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

377 citations · 740 across the 12 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…

gr-qc2023

Effects of spin-orbit coupling on gravitational waveforms from a triaxial non-aligned neutron star in a binary system

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

Spinning neutron stars (NSs) can emit continuous gravitational waves (GWs) that carry a wealth of information about the compact object. If such a signal is detected, it will provid…

astro-ph.HE2023★ 8 cited

Multi-messenger observations of double neutron stars in Galactic disk with gravitational and radio waves

Wen-Fan Feng, Jie-Wen Chen, Yan Wang +2

We evaluate the prospects for radio follow-up of the double neutron stars (DNSs) in the Galactic disk that could be detected through future space-borne gravitational wave (GW) dete…

gr-qc2020★ 377 cited

The TianQin project: current progress on science and technology

Jianwei Mei, Yan-Zheng Bai, Jiahui Bao +103

TianQin is a planned space-based gravitational wave (GW) observatory consisting of three earth orbiting satellites with an orbital radius of about . The satellites w…

astro-ph.HE2019★ 142 cited

Science with the TianQin observatory: Preliminary results on massive black hole binaries

Hai-Tian Wang, Zhen Jiang, Alberto Sesana +8

We investigate the prospects of detecting gravitational waves from coalescing massive black hole binaries in the Universe with the TianQin observatory, a space-based gravitational…

astro-ph.IM2019★ 71 cited

Preliminary study on parameter estimation accuracy of supermassive black hole binary inspirals for TianQin

Wen-Fan Feng, Hai-Tian Wang, Xin-Chun Hu +2

We use the Fisher information matrix method to calculate the parameter estimation accuracy of inspiraling supermassive black holes binaries for TianQin, a space-borne laser interfe…

gr-qc2018★ 138 cited

Fundamentals of the orbit and response for TianQin

Xin-Chun Hu, Xiao-Hong Li, Yan Wang +6

TianQin is a space-based laser interferometric gravitational wave detector aimed at detecting gravitational waves at low frequencies (0.1 mHz -- 1 Hz). It is formed by three identi…