activity
20162026
most citedDetermining the Hubble constant from Hubble parameter measurements

131 citations · 197 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2026

Redshift-Dependent Intrinsic Dispersion in the Quasar UV/X-ray Luminosity Relation

Jiaze Gao, Jianping Hu, Yun Chen +2

Accurate modeling of the intrinsic dispersion in the quasar UV/X-ray luminosity relation is essential for reliable cosmological inference. We investigate its redshift dependence us…

astro-ph.CO2023★ 5 cited

Cosmological application of the lens-redshift probability distribution with improved galaxy-scale gravitational lensing sample

Hui Li, Yun Chen

We conduct the cosmological analysis by using the lens-redshift distribution test with updated galaxy-scale strong lensing sample, where the considered scenarios involve three typi…

astro-ph.CO2021★ 4 cited

Diagnosing the cosmic coincidence problem and its evolution with recent observations

Jie Zheng, Yun Chen, Tengpeng Xu +1

In the framework of a phenomenological cosmological model with the assumption of ( and are the energy densities of dark energy and matter,…

astro-ph.CO2021★ 42 cited

Probing modified gravity theories with multiple measurements of high-redshift quasars

Yujie Lian, Shuo Cao, Marek Biesiada +3

In this paper, we quantify the ability of multiple measurements of high-redshift quasars (QSOs) to constrain several theories of modified gravity, including the Dvali-Gabadadze-Por…

astro-ph.CO2020★ 15 cited

Investigating the relationship between cosmic curvature and dark energy models with the latest supernova sample

Chao Gao, Yun Chen, Jie Zheng

We investigate the relationship between the cosmic curvature and the model of dark energy (hereafter DE) with the recent Type Ia supernovae (hereafter SNe Ia) data, i.e., the Panth…

astro-ph.CO2016★ 131 cited

Determining the Hubble constant from Hubble parameter measurements

Yun Chen, Suresh Kumar, Bharat Ratra

We use 28 Hubble parameter, , measurements at intermediate redshifts to determine the present-day Hubble constant in four cosmological models. We…