DESI recovers the CMB-constrained parameter combination at sub-percent precision; high-redshift DES supernovae fit flat Lambda CDM while a 0.05 mag offset in the low-redshift anchor sample may be systematic, supporting overall model consistency from recombination to the local universe.
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6 Pith papers cite this work, alongside 55 external citations. Polarity classification is still indexing.
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A calibration of the Tully-Fisher relation using DESI Survey Validation data yields a slope of -7.96±0.13 and a zero-point of -19.34(+0.30,-0.29) AB mag, enabling a 1,136-galaxy peculiar velocity catalog.
A new density-momentum cross-power spectrum estimator applied to SDSSv yields f sigma8 = 0.413 +0.050 -0.058, consistent with GR plus Planck LCDM.
Cosmicflows-4 is broadly consistent with LambdaCDM, and the reported large-scale flow tension is a localized, window-dependent excess toward negative supergalactic X at 120 to 160 h^-1 Mpc.
Bulk flow measurements from Hawai`i Supernova Flows SNe Ia yield speeds of 100-400 km/s consistent with ΛCDM expectations at z ≲ 0.1.
citing papers explorer
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Consistency of DES and DESI distances and the Standard Cosmological Model
DESI recovers the CMB-constrained parameter combination at sub-percent precision; high-redshift DES supernovae fit flat Lambda CDM while a 0.05 mag offset in the low-redshift anchor sample may be systematic, supporting overall model consistency from recombination to the local universe.
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Cosmicflows-4 and the Cosmological Consistency of Large-Scale Motions
Cosmicflows-4 is broadly consistent with LambdaCDM, and the reported large-scale flow tension is a localized, window-dependent excess toward negative supergalactic X at 120 to 160 h^-1 Mpc.
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Hawai`i Supernova Flows: Bulk Flow Measurements using SNe Ia in the Optical and NIR
Bulk flow measurements from Hawai`i Supernova Flows SNe Ia yield speeds of 100-400 km/s consistent with ΛCDM expectations at z ≲ 0.1.
- A low value of $H_0$ in tension with the distance ladder from Megamasers using peculiar velocity reconstruction