Image Details
Caption: Figure 2.
This figure shows the posterior distributions of different planes of the (a) oΛCDM, (b) ωCDM, (c) oωCDM, (d) ω0ωaCDM, (e) logarithmic, (f) exponential, (g) JBP, (h) BA, and (i) GEDE models, obtained using DESI DR2 with CC measurements and different SNe Ia catalogs (Pantheon+, DES-Dovekie, and Union3), at the 68% (1σ) and 95% (2σ) confidence levels.
© 2026. The Author(s). Published by the American Astronomical Society.