Figure 13 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 13.

Average vector residuals in milliarcseconds as a function of position within Channel 21 from the full Schmidt 14 parameter modeling of three Season 0 observation sets described in Section 5.3. Other than a strong tendency for larger residuals in the y direction, the pattern is satisfactorily random.

Other Images in This Article

Copyright and Terms & Conditions