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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 19.

Distance from ΛCDM in σ (left) and DETF FoM (right) as a function of the assumed zero-point calibration prior and gray dispersion—the two dominant systematics most likely to improve in the near future. Values in parentheses correspond to forecasts without a separate sample of new low-z SN. The 5σ threshold is reached or exceeded across a wide range of assumed priors. Neither systematic alone drives the final constraints.

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