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 7.

Selected x residuals as a function of time for four parameter modeling (Equations (3) and (4)) of 127 stars in Channel 26 from Season 3, Quarter 5. The star numbers are identified with Kepler IDs in Table 2. Note that stars [4,..., 62] are more astrometrically stable than stars [67,..., 106].

Other Images in This Article

Copyright and Terms & Conditions