Shulei Cao

most cited

H_{0} = 69.8 \pm 1.3

km s^{- 1} Mp c^{- 1}

Ω_{m 0} = 0.288 \pm 0.017

, and other constraints from lower-redshift, non-CMB, expansion-rate data

56 citations · 56 across the 2 of their papers we have counts for

collaborators

2 papers

astro-ph.CO2023

Cosmological constraints from standardized non-CMB observations

Shulei Cao

The current expansion of the Universe has been observed to be accelerating, and the widely accepted spatially-flat concordance model of general relativistic cosmology attributes th…

astro-ph.CO2023★ 56 cited

$H_{0} = 69.8 \pm 1.3$ $km s^{- 1} Mp c^{- 1}$ , $Ω_{m 0} = 0.288 \pm 0.017$ , and other constraints from lower-redshift, non-CMB, expansion-rate data

Shulei Cao, Bharat Ratra

We use updated Type Ia Pantheon+ supernova, baryon acoustic oscillation, and Hubble parameter (now also accounting for correlations) data, as well as new reverberation-measured C I…

Cosmological constraints from standardized non-CMB observations

H0​=69.8±1.3 km s−1 Mpc−1, Ωm0​=0.288±0.017, and other constraints from lower-redshift, non-CMB, expansion-rate data

$H_{0} = 69.8 \pm 1.3$ $km s^{- 1} Mp c^{- 1}$ , $Ω_{m 0} = 0.288 \pm 0.017$ , and other constraints from lower-redshift, non-CMB, expansion-rate data