Individual exclusions and matter priors
Individual run · T-8ccc2db2fe00
Public summary of an internal test, not yet independently validated or published.
Question investigated
In Pantheon+ and Union3, with Ωm = 0.315 ± 0.007, does the preference for dynamical dark energy persist after the separate exclusion of the low- and high-redshift BAO groups?
Test conditions
Refit Pantheon+ and Union3 after excluding, one at a time, the 2 DESI BAO groups at z = (0.295, 0.51, 0.706); (0.934, 1.321, 1.484, 2.33). Hold the supernova data and cosmic microwave background constraints fixed. Adopt Ωm = 0.315 ± 0.007. Compare fit quality and shifts in the dark-energy parameters.
Result
The group exclusions produced unequal responses in the fit. The comparison established neither independence of the preference from every group nor exclusive dependence on any one group.
Physical interpretation
This test measures how much each BAO tracer group contributes to the cosmological preference. Sensitivity to a group alone does not identify its physical or observational cause.