Figure 9 from Asteroseismic Determination of Obliquities of the Exoplanet Systems Kepler-50 and Kepler-65

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Asteroseismic Determination of Obliquities of the Exoplanet Systems Kepler-50 and Kepler-65

Authors: W. J. Chaplin, R. Sanchis-Ojeda, T. L. Campante, R. Handberg, D. Stello, J. N. Winn, S. Basu, J. Christensen-Dalsgaard, G. R. Davies, T. S. Metcalfe, L. A. Buchhave, D. A. Fischer, T. R. Bedding, W. D. Cochran, Y. Elsworth, R. L. Gilliland, S. Hekker, D. Huber, H. Isaacson, C. Karoff, S. D. Kawaler, H. Kjeldsen, D. W. Latham, M. N. Lund, M. Lundkvist, G. W. Marcy, A. Miglio, T. Barclay, and J. J. Lissauer

Chaplin et al. 2013 The Astrophysical Journal 766 101.

Provider: AAS Journals

Caption: Figure 9.

Asteroseismic results on Kepler-50. Lower left-hand panel: correlation map in angle of inclination i _s and rotational frequency splitting δν _s (highest likelihoods rendered in red). Top and right-hand panels: PDFs obtained after marginalization. Note that the PDFs are normalized so that the integral under each curve is unity. Bold crosses mark the final parameter estimates given in Table 4.

Other Images in This Article

Copyright and Terms & Conditions