Image Details
Caption: Figure 10.
Top: frequency scan of the angular evolution of the direction toward the DM offset. R 2 is the sum of the squared differences between the best-fit sinusoid of frequency ω and the angular position of the DM offset. Lower values of R 2 indicate a better fit, and the deep spike to R 2 < 1 at ~15 Gyr −1 corresponds to a periodicity of 69 Myr in the angular evolution. Bottom: the best-fitting sinusoid (red) overplotted on angular position of the DM offset in the last 22 outputs.
© 2013. The American Astronomical Society. All rights reserved.