activity
20182026
most citedThe TianQin project: current progress on science and technology

377 citations · 460 across the 10 of their papers we have counts for

collaborators

12 papers

astro-ph.CO2026

Measuring the Hubble constant with strongly lensed gravitational waves from space-based detector networks

Yong Yuan, Minghui Du, Wen-Fan Feng +4

The measurement of the Hubble constant plays a central role in modern cosmology. In this work, we investigate the potential of strongly lensed gravitational-wave (SLGW) signa…

astro-ph.GA2026

Bayesian Analysis of Gravitational Wave Microlensing Effects from Galactic Double White Dwarfs

Yan Sun, Yong Yuan, Minghui Du +3

Gravitational waves (GWs) from the galactic double white dwarf (DWD) systems are one of the primary targets for upcoming space-based detectors. Due to their vast abundance and wide…

gr-qc2025★ 1 cited

Influence of cosmic expansion on gravitational waveforms

Tan Liu, Wen-Fan Feng, Zong-Kuan Guo

Gravitational waves undergo redshift as they propagate through the expanding universe, and the redshift may exhibit time-dependent drift. Consequently, for any isolated gravitation…

gr-qc2025★ 1 cited

Galactic double neutron stars as dual-line gravitational-wave sources: Prospects with LISA and Cosmic Explorer

Wen-Fan Feng, Lijing Shao

Double neutron star (DNS) systems could serve as intriguing dual-line gravitational-wave (GW) sources, emitting both high- and low-frequency GWs, arising respectively from the asym…

gr-qc2024★ 2 cited

Effects of orbital eccentricity on continuous gravitational waveforms from triaxially deformed precessing neutron stars in tight binaries

Wen-Fan Feng, Tan Liu, Yan Wang +1

The successful detection of continuous gravitational waves from spinning neutron stars (NSs) will shape our understanding of the physical properties of dense matter under extreme c…

astro-ph.HE2024

Inferring binary parameters with dual-line gravitational wave detection from tight inspiraling double neutron stars

Wen-Fan Feng, Jie-Wen Chen, Tan Liu +2

Neutron star (NS) binaries can be potentially intriguing gravitational wave (GW) sources, with both high- and low-frequency radiations from the possibly aspherical individual stars…