Image Details
Caption: Figure 4.
Distance of DESI DR2+Planck+Union3 best-fit from ΛCDM given by the number of standard deviations, and FoM when adding SNe at one redshift bin z with different total uncertainties to DESI DR2+Planck+Union3 and low-z SNe. Total uncertainties include statistical and systematic errors, although statistical errors typically become subdominant for 103 to 104 SNe Ia. We find that measuring around z ≈ 0.6 increases the distance from ΛCDM and the FoM most.
© 2026. The Author(s). Published by the American Astronomical Society.