most citedGravitational wave standard sirens: A brief review of cosmological parameter estimation

10 citations · 10 across the 3 of their papers we have counts for

collaborators

5 papers

gr-qc2026

Two-Dimensional Pulsar Distance Inference from Nanohertz Gravitational Waves

Si-Ren Xiao, Ji-Yu Song, Yue Shao +3

Pulsar timing arrays (PTAs) are limited in localizing nanohertz continuous gravitational waves (CGWs) by uncertainties in pulsar distances. We introduce a method to infer pulsar di…

astro-ph.CO2026

Three-band dark-siren cosmology with intermediate-mass black hole binaries: synergy of Taiji, LGWA, and Einstein Telescope

Ji-Yu Song, Yue-Yan Dong, Shang-Jie Jin +3

Gravitational-wave (GW) dark sirens provide an independent probe of the cosmic expansion history. Their cosmological constraining power, however, depends critically on precise lumi…

astro-ph.CO202610 cited

Gravitational wave standard sirens: A brief review of cosmological parameter estimation

Shang-Jie Jin, Ji-Yu Song, Tian-Yang Sun +5

Gravitational wave (GW) observations are expected to serve as a powerful and independent probe of the expansion history of the universe. By providing direct and calibration-free me…

astro-ph.CO2025

Ultra-low-frequency gravitational waves from individual supermassive black hole binaries as standard sirens

Ling-Feng Wang, Yue Shao, Si-Ren Xiao +2

Ultra-low-frequency gravitational waves (GWs) generated by individual inspiraling supermassive black hole binaries (SMBHBs) at the centers of galaxies may be detected by pulsar tim…

astro-ph.CO2025

Nanohertz gravitational waves from a quasar-based supermassive black hole binary population model as dark sirens

Si-Ren Xiao, Yue Shao, Ling-Feng Wang +4

Recently, several pulsar timing array (PTA) projects have detected evidence of the existence of a stochastic gravitational wave background (SGWB) in the nanohertz frequency band, p…