Image Details
Caption: Figure 3.
Dynamical dark-energy results for the two CMB treatments. The panels compare marginalized wDM posteriors for CMB-1000 (left) and the CMB lensing-marginalized likelihood (right). Unrestricted w0wa+wDM allows phantom crossing and is consistent with wDM = 0. The positive preference returns when crossing is forbidden, both for nonphantom w0wa+wDM and for Padé-w+wDM.
© 2026. The Author(s). Published by the American Astronomical Society.