most citedAdaptive Modeling of Correlated Noise in Space-Based Gravitational Wave Detectors

1 citations · 1 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2025

The impact of AGN environmental effects on testing general relativity with space-borne gravitational wave detector

Xiangyu Lyu, Hongyu Chen, En-Kun Li +1

The space-borne gravitational wave detectors such as TianQin offers a new window to test General Relativity by observing the early inspiral phase of stellar-mass binary black holes…

astro-ph.HE2025

Probing AGN Disks Density Profiles through Gravitational Wave Observations

Xiangyu Lyu, En-Kun Li, Changfu Shi +1

Massive black holes surrounded by a gaseous disk have been a prevailing model to explain a wide spectrum of astrophysical phenomena related to active galactic nucle (AGNs). However…

astro-ph.HE2025

Exploring the Link between Fast Radio Burst and Binary Neutron Star Origins with Spaceborne Gravitational Wave Observations

Yu-xuan Yin, En-kun Li, Bing Zhang +1

The origin of repeating Fast Radio Bursts (FRBs) is an open question, with observations suggesting that at least some are associated with old stellar populations. It has been propo…

astro-ph.IM20251 cited

Adaptive Modeling of Correlated Noise in Space-Based Gravitational Wave Detectors

Ya-Nan Li, Yi-Ming Hu, En-Kun Li

Accurately estimating the statistical properties of noise is important in data analysis for space-based gravitational wave detectors. Noise in different time-delay interferometry c…

gr-qc2025

Progress of the TianQin project

Jun Luo, Shaojun Bai, Yan-Zheng Bai +97

TianQin is a future space-based gravitational wave observatory targeting the frequency window of Hz Hz. A large variety of gravitational wave sources are expecte…

gr-qc2024

Mapping Anisotropies in the Stochastic Gravitational-Wave Background with TianQin

Zhi-Yuan Li, Zheng-Cheng Liang, En-Kun Li +2

In the milli-Hertz frequency band, stochastic gravitational-wave background can be composed of both astronomical and cosmological sources, both can be anisotropic. Numerically depi…