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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 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.

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