Image Details
Caption: Figure 7.
The likelihood contours for the fit with a low-mass WD binary fraction of 7.5%. The 1σ and 2σ constraints on fbin,0.4 and α are shown in different shades. The contours are smoothed with a Gaussian filter. The black dotted lines represent the DWD merger rate per WD in the Galaxy, and the red dashed lines represent the number of super-Chandrasekhar-mass binaries in the Galaxy that can merge within the age of the Universe.
© 2026. The Author(s). Published by the American Astronomical Society.