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Testing ΛCDM versus Dynamical Dark Energy in 1 Yr: A DESI Spectroscopic Follow-up Program for Rubin Supernovae

  • Authors: Jannik Truong, Greg Aldering, Saul Perlmutter, David Rubin, David Schlegel

Jannik Truong et al 2026 The Astrophysical Journal 1009 .

  • Provider: AAS Journals

Caption: Figure 1.

Reconstructed 1σ and 2σ Gaussian contours for w0 and wa from different datasets: Union3 (D. Rubin et al. 2025a) SNe Ia only (blue), DESI DR2 BAO+Planck CMB without SNe (green, M. Abdul Karim et al. 2025), and all three combined (orange). When combining all three datasets, ΛCDM (w0 = −1 and wa = 0, top left black point) is 3.8σ from the best-fit values. The combined error ellipse of large-scale structure probes is highly degenerate and points toward ΛCDM. SNe break this degeneracy and thus are an important probe for establishing a departure from ΛCDM.

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