Image Details
Caption: Figure 10.
Binned spin profiles of J0846 in 20 nonoverlapping portions of the 6.7-day beat cycle. The top of each panel indicates which beat phases were used to construct each spin profile. The data are repeated along the x-axis for clarity. The pole near spin phase 0.5 has an associated photometric maximum for most of the beat cycle, but it becomes indistinct near beat phase 0.8. Error bars are too small to be visible at this scale.
© 2023. The Author(s). Published by the American Astronomical Society.