DESI measures BAO scales in six redshift bins with 0.52% combined precision using 5.7 million objects, detecting the signal at up to 9.1 sigma and finding larger scales than Planck LCDM at z<0.8.
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The matter power spectrum at z=0 inferred from DESI DR1 full-shape data is consistent with both LambdaCDM and w0waCDM when combined with CMB observations via EFT modeling.
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DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars
DESI measures BAO scales in six redshift bins with 0.52% combined precision using 5.7 million objects, detecting the signal at up to 9.1 sigma and finding larger scales than Planck LCDM at z<0.8.
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Inference of matter power spectrum at z=0 using DESI DR1 Full-Shape data
The matter power spectrum at z=0 inferred from DESI DR1 full-shape data is consistent with both LambdaCDM and w0waCDM when combined with CMB observations via EFT modeling.